Articles | Volume 39, issue 1
https://doi.org/10.5194/angeo-39-135-2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/angeo-39-135-2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
D-region impact area of energetic electron precipitation during pulsating aurora
Emma Bland
CORRESPONDING AUTHOR
Department of Arctic Geophysics, University Centre in Svalbard, Longyearbyen, Norway
Fasil Tesema
Department of Arctic Geophysics, University Centre in Svalbard, Longyearbyen, Norway
Birkeland Centre for Space Science, University of Bergen, Bergen, Norway
Noora Partamies
Department of Arctic Geophysics, University Centre in Svalbard, Longyearbyen, Norway
Birkeland Centre for Space Science, University of Bergen, Bergen, Norway
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Auroral displays typically take place at high latitudes, but the exact latitude where the auroral breakup occurs can vary. In this study, we compare the characteristics of the fluxes of precipitating electrons from space during auroral breakups occurring above Tromsø (central part of the auroral zone) and above Svalbard (poleward boundary of the auroral zone). We find that electrons responsible for the aurora above Tromsø carry more energy than those precipitating above Svalbard.
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Auroral imaging produces large amounts of image data that can no longer be analyzed by visual inspection. Thus, every step towards automatic analysis tools is crucial. Previously supervised learning methods have been used in auroral physics, with a human expert providing ground truth. However, this ground truth is debatable. We present an unsupervised learning method, which shows promising results in detecting auroral breakups in the all-sky image data.
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We investigate the local time behaviour of auroral structures and emission height. Data are collected from the Fennoscandian Lapland and Svalbard latitutes from 7 identical auroral all-sky cameras over about 1 solar cycle. The typical peak emission height of the green aurora varies from 110 km on the nightside to about 118 km in the morning over Lapland but stays systematically higher over Svalbard. During fast solar wind, nightside emission heights are 5 km lower than during slow solar wind.
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This paper is the first to simulate and analyse the pulsating aurorae impact on middle atmosphere on monthly/seasonal timescales. We find that pulsating aurorae have the potential to make a considerable contribution to the total energetic particle forcing and increase the impact on upper stratospheric odd nitrogen and ozone in the polar regions. Thus, it should be considered in atmospheric and climate simulations.
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Small-scale auroral features are still being discovered and are not well understood. Where aurorae are caused by particle precipitation, the newly reported fragmented aurora-like emissions (FAEs) seem to be locally generated in the ionosphere (hence,
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Noora Partamies, Fasil Tesema, Emma Bland, Erkka Heino, Hilde Nesse Tyssøy, and Erlend Kallelid
Ann. Geophys., 39, 69–83, https://doi.org/10.5194/angeo-39-69-2021, https://doi.org/10.5194/angeo-39-69-2021, 2021
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About 200 nights of substorm activity have been analysed for their magnetic disturbance magnitude and the level of cosmic radio noise absorption. We show that substorms with a single expansion phase have limited lifetimes and spatial extents. Starting from magnetically quiet conditions, the strongest absorption occurs after 1 to 2 nights of substorm activity. This prolonged activity is thus required to accelerate particles to energies, which may affect the atmospheric chemistry.
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Ann. Geophys., 38, 1191–1202, https://doi.org/10.5194/angeo-38-1191-2020, https://doi.org/10.5194/angeo-38-1191-2020, 2020
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In this study, we present the ionization level from EISCAT radar experiments and cosmic noise absorption level
from KAIRA riometer observations during pulsating auroras. We found thick layers of ionization that reach down
to 70 km (harder precipitation) and higher cosmic noise absorption during patchy pulsating aurora than
during amorphous pulsating and patchy auroras.
