the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Relativistic Kinematic Effects in the Interaction Time of WhistlerMode Chorus Waves and Electrons in the Outer Radiation Belt
Livia R. Alves
Marcio E. S. Alves
Ligia A. da Silva
Vinicius Deggeroni
Paulo R. Jauer
David G. Sibeck
Abstract. Whistlermode chorus waves propagate outside the plasmasphere. As they interact with energetic electrons in the outer radiation belt electrons, the phase space density distribution can change due to energy or pitch angle diffusion. Calculating the waveparticle interaction time is crucial to estimate the particle’s energy or pitch angle change efficiently. Although the wave and particle velocities are a fraction of the speed of light, in calculating the interaction time, the special relativistic effects are often misleading, incomplete, or simply unconsidered. In this work, we derive an equation for the waveparticle interaction time considering the special relativity kinematic effect. We solve the equation considering typical magnetospheric plasma parameters, and compare the results with the nonrelativistic calculations. Besides, we apply the methodology and the equation to calculate the interaction time for one wave cycle in four case studies. We consider waveparticle resonance conditions for chorus waves propagating at any wave normal angle in a dispersive and cold plasma. We use Van Allen Probes for in situ measurements of the relevant wave parameters for the calculation, the ambient magnetic field, and energetic electron flux under quiet and disturbed geomagnetic conditions. Thus, we use a test particle approach to calculate the interaction time for parallel and oblique propagating waves. Also, we evaluate the variation of pitch angle scattering for relativistic electrons interacting with whistlermode chorus waves propagating parallel to the ambient magnetic field. If the relativistic effects are not taken into account, the interaction time can be ∼ 30 % lower for quiet periods and a half lower for disturbed periods. As a consequence, the change in pitch angle is also underestimated. Besides, the longest interaction time occurs at waveparticle interaction with high pitch angle electrons, with energy ∼ 100′ s of keV, interacting with quasiparallel propagating waves. Additionally, the change in pitch angle depends on the time of interaction, and similar discrepancies can be found when the time is calculated with no special relativity consideration. The results described here have several implications for modeling relativistic outer radiation belt electron flux resulting from the waveparticle interaction. Finally, since we considered only one wavecycle interaction, the average result from some interactions can bring more confident results in the final flux modeling.
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Livia R. Alves et al.
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RC1: 'Comment on angeo20236', Anonymous Referee #1, 28 Mar 2023
General
This draft presents calculations regarding the interaction time for electrons with chorus waves, and the resultant effect on pitch angle transport (“delta alpha”). The main proposed contribution is that the calculation is presented as being consistent with special relativity. Impicitly, the reader is to assume that this is being performed for the first time in the literature.
I believe that the basic principle of the work presented in this draft is sound, and potentially important. Although I do have a major concern regarding the assumption of an inertial satellite frame of reference
Even if that major concern is cleared up, I believe that further major revisions are necessary before publication can be recommended.
These revisions mostly centre around
 Calculations – I have some serious questions regarding some of the calculations. Or clarifications that need to be made regarding the validity of the results
 Data – I do not see what significant value the presented Van Allen Probes data adds, for the manuscript in the current form. More work needs to be done, I would suggest.
 Context – we need much more justification and references to literature. And discussion.
Major comments
Calculations
1. All of the calculations rely on the comparisons of inertial frames of reference. Does a satellite have an inertial frame?
Not only is the satellite orbiting the Earth (and therefore undergoing acceleration), but it is also rotating around its own axis (and as a result so are the devices that measure BuBvBw etc). Please clarify. We need to have absolute clarity on this. Please can the authors give a thorough justification to explain why this is a reasonable approach. How are the inertial frames constructed and justified, given the above mentioned 2 sources of acceleration?
Relatedly, if there is a justification for this, we sould strongly suggest that the authors make a diagram that illustrates what S, S’, and the different relativistic considerations are regarding the wave and the satellite, in order to help the reader understand what is going on
2. e.g. going from equations 14 to 20, and in particular 19 to 20
All of this analysis assumes that
 the forces on the particle are constant during the timescale 0
 It also assumes that T is determined by some version of “T=X/V” (e.g equation 10 from Lakhina et al 2010), or a relativistic version equation 13 in this paper.
Both of these are quite restrictive approximations, although we accept that they are relatively standard methods that are used in the literature e.g. Kennel&Petschek 1966, Lakhina et al 2010 as cited by the authors. The approximations are as follows.
 The presented equations are a big approximation to the real answer, which requires the solution of coupled first order odes for gyrophase, pitch angle, energy, position (e.g. see exact solutions up to second order in Bwave/B0 in Allanson et al 2022 Front. Astron. Space Sci. 8:805699. doi:10.3389/fspas.2021.805699)
 the interaction time could be shorter than this if the particle is scattered away very quickly. Likewise it could be longer if the particle is trapped (e.g. see Bortnik et al 2008 GEOPHYSICAL RESEARCH LETTERS, VOL. 35, L21102, doi:10.1029/2008GL035500, 2008)
Therefore it is important to state these approximations, and to say that the answers could be very different if (i) and (ii) play an important role, e.g. for higher amplitude/nonlinear waves. Conversely, the results in this paper are probably only true for a quasilinear interaction (e.g. Kennel and Engelmann 1966 The Physics of Fluids 9, 2377 (1966).
3. Equation (3) in the manuscript is incorrect. E.g. see
Equation (1) in Lakhina et al 2010
Or equation (13) in Artemyev et al Space Sci Rev (2016) 200:261–355 DOI 10.1007/s1121401602525
or equation 1 in Shprits et al Journal ofAtmosphericandSolarTerrestrialPhysics70(2008)1694–1713
It should only be k_parallel and v_parallel in the doppler shift. The velocity component of interest is
v_parallel = v*cos\alpha
Therefore there are a range of speeds (v) and pitch angles (\alpha) that are resonant with any given wave frequency \omega. E.g.
see equations 151 and 152 from Omura Earth, Planets and Space (2021) 73:95.
Therefore equation 4 not quite correct. This could have serious implications for the rest of the draft? The point is that there are many different values of energy that can resonate with a given wave, and these are a function of pitchangle, e.g. see an example for the n=1 resonance in
Camporeale, E. (2015), Resonant and nonresonant whistlersparticle interaction in the radiation belts, Geophys. Res. Lett., 42, 3114–3121, doi:10.1002/2015GL063874.
Data
4. Case studies 1, 2 and 3 all have magnetic field wave amplitudes >= 1nT (see table 1). With B0 roughly 100nT. That gives Bw/B0 ~ 1/100. These are very intense waves and almost certainly fall into the nonlinear regime (e.g. phase trapping and phase bunching etc) e.g. see
Zhang et al JGR, 2018, 123, 5379–5393, https://doi.org/10.1029/2018JA025390 and
Zhang et al GRL, 2019, 46, 7182–7190. https://doi.org/10.1029/2019GL083833
As per the above comment (2), I question whether interaction time method described in the paper is applicable. Or to put it another way, I would need to be convinced – please!
5. implications of point 3 regarding resonant particles. There is not one single resonant energy. There is a single resonant v_parallel for a given value of n, but this corresponds to many energies and pitchangles. Therefore we do not understand figure 2 as it is currently presented, or any results or discussion that make use of the results from equation 5, and discussions about the given value of resonant energy
6. Lines 208 – 267: There is a lengthy description of some Van Allen Probes data here. But none of it really adds any genuine value to the manuscript in our opinion. From line 268 onwards there is a discussion of some parameters that are used and calculated for the interaction time. But that information is not really linked scientifically to the discussion of the data in lines 208267, except in a very superficial way. What are the implications of one on the other? What is the importance of the results and how does it related to the data? What new inferences can we make because of the data in the table etc? What might this show us in the Van Allen Probes data etc?
Context/References/Discussion
7. ~line 50: The authors claim that the relativistic approach is often simplified or misused, but they provide no references or discussion to support this claim. Please provide references and much more discussion! This is the foundation of the motivation for the paper. We suggest that there needs to be a much more thorough justification and motivation in the introduction of this draft
8. Line 69: Appleton/Hartree equation: please provide a citation and a justification for why this is the correct relation to use
9. Equation (20) How does the presented formula for \Delta\alpha compare to those presented in e.g. papers by Lakhina et al 2010, Tsurutani & Lakhina 1997, Kennel&Petschek66 and Allanson et al 2022? What differences has it made to include relativity, and what differences are observed because the integration was performed approximately and not exactly?
10. Lines 280 onwards: There is no meaningful discussion section. Section 5 has some conclusions. But the authors have not contextualised their work in detail with respect to previous results in the literature. This is an important missing piece of the draft and we would suggest needs to be fixed. Furthermore, now that we have these new estimates, how could they be used in practice by scientists in the future?
Technical
11. line 5 (“wave velocity”): is this group or phase velocity?
12. Line 15 (“interaction time can be ~30% lower for quiet periods”): we are not sure that it is appropriate to characterise things in this way. The authors have performed a small subset of case studies. Also, the details of the interaction time are fundamentally related to the microphysics of the waveparticle interaction, and not really whether it is an active or quiet period. Perhaps it is best not to phrase things in this way.
13. Line 99: The Shprits 2008 paper cited is a paper about radial diffusion. You should replace this with a local diffusion paper by Shprits in the same series in JASTP
14. Line 134: “wellknown formula of the addition of velocities”. What is this formula? Please provide the formula and a citation
15. Equation 18: the authors use \Delta on the LHS but “d” on the RHS for infinitesimal changes. They should either use one or the other, and be consistent on both sides of the equation.
Citation: https://doi.org/10.5194/angeo20236RC1 
AC2: 'Reply on RC1', Livia R. Alves, 10 May 2023
The authors appreciate all suggestions given by Reviewers 1 and 2, which were essential to improve this article. A careful revision was carried out in the manuscript taking into account all the comments and suggestions. The figures and Table 1, mentioned in the response, are available in the attached file (Figures_Table_response_to_reviewers.pdf).
