Articles | Volume 34, issue 11
https://doi.org/10.5194/angeo-34-1099-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-34-1099-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Regular paper
| 
23 Nov 2016
Regular paper |
| 23 Nov 2016
Mirror mode waves in Venus's magnetosheath: solar minimum vs. solar maximum
Space Research Institute, Austrian Academy of Sciences, Graz,
Austria
Daniel Schmid
Space Research Institute, Austrian Academy of Sciences, Graz,
Austria
University of Graz, NAWI Graz, Graz, Austria
Bruce T. Tsurutani
California Institute of Technology, Pasadena, California, USA
Magda Delva
Space Research Institute, Austrian Academy of Sciences, Graz,
Austria
Ferdinand Plaschke
Space Research Institute, Austrian Academy of Sciences, Graz,
Austria
Yasuhito Narita
Space Research Institute, Austrian Academy of Sciences, Graz,
Austria
Tielong Zhang
Space Research Institute, Austrian Academy of Sciences, Graz,
Austria
CAS Key Laboratory of Geospace Environment, University of Science
and Technology of China, Hefei, China
Karl-Heinz Glassmeier
Institute for Geophysics and
Extraterrestrial Physics, TU Braunschweig, Braunschweig, Germany
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Cited
21 citations as recorded by crossref.
- Solar Orbiter’s first Venus flyby M. Volwerk et al. 10.1051/0004-6361/202140910
- Oxygen Ion Escape From Venus Is Modulated by Ultra‐Low Frequency Waves R. Jarvinen et al. 10.1029/2020GL087462
- Ultra low frequency waves at Venus: Observations by the Venus Express spacecraft M. Fränz et al. 10.1016/j.pss.2017.08.011
- Statistical analysis of mirror mode waves in sheath regions driven by interplanetary coronal mass ejection M. Ala-Lahti et al. 10.5194/angeo-36-793-2018
- A Review of Alfvénic Turbulence in High-Speed Solar Wind Streams: Hints From Cometary Plasma Turbulence B. Tsurutani et al. 10.1002/2017JA024203
- The BepiColombo Planetary Magnetometer MPO-MAG: What Can We Learn from the Hermean Magnetic Field? D. Heyner et al. 10.1007/s11214-021-00822-x
- Making Waves: Mirror Mode Structures Around Mars Observed by the MAVEN Spacecraft C. Simon Wedlund et al. 10.1029/2021JA029811
- Proton Temperature Anisotropies in the Venus Plasma Environment During Solar Minimum and Maximum S. Rojas Mata et al. 10.1029/2021JA029611
- Electron magnetosonic waves and sub-ion magnetic holes in the magnetotail plasma P. Shustov et al. 10.1063/5.0075938
- A Fast Bow Shock Location Predictor‐Estimator From 2D and 3D Analytical Models: Application to Mars and the MAVEN Mission C. Simon Wedlund et al. 10.1029/2021JA029942
- Kinetic‐Scale Turbulence in the Venusian Magnetosheath T. Bowen et al. 10.1029/2020GL090783
- Stimulated Mirror Instability From the Interplay of Anisotropic Protons and Electrons, and their Suprathermal Populations S. Shaaban et al. 10.1002/2017JA025066
- Venus's induced magnetosphere during active solar wind conditions at BepiColombo's Venus 1 flyby M. Volwerk et al. 10.5194/angeo-39-811-2021
- Effect of streaming velocity, magnetic field, and higher-order correction on the nature of ion acoustic solitons in the Venusian ionosphere A. Fayad et al. 10.1088/1402-4896/abdbf4
- Statistical Properties of Electron-scale Magnetic Peaks in the Solar Wind at 1 au G. Wang et al. 10.3847/1538-4357/ac1c6c
- 3D Magnetic Holes in Collisionless Plasmas P. Shustov et al. 10.1134/S1063780X18080068
- BepiColombo Science Investigations During Cruise and Flybys at the Earth, Venus and Mercury V. Mangano et al. 10.1007/s11214-021-00797-9
- Foreshock as a Source Region of Electron-scale Magnetic Holes in the Solar Wind at 1 au G. Wang et al. 10.3847/1538-4357/abfd31
- Plasma Waves Around Venus and Mars V. Yadav 10.1080/02564602.2020.1819889
- Compiling Magnetosheath Statistical Data Sets Under Specific Solar Wind Conditions: Lessons Learnt From the Dayside Kinetic Southward IMF GEM Challenge A. Dimmock et al. 10.1029/2020EA001095
- Proton Temperature Anisotropies in the Plasma Environment of Venus A. Bader et al. 10.1029/2019JA026619
Latest update: 05 Jun 2023
Short summary
The behaviour of mirror mode waves in Venus's magnetosheath is investigated for solar minimum and maximum conditions. It is shown that the total observational rate of these waves does not change much; however, the distribution over the magnetosheath is significantly different, as well as the growth and decay of the waves during these different solar activity conditions.
The behaviour of mirror mode waves in Venus's magnetosheath is investigated for solar minimum...