Cited articles
Berkey, F. T., Driatskiy, V. M., Henriksen, K., Hultqvist, B., Jelly, D. H.,
Shchuka, T. I., Theander, A., and Ylindemi, J.: A synoptic investigation of
particle precipitation dynamics for 60 substorms in IQSY (1964–1965) and
IASY (1969), Planet. Space Sci., 22, 255–307,
https://doi.org/10.1016/0032-0633(74)90028-2, 1974. a
Berngardt, O. I.: Noise level forecasts at 8–20 MHz and their use for
morphological studies of ionospheric absorption variations at EKB ISTP SB
RAS radar, Adv. Space Res., 66, 278–291, https://doi.org/10.1016/j.asr.2020.04.005, 2020. a, b, c
Berngardt, O. I., Ruohoniemi, J. M., Nishitani, N., Shepherd, S. G., Bristow,
W. A., and Miller, E. S.: Attenuation of decameter wavelength sky noise
during x-ray solar flares in 2013–2017 based on the observations of
midlatitude HF radars, J. Atmos. Sol.-Terr.
Phy., 173, 1–13, https://doi.org/10.1016/j.jastp.2018.03.022, 2018. a
Bland, E. C., Heino, E., Kosch, M. J., and Partamies, N.: SuperDARN
Radar-Derived HF Radio Attenuation During the September 2017 Solar Proton
Events, Space Weather, 16, 1455–1469, https://doi.org/10.1029/2018SW001916, 2018. a, b, c, d
British Antarctic Survey: Super Dual Auroral Radar Network, available at: https://www.bas.ac.uk/project/superdarn, last access: 1 June 2020. a
Chakraborty, S., Ruohoniemi, J. M., Baker, J. B. H., and Nishitani, N.:
Characterization of Short-Wave Fadeout seen in Daytime SuperDARN Ground
Scatter Observations, Radio Sci., 53, 472–484, https://doi.org/10.1002/2017RS006488, 2018. a
Chakraborty, S., Baker, J. B. H., Ruohoniemi, J. M., Kunduri, B., Nishitani,
N., and Shepherd, S. G.: A Study of SuperDARN Response to Co-occurring
Space Weather Phenomena, Space Weather, 17, 1351–1363,
https://doi.org/10.1029/2019SW002179, 2019. a
Chisham, G., Lester, M., Milan, S. E., Freeman, M. P., Bristow, W. A., Grocott,
A., McWilliams, K. A., Ruohoniemi, J. M., Yeoman, T. K., Dyson, P. L.,
Greenwald, R. A., Kikuchi, T., Pinnock, M., Rash, J. P. S., Sato, N., Sofko,
G. J., Villain, J. P., and Walker, A. D. M.: A decade of the Super Dual
Auroral Radar Network (SuperDARN): Scientific achievements, new
techniques and future directions, Surv. Geophys., 28, 33–109,
https://doi.org/10.1007/s10712-007-9017-8, 2007. a
Cresswell-Moorcock, K., Rodger, C. J., Kero, A., Collier, A. B., Clilverd,
M. A., Häggström, I., and Pitkänen, T.: A reexamination of
latitudinal limits of substorm-produced energetic electron precipitation,
J. Geophys. Res.-Space, 118, 6694–6705,
https://doi.org/10.1002/jgra.50598, 2013. a, b
Donovan, E., Mende, S., Jackel, B., Frey, H., Syrjäsuo, M., Voronkov, I. Trondsen, T., Peticolas, L., Angelopoulos, V., Harris, S., Greffen, M., and Connors, M.: The
THEMIS all-sky imaging array – System design and initial results from the
prototype imager, J. Atmos. Sol.-Terr. Phy., 68,
1472–1487, 2006. a
Fang, X., Randall, C. E., Lummerzheim, D., Solomon, S. C., Mills, M. J., Marsh,
D. R., Jackman, C. H., Wang, W., and Lu, G.: Electron impact ionization: A
new parameterization for 100 eV to 1 MeV electrons, J.