Major comments
Calculations
 All of the calculations rely on the comparisons of inertial frames of reference. Does a satellite have an inertial frame?
Not only is the satellite orbiting the Earth (and therefore undergoing acceleration), but it is also rotating around its own axis (and as a result so are the devices that measure BuBvBw etc). Please clarify. We need to have absolute clarity on this. Please can the authors give a thorough justification to explain why this is a reasonable approach. How are the inertial frames constructed and justified, given the above mentioned 2 sources of acceleration?
We add the discussion below in lines 147154:
To justify the use of an inertial frame associated with the satellite, consider, for instance, the maximum acceleration achieved by the satellite at the perigee (data from satellite orbit can be found e.g. at Mauk et al., 2013), $8.2~{\rm m}{\rm s}^{2}$. The interaction time between the electron and the wave is of the order of $10^{3}$ s. Since the period of the satellite is $537.1$ min, its acceleration is nearly constant during the interaction. Therefore, the change in the speed of the satellite in its orbit during one interaction time is around $8.2 \times 10^{3}~{\rm m}/{\rm s}$ which is 6 orders of magnitude smaller than the speed of the satellite at the perigee 9,8 km/s. Similarly, the spin period of the satellite is 11 s (Breneman et al., 2022), which leads to a change in angle of about $1.8~{\rm arcmin}$ in one interaction time. Thus, for the purposes of the present article, it is reasonable to consider the satellite as an inertial reference frame during one interaction time. Moreover, it is a standard approach in the literature to consider the satellite as an inertial reference frame.
Breneman, A.W., Wygant, J.R., Tian, S. et al. The Van Allen Probes Electric Field and Waves Instrument: Science Results, Measurements, and Access to Data. Space Sci Rev 218, 69 (2022). https://doi.org/10.1007/s1121402200934y)
Mauk, B.H., Fox, N.J., Kanekal, S.G. et al. Science Objectives and Rationale for the Radiation Belt Storm Probes Mission. Space Sci Rev 179, 3–27 (2013). https://doi.org/10.1007/s112140129908y
Relatedly, if there is a justification for this, we sould strongly suggest that the authors make a diagram that illustrates what S, S’, and the different relativistic considerations are regarding the wave and the satellite, in order to help the reader understand what is going on
Resp.: The diagram was included in the manuscript as Figure 3
 e.g. going from equations 14 to 20, and in particular 19 to 20
All of this analysis assumes that
 the forces on the particle are constant during the timescale 0
 It also assumes that T is determined by some version of “T=X/V” (e.g equation 10 from Lakhina et al 2010), or a relativistic version equation 13 in this paper.
Both of these are quite restrictive approximations, although we accept that they are relatively standard methods that are used in the literature e.g. Kennel&Petschek 1966, Lakhina et al 2010 as cited by the authors. The approximations are as follows.
 e.g. going from equations 14 to 20, and in particular 19 to 20
All of this analysis assumes that
 the forces on the particle are constant during the timescale 0
 It also assumes that T is determined by some version of “T=X/V” (e.g equation 10 from Lakhina et al 2010), or a relativistic version equation 13 in this paper.
Both of these are quite restrictive approximations, although we accept that they are relatively standard methods that are used in the literature e.g. Kennel&Petschek 1966, Lakhina et al 2010 as cited by the authors. The approximations are as follows.
 The presented equations are a big approximation to the real answer, which requires the solution of coupled first order odes for gyrophase, pitch angle, energy, position (e.g. see exact solutions up to second order in Bwave/B0 in Allanson et al 2022 Front. Astron. Space Sci. 8:805699. doi:10.3389/fspas.2021.805699)
 the interaction time could be shorter than this if the particle is scattered away very quickly. Likewise it could be longer if the particle is trapped (e.g. see Bortnik et al 2008 GEOPHYSICAL RESEARCH LETTERS, VOL. 35, L21102, doi:10.1029/2008GL035500, 2008)
Therefore it is important to state these approximations, and to say that the answers could be very different if (i) and (ii) play an important role, e.g. for higher amplitude/nonlinear waves. Conversely, the results in this paper are probably only true for a quasilinear interaction (e.g. Kennel and Engelmann 1966 The Physics of Fluids 9, 2377 (1966).
Resp.: We thank the referee for this suggestion, and we include the following paragraph in the manuscript (lines 234241 and 337348):
The manuscript aims to improve the calculation of the interaction time in the quasilinear waveparticle interaction regime. Thus, we use firstorder solutions such as those done by Lakhina and Tsurutani, 2010. The weak turbulence in plasma and nonlinear events occurrence rate is around 10 to 15% considering the average occurrence of whistlermode chorus waves (Zhang et al., 2018). These events have a solution of the waveparticle interaction equation are based on, at least, secondorder terms in wave amplitude, e.g., Allanson et al., 2022; Artemyev et al., 2023; Omura, 2021; Osmane et al., 2016; Bortnik et al., 2008).
There are several difficulties in calculating the trapping time in nonlinear interactions (e.g., eq. (87) Omura, 2021, Omura et al., 2013, Omura et al., 2008) using in situ measurements. Though, the firstorder approach can give approximate solutions to nonlinear regimes, and Equation (13) can be used to estimate the interaction time from insitu measurements (e.g., Hsieh et al., 2021) since it is important to determine the energy gain of electrons undergoing a waveparticle interaction (Hsieh et al., 2021). However, the interaction time is known to be shorter than the trapping time (Hsieh et al., 2021; Bortnik et al., 2008)
Anton V. Artemyev, Jay M. Albert, Anatoli I. Neishtadt, Didier Mourenas; The effect of wave frequency drift on the electron nonlinear resonant interaction with whistlermode waves. Physics of Plasmas 1 January 2023; 30 (1): 012901. https://doi.org/10.1063/5.0131297
Omura, Y., Katoh, Y., and Summers, D. (2008), Theory and simulation of the generation of whistlermode chorus, J. Geophys. Res., 113, A04223, doi:10.1029/2007JA012622.
Osmane, A., Wilson, L. B., Blum, L., Pulkkinen, T. I. (2016), On The Connection Between Microbursts And Nonlinear Electronic Structures In Planetary Radiation Belts. The Astrophysical Journal, ApJ 816 51, https://dx.doi.org/10.3847/0004637X/816/2/51
Allanson, O., Thomas, E., Clare, W., Thomas, N. (2022), Weak Turbulence and Quasilinear Diffusion for Relativistic WaveParticle Interactions Via a Markov Approach. Front. Astron. Space Sci. 8:805699. doi:10.3389/fspas.2021.805699
Bortnik, J., Thorne, R. M., and Inan, U. S. (2008), Nonlinear interaction of energetic electrons with large amplitude chorus, Geophys. Res. Lett., 35, L21102, doi:10.1029/2008GL035500.
Zhang, J., Thorne, R., Artemyev, A., Mourenas, D., Angelopoulos, V., Bortnik, J., Kletzing, C. A., Kurth, W. S., & Hospodarsky, G. B. (2018). Properties of Intense FieldAligned LowerBand Chorus Waves: Implications for Nonlinear WaveParticle Interactions. Journal of Geophysical Research: Space Physics, 123(7), 53795393. https://doi.org/10.1029/2018JA025390
 Equation (3) in the manuscript is incorrect. E.g. see
Equation (1) in Lakhina et al 2010
Or equation (13) in Artemyev et al Space Sci Rev (2016) 200:261–355 DOI 10.1007/s1121401602525
or equation 1 in Shprits et al Journal ofAtmosphericandSolarTerrestrialPhysics70(2008)1694–1713
It should only be k_parallel and v_parallel in the doppler shift. The velocity component of interest is
v_parallel = v*cos\alpha
Resp.: We thank the referee for this point. In the manuscript, we write Equation (3) as a general equation for the Doppler shift in the wave frequency. We explain in lines 113115 that we are considering the wave vector parallel to the ambient magnetic field for the wave's direction being copropagating and counterpropagating to the energetic electron. In this case, the equatorial electron pitch angle \alpha used in equation (3) will be the same as done by Lakhina et al., 2020, Artemyev et al., 2016, and Camporeale (2015).
We call \delta the angle between the wave vector and the electron velocity vector. This correction was included in equation (4) and lines 118119. Also, Figure 2 was corrected, and the discussion was added in lines 128131.
Therefore there are a range of speeds (v) and pitch angles (\alpha) that are resonant with any given wave frequency \omega. E.g.
see equations 151 and 152 from Omura Earth, Planets and Space (2021) 73:95.
Resp.: Yes, we agree, and this is shown by the n (harmonic number) in Eq. (4) in the submitted manuscript.
Therefore equation 4 not quite correct. This could have serious implications for the rest of the draft?
Resp: Equation (4) was corrected by changing the angle between the electron velocity vector and the wave normal angle as \delta; both vectors' orientations are defined as related to the ambient magnetic field in a tridimensional coordinate system. In the manuscript, we solve Eq. (4) for \delta equals \alpha and \pi  \alpha for copropagating and counterpropagating waves, respectively. In such an approach, both resonant and perpendicular components of the electron velocity vector are considered in the calculation, similar to that done by Summers et al., 2012.
The point is that there are many different values of energy that can resonate with a given wave, and these are a function of pitchangle, e.g. see an example for the n=1 resonance in
Camporeale, E. (2015), Resonant and nonresonant whistlersparticle interaction in the radiation belts, Geophys. Res. Lett., 42, 3114–3121, doi:10.1002/2015GL063874.
Resp.: We agree with the referee that there are many different energies resonating with a given wave frequency, since we have the possibility to match several harmonics with the same wave; besides, for parallel propagating whistler waves, the angle between the wave vector and electron speed vector coincides with the electron's pitch angle, as shown by Camporeale, E. 2015. This information and reference were added in the manuscript in lines 129131.
