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.
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
31 citations as recorded by crossref.
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- Statistical distribution of mirror-mode-like structures in the magnetosheaths of unmagnetised planets – Part 1: Mars as observed by the MAVEN spacecraft C. Simon Wedlund et al. 10.5194/angeo-41-225-2023
- Oxygen Ion Escape From Venus Is Modulated by Ultra‐Low Frequency Waves R. Jarvinen et al. 10.1029/2020GL087462
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Latest update: 16 Aug 2024
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...