Geophys. Res.-Space, 113, A09311, https://doi.org/10.1029/2008JA013384, 2008. a
Fiori, R. A. D., Koustov, A. V., Chakraborty, S., Ruohoniemi, J. M., Danskin,
D. W., Boteler, D. H., and Shepherd, S. G.: Examining the potential of the
Super Dual Auroral Radar Network for monitoring the space weather
impact of solar X-ray flares, Space Weather, 16, 1348–1362, https://doi.org/10.1029/2018SW001905, 2018. a
Greenwald, R. A., Baker, K. B., Dudeney, J. R., Pinnock, M., Jones, T. B.,
Thomas, E. C., Villain, J. P., Cerisier, J. C., Senior, C., Hanuise, C.,
Hunsucker, R. D., Sofko, G. J., Koehler, J., Nielsen, E., Pellinen, R.,
Walker, A. D. M., Sato, N., and Yamagishi, H.: DARN/SuperDARN: A Global
View of the Dynamics of High-Latitude Convection, Space Sci. Rev., 71,
761–796, https://doi.org/10.1007/BF00751350, 1995. a
Grono, E. and Donovan, E.: Differentiating diffuse auroras based on phenomenology, Ann. Geophys., 36, 891–898, https://doi.org/10.5194/angeo-36-891-2018, 2018. a, b
Grono, E. and Donovan, E.: Constraining the Source Regions of Pulsating
Auroras, Geophys. Res. Lett., 46, 10267–10273, https://doi.org/10.1029/2019GL084611, 2019. a, b
Jones, S. L., Lessard, M. R., Rychert, K., Spanswick, E., and Donovan, E.:
Large-scale aspects and temporal evolution of pulsating aurora, J.
Geophys. Res.-Space, 116, A03214, https://doi.org/10.1029/2010JA015840, 2011. a, b, c, d
Jones, S. L., Lessard, M. R., Rychert, K., Spanswick, E., Donovan, E., and
Jaynes, A. N.: Persistent, widespread pulsating aurora: A case study, J. Geophys. Res.-Space, 118, 2998–3006,
https://doi.org/10.1002/jgra.50301, 2013. a, b, c, d
Juusola, L., Østgaard, N., Tanskanen, E., Partamies, N., and Snekvik, K.:
Earthward plasma sheet flows during substorm phases, J. Geophys.
Res.-Space, 116, A10228, https://doi.org/10.1029/2011JA016852, 2011. a
Kasahara, S., Miyoshi, Y., Yokota, S., Mitani, T., Kasahara, Y., Matsuda, S., Kumamoto, A., Matsuoka, A., Kazama, Y., Frey, H. U., Angelopoulos, V., Kurita, S., Keika, K., Seki, K., and Shinohara, I.: Pulsating aurora
from electron scattering by chorus waves, Nature, 554, 337–340, https://doi.org/10.1038/nature25505, 2018. a
Kvifte, G. J. and Pettersen, H.: Morphology of the pulsating aurora, Planet. Space Sci., 17, 1599–1607, https://doi.org/10.1016/0032-0633(69)90148-2, 1969. a
Lessard, M. R.: A review of pulsating aurora, Auroral phenomenology and
magnetospheric processes: Earth and Other Planets, 197, 55–68, https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2011GM001187 (last access: 8 February 2021), 2012. a
Marsh, D., Garcia, R., Kinnison, D., Boville, B., Sassi, F., Solomon, S., and
Matthes, K.: Modeling the whole atmosphere response to solar cycle changes in
radiative and geomagnetic forcing, J. Geophys. Res.-Atmos., 112, D23306, https://doi.org/10.1029/2006JD008306, 2007. a, b
Milan, S. E., Jones, T. B., Robinson, T. R., Thomas, E. C., and Yeoman, T. K.: Interferometric evidence for the observation of ground backscatter originating behind the CUTLASS coherent HF radars, Ann. Geophys., 15, 29–39, https://doi.org/10.1007/s00585-997-0029-y, 1997. a
Miyoshi, Y., Katoh, Y., Nishiyama, T., Sakanoi, T., Asamura, K., and Hirahara,
M.: Time of flight analysis of pulsating aurora electrons, considering
wave-particle interactions with propagating whistler mode waves, J.