Data
 Case studies 1, 2 and 3 all have magnetic field wave amplitudes >= 1nT (see table 1). With B0 roughly 100nT. That gives Bw/B0 ~ 1/100. These are very intense waves and almost certainly fall into the nonlinear regime (e.g. phase trapping and phase bunching etc) e.g. see
Zhang et al JGR, 2018, 123, 5379–5393, https://doi.org/10.1029/2018JA025390 and
Zhang et al GRL, 2019, 46, 7182–7190. https://doi.org/10.1029/2019GL083833
As per the above comment (2), I question whether interaction time method described in the paper is applicable. Or to put it another way, I would need to be convinced – please!
Resp: We thank the referee for this point, and we clarify that the interaction time calculated in this manuscript accounts for the firstorder cyclotron effect only. We included the citation of Hsieh et al., 2020 and 2017; Omura, 2021, Omura et al., 2013; Omura et al., 2008 to show an example in the literature of the interaction time in nonlinear cases. In addition, we changed the case studies presented in Table 1 to apply the derived equations to the linear waveparticle cases. Also, Figures 6, 7, D1, and E1 were updated.
Hsieh, Y.K., and Omura, Y. (2017), Nonlinear dynamics of electrons interacting with oblique whistlermode chorus in the magnetosphere, J. Geophys. Res. Space Physics, 122, 675– 694, doi:10.1002/2016JA023255.
 implications of point 3 regarding resonant particles. There is not one single resonant energy. There is a single resonant v_parallel for a given value of n, but this corresponds to many energies and pitchangles. Therefore we do not understand figure 2 as it is currently presented, or any results or discussion that make use of the results from equation 5, and discussions about the given value of resonant energy
Resp.: Figure (2) was corrected for the angle between the wave vector and electron velocity vector. Figure (2) is an example of Eq. (5) for a given ambient plasma parameters, wave normal angle, equatorial electron pitch angle, and one harmonic number. It is shown to give an example of how the resonant electron kinetic energy varies as a function of the wave frequency, for waves propagating parallel and oblique to the ambient magnetic field. Accordingly, if the harmonic number n is changed, all the curves would be shifted to the higher wave frequency side. We inserted a sentence about this point in line 128.
 Lines 208 – 267: There is a lengthy description of some Van Allen Probes data here. But none of it really adds any genuine value to the manuscript in our opinion. From line 268 onwards there is a discussion of some parameters that are used and calculated for the interaction time. But that information is not really linked scientifically to the discussion of the data in lines 208267, except in a very superficial way. What are the implications of one on the other? What is the importance of the results and how does it related to the data? What new inferences can we make because of the data in the table etc? What might this show us in the Van Allen Probes data etc?
Resp.: We apologize if we were not clear. Section 4 was revised and split to organize the dataset in a subsection (starting in line 246).
Using Van Allen Probes data, it is possible to identify the periods of the highenergy electron flux dropouts and enhancements in the outer radiation belt concomitant with whistlermode chorus wave activities for each case study shown in Table 1. It suggests that the resonance between the chorus waves and particles may have locally contributed to this electron flux variability.
To clarify the importance of the discussions about the PSD in this article, we decided to write a new paragraph before line 208 and rewrote the discussions about Figures 5.1, A1.1 e B1.1, as described below:
Figures 5.1, A1.1 e B1.1 shows the time evolution of the radial PSD profiles at inbound/outbound regions of Van Allen Probe B, which allows the identification of the local relativistic electron loss and/or local lowenergy acceleration in the outer radiation belt. The pitch angle diffusion mechanism driven by whistler mode chorus waves can cause this kind of local electron flux loss/acceleration, in which the local (L*), order of magnitude, and energy level are identified at the same period analyzed in previous sections.
Reference:
Tsyganenko, N. A., & Sitnov, M. I. (2005). Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms. Journal of Geophysical Research, 110, A03208. https://doi.org/10.1029/2004JA010798
Context/References/Discussion
 ~line 50: The authors claim that the relativistic approach is often simplified or misused, but they provide no references or discussion to support this claim. Please provide references and much more discussion! This is the foundation of the motivation for the paper. We suggest that there needs to be a much more thorough justification and motivation in the introduction of this draft
Resp.: We include the discussion and references related to the motivation and justification of the paper in lines 45  66:
In the magnetosphere, the kinematics description of the waveparticle interaction for relativistic electrons usually considers the relativistic Doppler shift in the resonance condition (e.g., Thorne et al. 2005, Summers et al. 1998) and the relativistic motion equation (e.g., Omura, 2021). Often, the resonant kinetic energy of the electrons results from the resonance condition and the motion equation, together with the wave group velocity (e.g., Omura 2021, Hsieh et al., 2021, Summers et al., 2012, Glauer et al., 2005, Lyons et al., 1972). The waveparticle interaction time ($T_r$) is a crucial parameter in estimating timedependent processes as the energy and pitch angle diffusion coefficients \citep{walker1993, lakhina2010, tsurutani2013, hsieh2020, hsieh2022}, however, the relativistic kinematics description mentioned above is incomplete to calculate this parameter. In this paper, we add to the latter approach a complete relativistic description of the problem: the relativistic velocity addition (between the electron and the wave) and the implications of the different reference frames in the estimates of the change in pitch angle and the diffusion coefficient.
We calculate the parameters for four case studies to give a quantitative comparison between the complete relativistic description and a nonrelativistic approach (used here as an approximation to calculate the interaction parameters). The interaction time is calculated using the test particle equations \citep{tsurutani1974, lakhina2010, horne2003b, bortnik2008} along with the special relativity theory applied to whistlermode chorus waves propagating in cold plasma magnetosphere (where group velocity is $~0.3c$ to $0.5 c$) and energetic electrons (with energy $ \sim 0.1$ to $2$ MeV). We consider that the resonance occurs in the electron's reference frame. At the same time, the result of such interaction and their parameters are measured in the local inertial reference frame of the satellite.
We considered parallel propagating whistlermode chorus waves linearly interacting with relativistic electrons to derive first the group velocity equation, then the resonant relativistic kinetic energy, and finally the interaction time. Thus, we calculate the change pitch angle and the diffusion coefficient rates. We use the Van Allen Probes measurement of wave parameters, ambient magnetic field, density, electron fluxes, and equatorial pitch angle to apply the interaction time equation.
A complete calculation of these parameters can improve relativistic outer radiation belt electron flux variation models.
 Line 69: Appleton/Hartree equation: please provide a citation and a justification for why this is the correct relation to use
Resp.: We add the following justification and reference in lines 7881: whistler mode chorus waves which occur in frequencies higher than the ion cyclotron frequency, besides the waveparticle interaction outside the plasmasphere, the dispersion relation for this case is obtained from the solution of the AppletonHartree equation \citep{bittencourt2004}.
 Equation (20) How does the presented formula for \Delta\alpha compare to those presented in e.g. papers by Lakhina et al 2010, Tsurutani & Lakhina 1997, Kennel&Petschek66 and Allanson et al 2022? What differences has it made to include relativity, and what differences are observed because the integration was performed approximately and not exactly?
Resp.: The change in pitch angle for nonrelativistic electrons due to waveparticle interaction in a quasilinear regime is given by equations (3.6) in Kennel and Petschek, 1966, and (11) in Tsurutani and Lakhina, 1997. Lakhina et al., 2010, derived equation (11) by considering the relativistic resonant condition and the nonrelativistic equation of motion. Allanson et al., 2022, show the exact equation for pitch angle scattering and secondorder equations for weak turbulence and nonlinear regimes.
In this manuscript, the change in pitch angle is given by equation (20), which is consistent with equations (3.6) in Kennel and Petschek, 1966; (11) in Tsurutani and Lakhina, 1997 and equation (11) in Lakhina et al., 2010. In the limit that \gamma ~ 1, for nonrelativistic electrons, Tr equals to \delta t (in Kennel and Petschek, 1966 and Tsurutani and Lakhina, 1997) or to \tau in (Lakhina et al., 2010). Also, Equation (20) in this manuscript is similar to Equation (S3) in Allanson et al., 2021.
The main difference we observe using a more complete relativity description is that the interaction time is often longer than that calculated with a nonrelativistic description, as shown in Table 1. The consequence of underestimating the interaction time is that diffusion coefficients are also underestimated and may deteriorate modeling results.
These sentences were included in lines (231248 and in lines 337341).
 Lines 280 onwards: There is no meaningful discussion section. Section 5 has some conclusions. But the authors have not contextualised their work in detail with respect to previous results in the literature. This is an important missing piece of the draft and we would suggest needs to be fixed. Furthermore, now that we have these new estimates, how could they be used in practice by scientists in the future?
Resp.: We revised this paragraph and section 5 to present the main results (lines 322326) and contextualize them in lines 337348.
Technical
 line 5 (“wave velocity”): is this group or phase velocity?
Resp.: We add the wave group velocity in line 5
 Line 15 (“interaction time can be ~30% lower for quiet periods”): we are not sure that it is appropriate to characterise things in this way. The authors have performed a small subset of case studies. Also, the details of the interaction time are fundamentally related to the microphysics of the waveparticle interaction, and not really whether it is an active or quiet period. Perhaps it is best not to phrase things in this way.
Resp.: We agree with the referee, and we remove this sentence
 Line 99: The Shprits 2008 paper cited is a paper about radial diffusion. You should replace this with a local diffusion paper by Shprits in the same series in JASTP
Resp.: The reference cited in the paper was correct to the following, in line (418): Yuri Y. Shprits, Dmitriy A. Subbotin, Nigel P. Meredith, Scot R. Elkington, Review of modeling of losses and sources of relativistic electrons in the outer radiation belt II: Local acceleration and loss, Journal of Atmospheric and SolarTerrestrial Physics, Volume 70, Issue 14, 2008, Pages 16941713, ISSN 13646826, https://doi.org/10.1016/j.jastp.2008.06.014.
