Articles | Volume 33, issue 10
https://doi.org/10.5194/angeo-33-1271-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Special issue:
https://doi.org/10.5194/angeo-33-1271-2015
© Author(s) 2015. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Regular paper
| 
16 Oct 2015
Regular paper |
| 16 Oct 2015
The relationship between plasmapause, solar wind and geomagnetic activity between 2007 and 2011
G. Verbanac
CORRESPONDING AUTHOR
Department of Geophysics, University of Zagreb, Zagreb, Croatia
V. Pierrard
Belgian Institute for Space Aeronomy (Space Physics and STCE), 3 Av. Circulaire, 1180 Brussels, Belgium
Université Catholique de Louvain, TECLIM, Earth and Life Institute, Place Louis Pasteur 3 bte L4.03.08, 1348 Louvain-La-Neuve, Belgium
M. Bandić
Preziosastr. 15a, 81927 München, Germany
F. Darrouzet
Belgian Institute for Space Aeronomy (Space Physics and STCE), 3 Av. Circulaire, 1180 Brussels, Belgium
J.-L. Rauch
Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Orléans, France
P. Décréau
Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Orléans, France
Viewed
Total article views: 1,777 (including HTML, PDF, and XML)
Cumulative views and downloads
(calculated since 16 Oct 2015)
| HTML | XML | Total | BibTeX | EndNote | |
|---|---|---|---|---|---|
| 1,019 | 690 | 68 | 1,777 | 78 | 88 |
- HTML: 1,019
- PDF: 690
- XML: 68
- Total: 1,777
- BibTeX: 78
- EndNote: 88
Cited
30 citations as recorded by crossref.
- MLT dependence in the relationship between plasmapause, solar wind, and geomagnetic activity based on CRRES: 1990–1991 M. Bandić et al. 10.1002/2015JA022278
- Prediction of Dynamic Plasmapause Location Using a Neural Network D. Guo et al. 10.1029/2020SW002622
- The Role of Plasmasphere in the Formation of Electron Heat Fluxes G. Khazanov et al. 10.1029/2023JA032013
- Satellite observations and modeling of the plasmapause structure and dynamics S. Watanabe et al. 10.1016/j.asr.2024.10.015
- Coincident Observations by the Kharkiv IS Radar and Ionosonde, DMSP and Arase (ERG) Satellites, and FLIP Model Simulations: Implications for the NRLMSISE‐00 Hydrogen Density, Plasmasphere, and Ionosphere D. Kotov et al. 10.1029/2018GL079206
- Influence of the solar wind high-speed streams on the thermospheric neutral density during the declining phase of solar cycle 23 G. Verbanac et al. 10.1016/j.asr.2022.03.032
- The distribution of plasmaspheric hiss wave power with respect to plasmapause location D. Malaspina et al. 10.1002/2016GL069982
- Regular Density Inhomogeneities in the Boundary Layer of the Plasmasphere G. Kotova et al. 10.1134/S0016793223600674
- The Midlatitude Trough and the Plasmapause in the Nighttime Ionosphere Simultaneously Observed by DEMETER During 2006–2009 C. Chen et al. 10.1029/2017JA024840
- Evidence of MLT propagation of the plasmapause inferred from THEMIS data M. Bandić et al. 10.1016/j.jastp.2017.05.005
- A Tomographic Method for the Reconstruction of the Plasmasphere Based on COSMIC/ FORMOSAT-3 Data F. Prol & M. Hoque 10.1109/JSTARS.2022.3155926
- Relationship Between Global Plasmapause Characteristics and Plasmapause Structures in the Frame of Interchange Instability Mechanism M. Bandić et al. 10.1029/2019JA026768
- Relative Timing of Nightside and Dayside Plasmapause Motion: Two Events in June 2001 J. Goldstein & B. Sandel 10.1029/2019JA027153
- Modeling the Dynamics of Radiation Belt Electrons With Source and Loss Driven by the Solar Wind Z. Xiang et al. 10.1029/2020JA028988
- The Spatio-Temporal Features of Pc1 Structured Geomagnetic Pulsations B. Klain & N. Kurazhkovskaya 10.1134/S0016793222600618
- Improving Predictions of the 3D Dynamic Model of the Plasmasphere V. Pierrard et al. 10.3389/fspas.2021.681401
- Plasmasphere and topside ionosphere reconstruction using METOP satellite data during geomagnetic storms F. Prol et al. 10.1051/swsc/2020076
- A Statistical Model of Inner Magnetospheric Electron Density: Van Allen Probes Observations J. Lv et al. 10.1029/2022SW003182
- Epoch‐Based Model for Stormtime Plasmapause Location J. Goldstein et al. 10.1029/2018JA025996
- Statistics and Empirical Models of the Plasmasphere Boundaries From the Van Allen Probes for Radiation Belt Physics J. Ripoll et al. 10.1029/2022GL101402
- Modeling of the cold electron plasma density for radiation belt physics J. Ripoll et al. 10.3389/fspas.2023.1096595
- Links of the Plasmapause With Other Boundary Layers of the Magnetosphere: Ionospheric Convection, Radiation Belt Boundaries, Auroral Oval V. Pierrard et al. 10.3389/fspas.2021.728531
- Does the Time Resolution of the Geoeffective IMF Component Influence Its Annual, Semiannual and Diurnal Patterns? S. Živković et al. 10.1007/s11207-023-02184-9
- Narrow-band emission with 0.5 to 3.5 Hz varying frequency in the background of the main phase of the 17 March 2013 magnetic storm А. Потапов et al. 10.12737/24271
- MLT Plasmapause Characteristics: Comparison Between THEMIS Observations and Numerical Simulations G. Verbanac et al. 10.1002/2017JA024573
- The Spatio-Temporal Features of Pc1 Structured Geomagnetic Pulsations B. Klain & N. Kurazhkovskaya 10.31857/S0016794022600429
- Experimental Study of the Plasmasphere Boundary Layer Using MAGION 5 Data G. Kotova et al. 10.1002/2017JA024590
- Development of a 3‐D Plasmapause Model With a Back‐Propagation Neural Network Z. Zheng et al. 10.1029/2019SW002360
- Postmidnight ionospheric troughs in summer at high latitudes M. Voiculescu et al. 10.1002/2016JA023360
- Regular Density Inhomogeneities in the Boundary Layer of the Plasmasphere G. Kotova et al. 10.31857/S0016794023700013
Latest update: 27 Dec 2024
Short summary
Using Cluster data, we develop plasmapause Lpp models parameterized by solar wind coupling functions and geomagnetic activity indices. We show that the Lpp response to the changes in the interplanetary conditions depends on the magnetic local time. The faster plasmapause response is observed in the post-midnight sector. At low activity, Lpp exhibits the largest values on the dayside. For enhanced activity, displacements towards larger values on the evening side are identified.
Using Cluster data, we develop plasmapause Lpp models parameterized by solar wind coupling...
Special issue