Geophys. Res.-Space, 115, A10312, https://doi.org/10.1029/2009JA015127, 2010. a
Miyoshi, Y., Oyama, S., Saito, S., Kurita, S., Fujiwara, H., Kataoka, R., Ebihara, Y., Kletzing, C., Reeves, G., Santolik, O., Clilverd, M., Rodger, C. J., Turunen, E., and Tsuchiya, F.: Energetic
electron precipitation associated with pulsating aurora: EISCAT and Van
Allen Probe observations, J. Geophys. Res.-Space,
120, 2754–2766, https://doi.org/10.1002/2014JA020690, 2015. a
NASA: GSFC/SPDF OMNIWeb interface, available at: https://omniweb.gsfc.nasa.gov, last access: 1 June 2020. a
National Institute of Polar Research, Japan: Syowa Color Digital Camera (CDC), available at: http://polaris.nipr.ac.jp/~acaurora/syowa_CDC_QL/, last access: 1 June 2020. a
Nishimura, Y., Lessard, M. R., Katoh, Y., Miyoshi, Y., Grono, E., Partamies, N., Sivadas, N., Hosokawa, K., Fukizawa, M., Samara, M., Michell, R. G., Kataoka, R., Sakanoi, T., Whiter, D. K., Oyama, S., Ogawa, Y., and Kurita, S.: Diffuse and
pulsating aurora, Space Sci. Rev., 216, 1–38, https://doi.org/10.1007/s11214-019-0629-3, 2020. a
Nishitani, N., Ruohoniemi, J. M., Lester, M., Baker, J. B. H., Koustov, A. V., Shepherd, S. G., Chisham, G., Hori, T., Thomas, E. G., Makarevich, R. A., Marchaudon, A., Ponomarenko, P., Wild, J. A., Milan, S. E., Bristow, W. A., Devlin, J., Miller, E., Greenwald, R. A., Ogawa, T., and Kikuchi, T.: Review of the accomplishments of mid-latitude Super Dual
Auroral Radar Network (SuperDARN) HF radars, Prog. Earth Planet. Sc., 6, 1–57, https://doi.org/10.1186/s40645-019-0270-5, 2019. a, b
Oguti, T., Kokubun, S., Hayashi, K., Tsuruda, K., Machida, S., Kitamura, T.,
Saka, O., and Watanabe, T.: Statistics of pulsating auroras on the basis of
all-sky TV data from five stations. I. Occurrence frequency, Can.
J. Phys., 59, 1150–1157, https://doi.org/10.1139/p81-152, 1981. a
Partamies, N., Juusola, L., Tanskanen, E., and Kauristie, K.: Statistical properties of substorms during different storm and solar cycle phases, Ann. Geophys., 31, 349–358, https://doi.org/10.5194/angeo-31-349-2013, 2013. a
Partamies, N., Whiter, D., Kadokura, A., Kauristie, K., Nesse Tyssøy, H.,
Massetti, S., Stauning, P., and Raita, T.: Occurrence and average behavior of
pulsating aurora, J. Geophys. Res.-Space, 122,
5606–5618, https://doi.org/10.1002/2017JA024039, 2017. a, b, c, d
SuperDARN Data Analysis Working Group, Thomas, E. G., Schmidt, M. T., Bland, E. C., Burrell, A. G., Ponomarenko, P. V., Reimer, A. S., Sterne, K. T., and Walach, M.-T.: SuperDARN Radar Software Toolkit (RST) 4.5, Zenodo, https://doi.org/10.5281/zenodo.801458, 2021. a
Tesema, F., Partamies, N., Nesse Tyssøy, H., Kero, A., and Smith-Johnsen,
C.: Observations of electron precipitation during pulsating aurora and its
chemical impact, J. Geophys. Res.-Space, 125,
e2019JA027713, https://doi.org/10.1029/2019JA027713, 2020a. a, b, c
Tesema, F., Partamies, N., Nesse Tyssøy, H., and McKay, D.: Observations of precipitation energies during different types of pulsating aurora, Ann. Geophys., 38, 1191–1202, https://doi.org/10.5194/angeo-38-1191-2020, 2020b. a, b, c
Thorne, R. M., Ni, B., Tao, X., Horne, R. B., and Meredith, N. P.: Scattering
by chorus waves as the dominant cause of diffuse auroral precipitation,
Nature, 467, 943–946, https://doi.org/10.1038/nature09467, 2010. a
Turunen, E., Verronen, P. T., Seppälä, A., Rodger, C. J., Clilverd,
M. A., Tamminen, J., Enell, C.-F., and Ulich, T.: Impact of different
energies of precipitating particles on NOx generation in the middle and
upper atmosphere during geomagnetic storms, J. Atmos.