 Line 134: “wellknown formula of the addition of velocities”. What is this formula? Please provide the formula and a citation
Resp.: Equation (7) in the manuscript is the general equation for the relativistic addition of velocities between vg and vgc. In line 133, we add the citation of Jackson, J. D. Classical Electrodynamics, which was included in line 378
 Equation 18: the authors use \Delta on the LHS but “d” on the RHS for infinitesimal changes. They should either use one or the other, and be consistent on both sides of the equation.
Resp.: We made the suggested change in equation (18), line 190

AC3: 'Reply on AC2', Livia R. Alves, 17 Aug 2023
Response to Reviewer  #2
The authors have done a good job incorporating additional literature and answering several of the reviewers’ feedback, especially concerning the validity of the inertial frame of reference and by adding the effect on the diffusion coefficient through the Lakhina et al method. The authors have convinced me that incorporating relativistic effects to account for the transit time of interaction is potentially worthy of additional studies. However, the use of the Lakhina et al. method (which is heuristic at best, and has often been used in the literature because it is less cumbersome than the Kennel and Engelman or Hamiltonian methodologies), to account for a higher order effect (length and time contraction), is not a good enough choice. The \Delta t in Equation (19) is entirely arbitrary and all the changes highlighted by the authors between relativistic and nonrelativistic effects stem from it. The numerous definition of Delta t given in the literature are certainly plausible but nonetheless ad hoc and would require a more carefully theoretical (e.g. through Hamiltonian methods) or/and numerical analysis. I will therefore recommend publication with the following additional caveat added to the paper: when compared with the Lakhina et al. methodology for pitchangle scattering, we find that relativistic effects result in larger pitchangle diffusion. Our results indicate that more accurate descriptions of pitchangle scattering by whistler waves (e.g. through the Kennel and Engelman method or through Hamiltonian methods) can also potentially be significantly affected by the addition of relativistic effects.
Response: We thank to referee for this recommendation. We added it at the Conclusion in lines 345348
Additional comments:
L160 The definition of the guidingcentre trajectory in the paper seems incorrect to me. What the authors are using is the exact particle’s motion in a frame they do not define. What is known as the guidingcentre trajectory is the one accounting for various particle’s drifts perpendicular to the mean field plus the parallel motion (à la Northrop and Teller).
Response: In this manuscript, the guiding center is defined as the center of a circular orbit of the electron around the magnetic field line, according to Baumjohann and Treumann (1997). We added this information and the reference in lines 145146.
Baumjohann and Treumann, (1997) Basic Space Plasma Physics, Imperial College Press, 1ed, ISBN 186094079X
And the guidingcentre velocity is frame specific (for instance, sometimes it’s defined in the E cross B frame of reference). What the authors define as a guiding centre drift is the resonant velocity (Equation 4) projected along the mean field. However, it is not clear in which frame this velocity of Equation (4) is defined to start with. Which makes me wonder why the authors did not more simply compute the resonance in the frame of the wave (which has the advantage of having no electric field for parallel propagation) and then transform in the frame of the satellite with the relativistic effect accounted for.
Response: Eq. 4 is in the frame of the satellite because this is the frame where the measurements are taken, including the velocity of the electron's guiding center. This information was added in line 120.
L240 the last sentence of the paragraph in Equation 21 is unclear. Moreover, in the pitchangle diffusion coefficient of Equation 21 the average is taken over some randomphases or for a collection of particles (ensembleaverage). The author seem to average over multiple interaction times by assuming some powerlaw distribution in the wavepacket element duration tau. Therefore Equation 21 is a diffusion equation for a collection of particle, and the definition of the last sentence of L240 is for a particle with a given pitchangle and energy that encounters a large number of wavepackets. It’s not clear to me if these two definitions are consistent with one another but the former one (à la Kennel and Engelman) is the only one that makes sense to me when applied to a kinetic equation for a collection of particles.
Response: We apologize that this point is not clear in the manuscript.
We consider that waveparticle interaction occurs at the equator. Then, the change in the electron's pitch angle derived in Eq. (20) considers the interaction with one chorus wave subelement with a constant time duration (tau). However, Santolik et al., 2004 showed that the whistlermode chorus wave time duration can follow a power law distribution. Thus, in Eq. (21), we use a time average in pitch angle calculation to account for a subelement that has a power law time (such as done before by Lakhina et al., 2010). This emphasizes the relevance of the interaction time, which is the main topic of this manuscript. As a consequence of such construction, a limitation of this approach is that other averaged effects, such as spectrum fluctuation (Kennel and Petschek, 1966) or random phase (Li et al., 2015), bounceorbit (Lyons et al., 1972; Glauert and Horne, 2005), and ensemble contributions (Tao et al., 2011, 2012) affecting the pitch angle diffusion coefficient have to be considered separated. Finally, Table 1 compares the pitch angle diffusion coefficient resulting from different interaction times for relativistic and nonrelativistic approaches used to describe the interaction between electron and wave (with a subelement time duration given by a power law distribution) interaction. This discussion was inserted in the manuscript in lines 225, 238242. Also, the following references were included.
Glauert, S. A., and Horne, R. B. (2005), Calculation of pitch angle and energy diffusion coefficients with the PADIE code, J. Geophys. Res., 110, A04206, doi:10.1029/2004JA010851.
Li, X., Tao, X., Lu, Q., and Dai, L. (2015), Bounce resonance diffusion coefficients for spatially confined waves, Geophys. Res. Lett., 42, 9591–9599, doi:10.1002/2015GL066324.
Tao, X., Bortnik, J., Albert, J. M., Liu, K., and Thorne, R. M. (2011), Comparison of quasilinear diffusion coefficients for parallel propagating whistler mode waves with test particle simulations, Geophys. Res. Lett., 38, L06105, doi:10.1029/2011GL046787.
Tao, X., Bortnik, J., Albert, J. M., and Thorne, R. M. (2012), Comparison of bounceaveraged quasilinear diffusion coefficients for parallel propagating whistler mode waves with test particle simulations, J. Geophys. Res., 117, A10205, doi:10.1029/2012JA017931.
Citation: https://doi.org/10.5194/angeo20236AC3

RC2: 'Comment on angeo20236', Anonymous Referee #2, 29 Mar 2023
The authors argue that taking into account special relativity effects would alter the waveparticle interactions between chorus and energetic electrons in the radiation belts. Unfortunately their results (most notably shown in Table 1) demonstrate the opposite, that is that relativistic effects are most likely inconsequential. And here is why. Their calculation assumes that electrons interacting with chorus waves will experience weak scattering, and thus nonlinear effects such as phasetrapping (Bortnik et al. 2008 GRL) or physical trapping (Artemyev et al. 2013 PoP, Osmane et al. ApJ 2016) can be neglected. Thus, by assuming that the waves are indeed sufficiently small in amplitude (clearly not the case for some of their events since delta B/B_0 >=1%) and that we are in a quasilinear regime, the transit time they are calculating with or without relativistic effects are comparable, with some minor differences of 0.10.01 ms. What would actually justify their thesis would be to show that the pitchangle diffusion coefficient they can compute from Delta_alpha (Equation 20) would lead to notable differences in the particle scattering. But they do not provide such an analysis and the change in the pitchangle shown in Table 1 (assuming again we are within a quasilinear regime despite the large amplitudes of the waves) are essentially identical for both relativistic and nonlinear relativistic effects with differences of the order 1/10 or 1/100. If we are interested with the nonlinear regime, the transit time they compute only make sense when compared with some nonlinear timescales, such as the trapping time. But since their transit time are essentially identitical I don't see how relativistic effect could turn a linear interaction into a nonlinear one either. I am therefore not certain how the paper could be salvaged since the relativistic effect they study seems to have no impact for both linear and nonlinear waveparticle interactions. If the editors are willing to accept a null result, the authors could perhaps compute the diffusion coefficients with relativistic effects included, and if the difference is marginal publish it as such.
Citation: https://doi.org/10.5194/angeo20236RC2 
AC1: 'Reply on RC2', Livia R. Alves, 10 May 2023
Response to Referee #2
The authors appreciate all suggestions given by Reviewers 1 and 2, which were essential to improve this article. A careful revision was carried out in the manuscript taking into account all the comments and suggestions.
1. The authors argue that taking into account special relativity effects would alter the waveparticle interactions between chorus and energetic electrons in the radiation belts. Unfortunately their results (most notably shown in Table 1) demonstrate the opposite, that is that relativistic effects are most likely inconsequential. And here is why. Their calculation assumes that electrons interacting with chorus waves will experience weak scattering, and thus nonlinear effects such as phasetrapping (Bortnik et al. 2008 GRL) or physical trapping (Artemyev et al. 2013 PoP, Osmane et al. ApJ 2016) can be neglected.
Resp.: We clarify in the manuscript that the derived equations described in this paper are applicable to a quasilinear regime.
2. Thus, by assuming that the waves are indeed sufficiently small in amplitude (clearly not the case for some of their events since delta B/B_0 >=1%) and that we are in a quasilinear regime, the transit time they are calculating with or without relativistic effects are comparable, with some minor differences of 0.10.01 ms. What would actually justify their thesis would be to show that the pitchangle diffusion coefficient they can compute from Delta_alpha (Equation 20) would lead to notable differences in the particle scattering. But they do not provide such an analysis and the change in the pitchangle shown in Table 1 (assuming again we are within a quasilinear regime despite the large amplitudes of the waves) are essentially identical for both relativistic and nonlinear relativistic effects with differences of the order 1/10 or 1/100.
Resp.: We thank the referee for this point, which improves the manuscript. As we are interested in showing the relevance of a more complete relativistic description in linear waveparticle events, we choose periods in which linear processes are likely in the previous events and substitute case 2 for a new event. Then we revised the periods selected for each event and chose a linear one. Besides, we calculate the pitch angle diffusion coefficient (Da) following the same approach as done by Lakhina et al., 2010. The results are summarized in Table 1 (attached). The comparison between nonrelativistic and complete relativistic calculations shows that the interaction time is around 4 times higher when the Special Relativity kinematics is considered. Also, the diffusion coefficient rates show notable differences in the pitch angle scattering.
3. If we are interested with the nonlinear regime, the transit time they compute only make sense when compared with some nonlinear timescales, such as the trapping time. But since their transit time are essentially identitical I don't see how relativistic effect could turn a linear interaction into a nonlinear one either. I am therefore not certain how the paper could be salvaged since the relativistic effect they study seems to have no impact for both linear and nonlinear waveparticle interactions. If the editors are willing to accept a null result, the authors could perhaps compute the diffusion coefficients with relativistic effects included, and if the difference is marginal publish it as such.
Resp.: Accordingly, we show that for the selected case studies, the relativistic diffusion coefficient rates in Table 1 (attached) can be more than 5 times higher than the nonrelativistic diffusion rates.

AC1: 'Reply on RC2', Livia R. Alves, 10 May 2023
Status: closed

RC1: 'Comment on angeo20236', Anonymous Referee #1, 28 Mar 2023
General
This draft presents calculations regarding the interaction time for electrons with chorus waves, and the resultant effect on pitch angle transport (“delta alpha”). The main proposed contribution is that the calculation is presented as being consistent with special relativity. Impicitly, the reader is to assume that this is being performed for the first time in the literature.
I believe that the basic principle of the work presented in this draft is sound, and potentially important. Although I do have a major concern regarding the assumption of an inertial satellite frame of reference
Even if that major concern is cleared up, I believe that further major revisions are necessary before publication can be recommended.
These revisions mostly centre around
 Calculations – I have some serious questions regarding some of the calculations. Or clarifications that need to be made regarding the validity of the results
 Data – I do not see what significant value the presented Van Allen Probes data adds, for the manuscript in the current form. More work needs to be done, I would suggest.
 Context – we need much more justification and references to literature. And discussion.
Major comments
Calculations
1. All of the calculations rely on the comparisons of inertial frames of reference. Does a satellite have an inertial frame?
Not only is the satellite orbiting the Earth (and therefore undergoing acceleration), but it is also rotating around its own axis (and as a result so are the devices that measure BuBvBw etc). Please clarify. We need to have absolute clarity on this. Please can the authors give a thorough justification to explain why this is a reasonable approach. How are the inertial frames constructed and justified, given the above mentioned 2 sources of acceleration?
Relatedly, if there is a justification for this, we sould strongly suggest that the authors make a diagram that illustrates what S, S’, and the different relativistic considerations are regarding the wave and the satellite, in order to help the reader understand what is going on
2. e.g. going from equations 14 to 20, and in particular 19 to 20
All of this analysis assumes that
 the forces on the particle are constant during the timescale 0
 It also assumes that T is determined by some version of “T=X/V” (e.g equation 10 from Lakhina et al 2010), or a relativistic version equation 13 in this paper.
Both of these are quite restrictive approximations, although we accept that they are relatively standard methods that are used in the literature e.g. Kennel&Petschek 1966, Lakhina et al 2010 as cited by the authors. The approximations are as follows.
 The presented equations are a big approximation to the real answer, which requires the solution of coupled first order odes for gyrophase, pitch angle, energy, position (e.g. see exact solutions up to second order in Bwave/B0 in Allanson et al 2022 Front. Astron. Space Sci. 8:805699. doi:10.3389/fspas.2021.805699)
 the interaction time could be shorter than this if the particle is scattered away very quickly. Likewise it could be longer if the particle is trapped (e.g. see Bortnik et al 2008 GEOPHYSICAL RESEARCH LETTERS, VOL. 35, L21102, doi:10.1029/2008GL035500, 2008)
Therefore it is important to state these approximations, and to say that the answers could be very different if (i) and (ii) play an important role, e.g. for higher amplitude/nonlinear waves. Conversely, the results in this paper are probably only true for a quasilinear interaction (e.g. Kennel and Engelmann 1966 The Physics of Fluids 9, 2377 (1966).
3. Equation (3) in the manuscript is incorrect. E.g. see
Equation (1) in Lakhina et al 2010
Or equation (13) in Artemyev et al Space Sci Rev (2016) 200:261–355 DOI 10.1007/s1121401602525
or equation 1 in Shprits et al Journal ofAtmosphericandSolarTerrestrialPhysics70(2008)1694–1713
It should only be k_parallel and v_parallel in the doppler shift. The velocity component of interest is
v_parallel = v*cos\alpha
Therefore there are a range of speeds (v) and pitch angles (\alpha) that are resonant with any given wave frequency \omega. E.g.
see equations 151 and 152 from Omura Earth, Planets and Space (2021) 73:95.
Therefore equation 4 not quite correct. This could have serious implications for the rest of the draft? The point is that there are many different values of energy that can resonate with a given wave, and these are a function of pitchangle, e.g. see an example for the n=1 resonance in
Camporeale, E. (2015), Resonant and nonresonant whistlersparticle interaction in the radiation belts, Geophys. Res. Lett., 42, 3114–3121, doi:10.1002/2015GL063874.
Data
4. Case studies 1, 2 and 3 all have magnetic field wave amplitudes >= 1nT (see table 1). With B0 roughly 100nT. That gives Bw/B0 ~ 1/100. These are very intense waves and almost certainly fall into the nonlinear regime (e.g. phase trapping and phase bunching etc) e.g. see
Zhang et al JGR, 2018, 123, 5379–5393, https://doi.org/10.1029/2018JA025390 and
Zhang et al GRL, 2019, 46, 7182–7190. https://doi.org/10.1029/2019GL083833
As per the above comment (2), I question whether interaction time method described in the paper is applicable. Or to put it another way, I would need to be convinced – please!
5. implications of point 3 regarding resonant particles. There is not one single resonant energy. There is a single resonant v_parallel for a given value of n, but this corresponds to many energies and pitchangles. Therefore we do not understand figure 2 as it is currently presented, or any results or discussion that make use of the results from equation 5, and discussions about the given value of resonant energy
6. Lines 208 – 267: There is a lengthy description of some Van Allen Probes data here. But none of it really adds any genuine value to the manuscript in our opinion. From line 268 onwards there is a discussion of some parameters that are used and calculated for the interaction time. But that information is not really linked scientifically to the discussion of the data in lines 208267, except in a very superficial way. What are the implications of one on the other? What is the importance of the results and how does it related to the data? What new inferences can we make because of the data in the table etc? What might this show us in the Van Allen Probes data etc?
Context/References/Discussion
7. ~line 50: The authors claim that the relativistic approach is often simplified or misused, but they provide no references or discussion to support this claim. Please provide references and much more discussion! This is the foundation of the motivation for the paper. We suggest that there needs to be a much more thorough justification and motivation in the introduction of this draft
8. Line 69: Appleton/Hartree equation: please provide a citation and a justification for why this is the correct relation to use
9. Equation (20) How does the presented formula for \Delta\alpha compare to those presented in e.g. papers by Lakhina et al 2010, Tsurutani & Lakhina 1997, Kennel&Petschek66 and Allanson et al 2022? What differences has it made to include relativity, and what differences are observed because the integration was performed approximately and not exactly?
10. Lines 280 onwards: There is no meaningful discussion section. Section 5 has some conclusions. But the authors have not contextualised their work in detail with respect to previous results in the literature. This is an important missing piece of the draft and we would suggest needs to be fixed. Furthermore, now that we have these new estimates, how could they be used in practice by scientists in the future?
Technical
11. line 5 (“wave velocity”): is this group or phase velocity?
12. Line 15 (“interaction time can be ~30% lower for quiet periods”): we are not sure that it is appropriate to characterise things in this way. The authors have performed a small subset of case studies. Also, the details of the interaction time are fundamentally related to the microphysics of the waveparticle interaction, and not really whether it is an active or quiet period. Perhaps it is best not to phrase things in this way.
13. Line 99: The Shprits 2008 paper cited is a paper about radial diffusion. You should replace this with a local diffusion paper by Shprits in the same series in JASTP
14. Line 134: “wellknown formula of the addition of velocities”. What is this formula? Please provide the formula and a citation
15. Equation 18: the authors use \Delta on the LHS but “d” on the RHS for infinitesimal changes. They should either use one or the other, and be consistent on both sides of the equation.
Citation: https://doi.org/10.5194/angeo20236RC1 
AC2: 'Reply on RC1', Livia R. Alves, 10 May 2023
The authors appreciate all suggestions given by Reviewers 1 and 2, which were essential to improve this article. A careful revision was carried out in the manuscript taking into account all the comments and suggestions. The figures and Table 1, mentioned in the response, are available in the attached file (Figures_Table_response_to_reviewers.pdf).
Major comments
Calculations
 All of the calculations rely on the comparisons of inertial frames of reference. Does a satellite have an inertial frame?
Not only is the satellite orbiting the Earth (and therefore undergoing acceleration), but it is also rotating around its own axis (and as a result so are the devices that measure BuBvBw etc). Please clarify. We need to have absolute clarity on this. Please can the authors give a thorough justification to explain why this is a reasonable approach. How are the inertial frames constructed and justified, given the above mentioned 2 sources of acceleration?
We add the discussion below in lines 147154:
To justify the use of an inertial frame associated with the satellite, consider, for instance, the maximum acceleration achieved by the satellite at the perigee (data from satellite orbit can be found e.g. at Mauk et al., 2013), $8.2~{\rm m}{\rm s}^{2}$. The interaction time between the electron and the wave is of the order of $10^{3}$ s. Since the period of the satellite is $537.1$ min, its acceleration is nearly constant during the interaction. Therefore, the change in the speed of the satellite in its orbit during one interaction time is around $8.2 \times 10^{3}~{\rm m}/{\rm s}$ which is 6 orders of magnitude smaller than the speed of the satellite at the perigee 9,8 km/s. Similarly, the spin period of the satellite is 11 s (Breneman et al., 2022), which leads to a change in angle of about $1.8~{\rm arcmin}$ in one interaction time. Thus, for the purposes of the present article, it is reasonable to consider the satellite as an inertial reference frame during one interaction time. Moreover, it is a standard approach in the literature to consider the satellite as an inertial reference frame.