Sol.-Terr. Phy., 71, 1176–1189, https://doi.org/10.1016/j.jastp.2008.07.005,
2009. a, b
Turunen, E., Kero, A., Verronen, P. T., Miyoshi, Y., Oyama, S.-I., and Saito,
S.: Mesospheric ozone destruction by high-energy electron precipitation
associated with pulsating aurora, J. Geophys. Res.-Atmos., 121, 11852–11861, https://doi.org/10.1002/2016JD025015, 2016. a
van de Kamp, M., Seppälä, A., Clilverd, M. A., Rodger, C. J., Verronen,
P. T., and Whittaker, I. C.: A model providing long-term data sets of
energetic electron precipitation during geomagnetic storms, J.
Geophys. Res.-Atmos., 121, 12520–12540, https://doi.org/10.1002/2015JD024212, 2016.
a
Verronen, P. T., Seppälä, A., Clilverd, M. A., Rodger, C. J., Kyrölä,
E., Enell, C.-F., Ulich, T., and Turunen, E.: Diurnal variation of ozone
depletion during the October–November 2003 solar proton events, J. Geophys. Res.-Space, 110, A09S32, https://doi.org/10.1029/2004JA010932,
2005. a
Verronen, P. T., Andersson, M. E., Marsh, D. R., Kovács, T., and Plane, J.
M. C.: WACCM-D – Whole Atmosphere Community Climate Model with
D-region ion chemistry, J. Adv. Model. Earth Sy., 8,
954–975, https://doi.org/10.1002/2015MS000592, 2016. a
Watanabe, D. and Nishitani, N.: Study of ionospheric disturbances during solar
flare events using the SuperDARN Hokkaido radar, Advances in Polar
Science, 24, 12–18, https://doi.org/10.3724/SP.J.1085.2013.00012, 2013. a
Yang, B., Donovan, E., Liang, J., and Spanswick, E.: A statistical study of the motion of pulsating aurora patches: using the THEMIS All-Sky Imager, Ann. Geophys., 35, 217–225, https://doi.org/10.5194/angeo-35-217-2017, 2017. a
Yang, B., Spanswick, E., Liang, J., Grono, E., and Donovan, E.: Responses of
Different Types of Pulsating Aurora in Cosmic Noise Absorption, Geophys.
Res. Lett., 46, 5717–5724, https://doi.org/10.1029/2019GL083289, 2019. a, b
Short summary
A total of 10 Super Dual Auroral Radar Network radars were used to estimate the horizontal area over which energetic electrons impact the atmosphere at 70–100 km altitude during pulsating aurorae (PsAs). The impact area varies significantly from event to event. Approximately one-third extend over 12° of magnetic latitude, while others are highly localised. Our results could be used to improve the forcing used in atmospheric/climate models to properly capture the energy contribution from PsAs.
A total of 10 Super Dual Auroral Radar Network radars were used to estimate the horizontal area...