Breneman, A.W., Wygant, J.R., Tian, S. et al. The Van Allen Probes Electric Field and Waves Instrument: Science Results, Measurements, and Access to Data. Space Sci Rev 218, 69 (2022). https://doi.org/10.1007/s1121402200934y)
Mauk, B.H., Fox, N.J., Kanekal, S.G. et al. Science Objectives and Rationale for the Radiation Belt Storm Probes Mission. Space Sci Rev 179, 3–27 (2013). https://doi.org/10.1007/s112140129908y
Relatedly, if there is a justification for this, we sould strongly suggest that the authors make a diagram that illustrates what S, S’, and the different relativistic considerations are regarding the wave and the satellite, in order to help the reader understand what is going on
Resp.: The diagram was included in the manuscript as Figure 3
 e.g. going from equations 14 to 20, and in particular 19 to 20
All of this analysis assumes that
 the forces on the particle are constant during the timescale 0
 It also assumes that T is determined by some version of “T=X/V” (e.g equation 10 from Lakhina et al 2010), or a relativistic version equation 13 in this paper.
Both of these are quite restrictive approximations, although we accept that they are relatively standard methods that are used in the literature e.g. Kennel&Petschek 1966, Lakhina et al 2010 as cited by the authors. The approximations are as follows.
 e.g. going from equations 14 to 20, and in particular 19 to 20
All of this analysis assumes that
 the forces on the particle are constant during the timescale 0
 It also assumes that T is determined by some version of “T=X/V” (e.g equation 10 from Lakhina et al 2010), or a relativistic version equation 13 in this paper.
Both of these are quite restrictive approximations, although we accept that they are relatively standard methods that are used in the literature e.g. Kennel&Petschek 1966, Lakhina et al 2010 as cited by the authors. The approximations are as follows.
 The presented equations are a big approximation to the real answer, which requires the solution of coupled first order odes for gyrophase, pitch angle, energy, position (e.g. see exact solutions up to second order in Bwave/B0 in Allanson et al 2022 Front. Astron. Space Sci. 8:805699. doi:10.3389/fspas.2021.805699)
 the interaction time could be shorter than this if the particle is scattered away very quickly. Likewise it could be longer if the particle is trapped (e.g. see Bortnik et al 2008 GEOPHYSICAL RESEARCH LETTERS, VOL. 35, L21102, doi:10.1029/2008GL035500, 2008)
Therefore it is important to state these approximations, and to say that the answers could be very different if (i) and (ii) play an important role, e.g. for higher amplitude/nonlinear waves. Conversely, the results in this paper are probably only true for a quasilinear interaction (e.g. Kennel and Engelmann 1966 The Physics of Fluids 9, 2377 (1966).
Resp.: We thank the referee for this suggestion, and we include the following paragraph in the manuscript (lines 234241 and 337348):
The manuscript aims to improve the calculation of the interaction time in the quasilinear waveparticle interaction regime. Thus, we use firstorder solutions such as those done by Lakhina and Tsurutani, 2010. The weak turbulence in plasma and nonlinear events occurrence rate is around 10 to 15% considering the average occurrence of whistlermode chorus waves (Zhang et al., 2018). These events have a solution of the waveparticle interaction equation are based on, at least, secondorder terms in wave amplitude, e.g., Allanson et al., 2022; Artemyev et al., 2023; Omura, 2021; Osmane et al., 2016; Bortnik et al., 2008).
There are several difficulties in calculating the trapping time in nonlinear interactions (e.g., eq. (87) Omura, 2021, Omura et al., 2013, Omura et al., 2008) using in situ measurements. Though, the firstorder approach can give approximate solutions to nonlinear regimes, and Equation (13) can be used to estimate the interaction time from insitu measurements (e.g., Hsieh et al., 2021) since it is important to determine the energy gain of electrons undergoing a waveparticle interaction (Hsieh et al., 2021). However, the interaction time is known to be shorter than the trapping time (Hsieh et al., 2021; Bortnik et al., 2008)
Anton V. Artemyev, Jay M. Albert, Anatoli I. Neishtadt, Didier Mourenas; The effect of wave frequency drift on the electron nonlinear resonant interaction with whistlermode waves. Physics of Plasmas 1 January 2023; 30 (1): 012901. https://doi.org/10.1063/5.0131297
Omura, Y., Katoh, Y., and Summers, D. (2008), Theory and simulation of the generation of whistlermode chorus, J. Geophys. Res., 113, A04223, doi:10.1029/2007JA012622.
Osmane, A., Wilson, L. B., Blum, L., Pulkkinen, T. I. (2016), On The Connection Between Microbursts And Nonlinear Electronic Structures In Planetary Radiation Belts. The Astrophysical Journal, ApJ 816 51, https://dx.doi.org/10.3847/0004637X/816/2/51
Allanson, O., Thomas, E., Clare, W., Thomas, N. (2022), Weak Turbulence and Quasilinear Diffusion for Relativistic WaveParticle Interactions Via a Markov Approach. Front. Astron. Space Sci. 8:805699. doi:10.3389/fspas.2021.805699
Bortnik, J., Thorne, R. M., and Inan, U. S. (2008), Nonlinear interaction of energetic electrons with large amplitude chorus, Geophys. Res. Lett., 35, L21102, doi:10.1029/2008GL035500.
Zhang, J., Thorne, R., Artemyev, A., Mourenas, D., Angelopoulos, V., Bortnik, J., Kletzing, C. A., Kurth, W. S., & Hospodarsky, G. B. (2018). Properties of Intense FieldAligned LowerBand Chorus Waves: Implications for Nonlinear WaveParticle Interactions. Journal of Geophysical Research: Space Physics, 123(7), 53795393. https://doi.org/10.1029/2018JA025390
 Equation (3) in the manuscript is incorrect. E.g. see
Equation (1) in Lakhina et al 2010
Or equation (13) in Artemyev et al Space Sci Rev (2016) 200:261–355 DOI 10.1007/s1121401602525
or equation 1 in Shprits et al Journal ofAtmosphericandSolarTerrestrialPhysics70(2008)1694–1713
It should only be k_parallel and v_parallel in the doppler shift. The velocity component of interest is
v_parallel = v*cos\alpha
Resp.: We thank the referee for this point. In the manuscript, we write Equation (3) as a general equation for the Doppler shift in the wave frequency. We explain in lines 113115 that we are considering the wave vector parallel to the ambient magnetic field for the wave's direction being copropagating and counterpropagating to the energetic electron. In this case, the equatorial electron pitch angle \alpha used in equation (3) will be the same as done by Lakhina et al., 2020, Artemyev et al., 2016, and Camporeale (2015).
We call \delta the angle between the wave vector and the electron velocity vector. This correction was included in equation (4) and lines 118119. Also, Figure 2 was corrected, and the discussion was added in lines 128131.
Therefore there are a range of speeds (v) and pitch angles (\alpha) that are resonant with any given wave frequency \omega. E.g.
see equations 151 and 152 from Omura Earth, Planets and Space (2021) 73:95.
Resp.: Yes, we agree, and this is shown by the n (harmonic number) in Eq. (4) in the submitted manuscript.
Therefore equation 4 not quite correct. This could have serious implications for the rest of the draft?
Resp: Equation (4) was corrected by changing the angle between the electron velocity vector and the wave normal angle as \delta; both vectors' orientations are defined as related to the ambient magnetic field in a tridimensional coordinate system. In the manuscript, we solve Eq. (4) for \delta equals \alpha and \pi  \alpha for copropagating and counterpropagating waves, respectively. In such an approach, both resonant and perpendicular components of the electron velocity vector are considered in the calculation, similar to that done by Summers et al., 2012.
The point is that there are many different values of energy that can resonate with a given wave, and these are a function of pitchangle, e.g. see an example for the n=1 resonance in
Camporeale, E. (2015), Resonant and nonresonant whistlersparticle interaction in the radiation belts, Geophys. Res. Lett., 42, 3114–3121, doi:10.1002/2015GL063874.
Resp.: We agree with the referee that there are many different energies resonating with a given wave frequency, since we have the possibility to match several harmonics with the same wave; besides, for parallel propagating whistler waves, the angle between the wave vector and electron speed vector coincides with the electron's pitch angle, as shown by Camporeale, E. 2015. This information and reference were added in the manuscript in lines 129131.
Data
 Case studies 1, 2 and 3 all have magnetic field wave amplitudes >= 1nT (see table 1). With B0 roughly 100nT. That gives Bw/B0 ~ 1/100. These are very intense waves and almost certainly fall into the nonlinear regime (e.g. phase trapping and phase bunching etc) e.g. see
Zhang et al JGR, 2018, 123, 5379–5393, https://doi.org/10.1029/2018JA025390 and
Zhang et al GRL, 2019, 46, 7182–7190. https://doi.org/10.1029/2019GL083833
As per the above comment (2), I question whether interaction time method described in the paper is applicable. Or to put it another way, I would need to be convinced – please!
Resp: We thank the referee for this point, and we clarify that the interaction time calculated in this manuscript accounts for the firstorder cyclotron effect only. We included the citation of Hsieh et al., 2020 and 2017; Omura, 2021, Omura et al., 2013; Omura et al., 2008 to show an example in the literature of the interaction time in nonlinear cases. In addition, we changed the case studies presented in Table 1 to apply the derived equations to the linear waveparticle cases. Also, Figures 6, 7, D1, and E1 were updated.
Hsieh, Y.K., and Omura, Y. (2017), Nonlinear dynamics of electrons interacting with oblique whistlermode chorus in the magnetosphere, J. Geophys. Res. Space Physics, 122, 675– 694, doi:10.1002/2016JA023255.
 implications of point 3 regarding resonant particles. There is not one single resonant energy. There is a single resonant v_parallel for a given value of n, but this corresponds to many energies and pitchangles. Therefore we do not understand figure 2 as it is currently presented, or any results or discussion that make use of the results from equation 5, and discussions about the given value of resonant energy
Resp.: Figure (2) was corrected for the angle between the wave vector and electron velocity vector. Figure (2) is an example of Eq. (5) for a given ambient plasma parameters, wave normal angle, equatorial electron pitch angle, and one harmonic number. It is shown to give an example of how the resonant electron kinetic energy varies as a function of the wave frequency, for waves propagating parallel and oblique to the ambient magnetic field. Accordingly, if the harmonic number n is changed, all the curves would be shifted to the higher wave frequency side. We inserted a sentence about this point in line 128.
 Lines 208 – 267: There is a lengthy description of some Van Allen Probes data here. But none of it really adds any genuine value to the manuscript in our opinion. From line 268 onwards there is a discussion of some parameters that are used and calculated for the interaction time. But that information is not really linked scientifically to the discussion of the data in lines 208267, except in a very superficial way. What are the implications of one on the other? What is the importance of the results and how does it related to the data? What new inferences can we make because of the data in the table etc? What might this show us in the Van Allen Probes data etc?
Resp.: We apologize if we were not clear. Section 4 was revised and split to organize the dataset in a subsection (starting in line 246).
Using Van Allen Probes data, it is possible to identify the periods of the highenergy electron flux dropouts and enhancements in the outer radiation belt concomitant with whistlermode chorus wave activities for each case study shown in Table 1. It suggests that the resonance between the chorus waves and particles may have locally contributed to this electron flux variability.
To clarify the importance of the discussions about the PSD in this article, we decided to write a new paragraph before line 208 and rewrote the discussions about Figures 5.1, A1.1 e B1.1, as described below:
Figures 5.1, A1.1 e B1.1 shows the time evolution of the radial PSD profiles at inbound/outbound regions of Van Allen Probe B, which allows the identification of the local relativistic electron loss and/or local lowenergy acceleration in the outer radiation belt. The pitch angle diffusion mechanism driven by whistler mode chorus waves can cause this kind of local electron flux loss/acceleration, in which the local (L*), order of magnitude, and energy level are identified at the same period analyzed in previous sections.
Reference:
Tsyganenko, N. A., & Sitnov, M. I. (2005). Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms. Journal of Geophysical Research, 110, A03208. https://doi.org/10.1029/2004JA010798
Context/References/Discussion
 ~line 50: The authors claim that the relativistic approach is often simplified or misused, but they provide no references or discussion to support this claim. Please provide references and much more discussion! This is the foundation of the motivation for the paper. We suggest that there needs to be a much more thorough justification and motivation in the introduction of this draft
Resp.: We include the discussion and references related to the motivation and justification of the paper in lines 45  66:
In the magnetosphere, the kinematics description of the waveparticle interaction for relativistic electrons usually considers the relativistic Doppler shift in the resonance condition (e.g., Thorne et al. 2005, Summers et al. 1998) and the relativistic motion equation (e.g., Omura, 2021). Often, the resonant kinetic energy of the electrons results from the resonance condition and the motion equation, together with the wave group velocity (e.g., Omura 2021, Hsieh et al., 2021, Summers et al., 2012, Glauer et al., 2005, Lyons et al., 1972). The waveparticle interaction time ($T_r$) is a crucial parameter in estimating timedependent processes as the energy and pitch angle diffusion coefficients \citep{walker1993, lakhina2010, tsurutani2013, hsieh2020, hsieh2022}, however, the relativistic kinematics description mentioned above is incomplete to calculate this parameter. In this paper, we add to the latter approach a complete relativistic description of the problem: the relativistic velocity addition (between the electron and the wave) and the implications of the different reference frames in the estimates of the change in pitch angle and the diffusion coefficient.
We calculate the parameters for four case studies to give a quantitative comparison between the complete relativistic description and a nonrelativistic approach (used here as an approximation to calculate the interaction parameters). The interaction time is calculated using the test particle equations \citep{tsurutani1974, lakhina2010, horne2003b, bortnik2008} along with the special relativity theory applied to whistlermode chorus waves propagating in cold plasma magnetosphere (where group velocity is $~0.3c$ to $0.5 c$) and energetic electrons (with energy $ \sim 0.1$ to $2$ MeV). We consider that the resonance occurs in the electron's reference frame. At the same time, the result of such interaction and their parameters are measured in the local inertial reference frame of the satellite.
We considered parallel propagating whistlermode chorus waves linearly interacting with relativistic electrons to derive first the group velocity equation, then the resonant relativistic kinetic energy, and finally the interaction time. Thus, we calculate the change pitch angle and the diffusion coefficient rates. We use the Van Allen Probes measurement of wave parameters, ambient magnetic field, density, electron fluxes, and equatorial pitch angle to apply the interaction time equation.
A complete calculation of these parameters can improve relativistic outer radiation belt electron flux variation models.
 Line 69: Appleton/Hartree equation: please provide a citation and a justification for why this is the correct relation to use
Resp.: We add the following justification and reference in lines 7881: whistler mode chorus waves which occur in frequencies higher than the ion cyclotron frequency, besides the waveparticle interaction outside the plasmasphere, the dispersion relation for this case is obtained from the solution of the AppletonHartree equation \citep{bittencourt2004}.
 Equation (20) How does the presented formula for \Delta\alpha compare to those presented in e.g. papers by Lakhina et al 2010, Tsurutani & Lakhina 1997, Kennel&Petschek66 and Allanson et al 2022? What differences has it made to include relativity, and what differences are observed because the integration was performed approximately and not exactly?
Resp.: The change in pitch angle for nonrelativistic electrons due to waveparticle interaction in a quasilinear regime is given by equations (3.6) in Kennel and Petschek, 1966, and (11) in Tsurutani and Lakhina, 1997. Lakhina et al., 2010, derived equation (11) by considering the relativistic resonant condition and the nonrelativistic equation of motion. Allanson et al., 2022, show the exact equation for pitch angle scattering and secondorder equations for weak turbulence and nonlinear regimes.
In this manuscript, the change in pitch angle is given by equation (20), which is consistent with equations (3.6) in Kennel and Petschek, 1966; (11) in Tsurutani and Lakhina, 1997 and equation (11) in Lakhina et al., 2010. In the limit that \gamma ~ 1, for nonrelativistic electrons, Tr equals to \delta t (in Kennel and Petschek, 1966 and Tsurutani and Lakhina, 1997) or to \tau in (Lakhina et al., 2010). Also, Equation (20) in this manuscript is similar to Equation (S3) in Allanson et al., 2021.
The main difference we observe using a more complete relativity description is that the interaction time is often longer than that calculated with a nonrelativistic description, as shown in Table 1. The consequence of underestimating the interaction time is that diffusion coefficients are also underestimated and may deteriorate modeling results.
These sentences were included in lines (231248 and in lines 337341).
 Lines 280 onwards: There is no meaningful discussion section. Section 5 has some conclusions. But the authors have not contextualised their work in detail with respect to previous results in the literature. This is an important missing piece of the draft and we would suggest needs to be fixed. Furthermore, now that we have these new estimates, how could they be used in practice by scientists in the future?
Resp.: We revised this paragraph and section 5 to present the main results (lines 322326) and contextualize them in lines 337348.
Technical
 line 5 (“wave velocity”): is this group or phase velocity?
Resp.: We add the wave group velocity in line 5
 Line 15 (“interaction time can be ~30% lower for quiet periods”): we are not sure that it is appropriate to characterise things in this way. The authors have performed a small subset of case studies. Also, the details of the interaction time are fundamentally related to the microphysics of the waveparticle interaction, and not really whether it is an active or quiet period. Perhaps it is best not to phrase things in this way.
Resp.: We agree with the referee, and we remove this sentence
 Line 99: The Shprits 2008 paper cited is a paper about radial diffusion. You should replace this with a local diffusion paper by Shprits in the same series in JASTP
Resp.: The reference cited in the paper was correct to the following, in line (418): Yuri Y. Shprits, Dmitriy A. Subbotin, Nigel P. Meredith, Scot R. Elkington, Review of modeling of losses and sources of relativistic electrons in the outer radiation belt II: Local acceleration and loss, Journal of Atmospheric and SolarTerrestrial Physics, Volume 70, Issue 14, 2008, Pages 16941713, ISSN 13646826, https://doi.org/10.1016/j.jastp.2008.06.014.
 Line 134: “wellknown formula of the addition of velocities”. What is this formula? Please provide the formula and a citation
Resp.: Equation (7) in the manuscript is the general equation for the relativistic addition of velocities between vg and vgc. In line 133, we add the citation of Jackson, J. D. Classical Electrodynamics, which was included in line 378
 Equation 18: the authors use \Delta on the LHS but “d” on the RHS for infinitesimal changes. They should either use one or the other, and be consistent on both sides of the equation.
Resp.: We made the suggested change in equation (18), line 190

AC3: 'Reply on AC2', Livia R. Alves, 17 Aug 2023
Response to Reviewer  #2
The authors have done a good job incorporating additional literature and answering several of the reviewers’ feedback, especially concerning the validity of the inertial frame of reference and by adding the effect on the diffusion coefficient through the Lakhina et al method. The authors have convinced me that incorporating relativistic effects to account for the transit time of interaction is potentially worthy of additional studies. However, the use of the Lakhina et al. method (which is heuristic at best, and has often been used in the literature because it is less cumbersome than the Kennel and Engelman or Hamiltonian methodologies), to account for a higher order effect (length and time contraction), is not a good enough choice. The \Delta t in Equation (19) is entirely arbitrary and all the changes highlighted by the authors between relativistic and nonrelativistic effects stem from it. The numerous definition of Delta t given in the literature are certainly plausible but nonetheless ad hoc and would require a more carefully theoretical (e.g. through Hamiltonian methods) or/and numerical analysis. I will therefore recommend publication with the following additional caveat added to the paper: when compared with the Lakhina et al. methodology for pitchangle scattering, we find that relativistic effects result in larger pitchangle diffusion. Our results indicate that more accurate descriptions of pitchangle scattering by whistler waves (e.g. through the Kennel and Engelman method or through Hamiltonian methods) can also potentially be significantly affected by the addition of relativistic effects.
Response: We thank to referee for this recommendation. We added it at the Conclusion in lines 345348
Additional comments:
L160 The definition of the guidingcentre trajectory in the paper seems incorrect to me. What the authors are using is the exact particle’s motion in a frame they do not define. What is known as the guidingcentre trajectory is the one accounting for various particle’s drifts perpendicular to the mean field plus the parallel motion (à la Northrop and Teller).
Response: In this manuscript, the guiding center is defined as the center of a circular orbit of the electron around the magnetic field line, according to Baumjohann and Treumann (1997). We added this information and the reference in lines 145146.
Baumjohann and Treumann, (1997) Basic Space Plasma Physics, Imperial College Press, 1ed, ISBN 186094079X
And the guidingcentre velocity is frame specific (for instance, sometimes it’s defined in the E cross B frame of reference). What the authors define as a guiding centre drift is the resonant velocity (Equation 4) projected along the mean field. However, it is not clear in which frame this velocity of Equation (4) is defined to start with. Which makes me wonder why the authors did not more simply compute the resonance in the frame of the wave (which has the advantage of having no electric field for parallel propagation) and then transform in the frame of the satellite with the relativistic effect accounted for.
Response: Eq. 4 is in the frame of the satellite because this is the frame where the measurements are taken, including the velocity of the electron's guiding center. This information was added in line 120.
L240 the last sentence of the paragraph in Equation 21 is unclear. Moreover, in the pitchangle diffusion coefficient of Equation 21 the average is taken over some randomphases or for a collection of particles (ensembleaverage). The author seem to average over multiple interaction times by assuming some powerlaw distribution in the wavepacket element duration tau. Therefore Equation 21 is a diffusion equation for a collection of particle, and the definition of the last sentence of L240 is for a particle with a given pitchangle and energy that encounters a large number of wavepackets. It’s not clear to me if these two definitions are consistent with one another but the former one (à la Kennel and Engelman) is the only one that makes sense to me when applied to a kinetic equation for a collection of particles.
Response: We apologize that this point is not clear in the manuscript.
We consider that waveparticle interaction occurs at the equator. Then, the change in the electron's pitch angle derived in Eq. (20) considers the interaction with one chorus wave subelement with a constant time duration (tau). However, Santolik et al., 2004 showed that the whistlermode chorus wave time duration can follow a power law distribution. Thus, in Eq. (21), we use a time average in pitch angle calculation to account for a subelement that has a power law time (such as done before by Lakhina et al., 2010). This emphasizes the relevance of the interaction time, which is the main topic of this manuscript. As a consequence of such construction, a limitation of this approach is that other averaged effects, such as spectrum fluctuation (Kennel and Petschek, 1966) or random phase (Li et al., 2015), bounceorbit (Lyons et al., 1972; Glauert and Horne, 2005), and ensemble contributions (Tao et al., 2011, 2012) affecting the pitch angle diffusion coefficient have to be considered separated. Finally, Table 1 compares the pitch angle diffusion coefficient resulting from different interaction times for relativistic and nonrelativistic approaches used to describe the interaction between electron and wave (with a subelement time duration given by a power law distribution) interaction. This discussion was inserted in the manuscript in lines 225, 238242. Also, the following references were included.
Glauert, S. A., and Horne, R. B. (2005), Calculation of pitch angle and energy diffusion coefficients with the PADIE code, J. Geophys. Res., 110, A04206, doi:10.1029/2004JA010851.
Li, X., Tao, X., Lu, Q., and Dai, L. (2015), Bounce resonance diffusion coefficients for spatially confined waves, Geophys. Res. Lett., 42, 9591–9599, doi:10.1002/2015GL066324.
Tao, X., Bortnik, J., Albert, J. M., Liu, K., and Thorne, R. M. (2011), Comparison of quasilinear diffusion coefficients for parallel propagating whistler mode waves with test particle simulations, Geophys. Res. Lett., 38, L06105, doi:10.1029/2011GL046787.
Tao, X., Bortnik, J., Albert, J. M., and Thorne, R. M. (2012), Comparison of bounceaveraged quasilinear diffusion coefficients for parallel propagating whistler mode waves with test particle simulations, J. Geophys. Res., 117, A10205, doi:10.1029/2012JA017931.
Citation: https://doi.org/10.5194/angeo20236AC3

RC2: 'Comment on angeo20236', Anonymous Referee #2, 29 Mar 2023
The authors argue that taking into account special relativity effects would alter the waveparticle interactions between chorus and energetic electrons in the radiation belts. Unfortunately their results (most notably shown in Table 1) demonstrate the opposite, that is that relativistic effects are most likely inconsequential. And here is why. Their calculation assumes that electrons interacting with chorus waves will experience weak scattering, and thus nonlinear effects such as phasetrapping (Bortnik et al. 2008 GRL) or physical trapping (Artemyev et al. 2013 PoP, Osmane et al. ApJ 2016) can be neglected. Thus, by assuming that the waves are indeed sufficiently small in amplitude (clearly not the case for some of their events since delta B/B_0 >=1%) and that we are in a quasilinear regime, the transit time they are calculating with or without relativistic effects are comparable, with some minor differences of 0.10.01 ms. What would actually justify their thesis would be to show that the pitchangle diffusion coefficient they can compute from Delta_alpha (Equation 20) would lead to notable differences in the particle scattering. But they do not provide such an analysis and the change in the pitchangle shown in Table 1 (assuming again we are within a quasilinear regime despite the large amplitudes of the waves) are essentially identical for both relativistic and nonlinear relativistic effects with differences of the order 1/10 or 1/100. If we are interested with the nonlinear regime, the transit time they compute only make sense when compared with some nonlinear timescales, such as the trapping time. But since their transit time are essentially identitical I don't see how relativistic effect could turn a linear interaction into a nonlinear one either. I am therefore not certain how the paper could be salvaged since the relativistic effect they study seems to have no impact for both linear and nonlinear waveparticle interactions. If the editors are willing to accept a null result, the authors could perhaps compute the diffusion coefficients with relativistic effects included, and if the difference is marginal publish it as such.
Citation: https://doi.org/10.5194/angeo20236RC2 
AC1: 'Reply on RC2', Livia R. Alves, 10 May 2023
Response to Referee #2
The authors appreciate all suggestions given by Reviewers 1 and 2, which were essential to improve this article. A careful revision was carried out in the manuscript taking into account all the comments and suggestions.
1. The authors argue that taking into account special relativity effects would alter the waveparticle interactions between chorus and energetic electrons in the radiation belts. Unfortunately their results (most notably shown in Table 1) demonstrate the opposite, that is that relativistic effects are most likely inconsequential. And here is why. Their calculation assumes that electrons interacting with chorus waves will experience weak scattering, and thus nonlinear effects such as phasetrapping (Bortnik et al. 2008 GRL) or physical trapping (Artemyev et al. 2013 PoP, Osmane et al. ApJ 2016) can be neglected.
Resp.: We clarify in the manuscript that the derived equations described in this paper are applicable to a quasilinear regime.
2. Thus, by assuming that the waves are indeed sufficiently small in amplitude (clearly not the case for some of their events since delta B/B_0 >=1%) and that we are in a quasilinear regime, the transit time they are calculating with or without relativistic effects are comparable, with some minor differences of 0.10.01 ms. What would actually justify their thesis would be to show that the pitchangle diffusion coefficient they can compute from Delta_alpha (Equation 20) would lead to notable differences in the particle scattering. But they do not provide such an analysis and the change in the pitchangle shown in Table 1 (assuming again we are within a quasilinear regime despite the large amplitudes of the waves) are essentially identical for both relativistic and nonlinear relativistic effects with differences of the order 1/10 or 1/100.
Resp.: We thank the referee for this point, which improves the manuscript. As we are interested in showing the relevance of a more complete relativistic description in linear waveparticle events, we choose periods in which linear processes are likely in the previous events and substitute case 2 for a new event. Then we revised the periods selected for each event and chose a linear one. Besides, we calculate the pitch angle diffusion coefficient (Da) following the same approach as done by Lakhina et al., 2010. The results are summarized in Table 1 (attached). The comparison between nonrelativistic and complete relativistic calculations shows that the interaction time is around 4 times higher when the Special Relativity kinematics is considered. Also, the diffusion coefficient rates show notable differences in the pitch angle scattering.
3. If we are interested with the nonlinear regime, the transit time they compute only make sense when compared with some nonlinear timescales, such as the trapping time. But since their transit time are essentially identitical I don't see how relativistic effect could turn a linear interaction into a nonlinear one either. I am therefore not certain how the paper could be salvaged since the relativistic effect they study seems to have no impact for both linear and nonlinear waveparticle interactions. If the editors are willing to accept a null result, the authors could perhaps compute the diffusion coefficients with relativistic effects included, and if the difference is marginal publish it as such.
Resp.: Accordingly, we show that for the selected case studies, the relativistic diffusion coefficient rates in Table 1 (attached) can be more than 5 times higher than the nonrelativistic diffusion rates.

AC1: 'Reply on RC2', Livia R. Alves, 10 May 2023
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