Zobrazeno 1 - 10
of 203
pro vyhledávání: '"Martin Volwerk"'
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
Externí odkaz:
https://doaj.org/article/e1b2d58fac6e4f4ea9366558c762c32d
Autor:
Cyril Simon Wedlund, Martin Volwerk, Christian Mazelle, Sebastián Rojas Mata, Gabriella Stenberg Wieser, Yoshifumi Futaana, Jasper Halekas, Diana Rojas-Castillo, César Bertucci, Jared Espley
In this series of papers, we present statistical maps of mirror-mode-like (MM) structures in the magnetosheaths of Mars and Venus and calculate the probability of detecting them in spacecraft data. We aim to study and compare them with the same tools
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d81517176b7fd08a30cbc4c8820b068b
https://angeo.copernicus.org/articles/41/225/2023/
https://angeo.copernicus.org/articles/41/225/2023/
Autor:
Cyril Simon Wedlund, Martin Volwerk, Christian Mazelle, Sebastián Rojas Mata, Gabriella Stenberg Wieser, Yoshifumi Futaana, Jasper Halekas, Diana Rojas-Castillo, César Bertucci, Jared Espley
Publikováno v:
eISSN
In this series of papers, we present statistical maps of mirror mode-like (MM) structures in the magnetosheaths of Mars and Venus and calculate the probability of detecting them in spacecraft data. We aim to study and compare them with the same tools
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d767b4b2681cf3d21c48db5e6d91d9bc
https://egusphere.copernicus.org/preprints/2022/egusphere-2022-634/
https://egusphere.copernicus.org/preprints/2022/egusphere-2022-634/
Autor:
Daniel Schmid, David Fischer, Werner Magnes, Yasuhito Narita, Martin Volwerk, Wolfgang Baumjohann, Ayako Matsuoka, Hans-Ulrich Auster, Ingo Richter, Daniel Heyner, Ferdinand Plaschke, Rumi Nakamura
BepiColombo MPO and Mio spacecraft encounter the Mercury magnetosphere six times from 2021 to 2025 during the flyby maneuvers. Each flyby trajectory is unique and includes the magnetospheric regions that were not covered by MESSENGER. Mio/MGF magneti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::61b41b59b2408f3963b14917f2b6f93c
https://doi.org/10.5194/egusphere-egu23-12906
https://doi.org/10.5194/egusphere-egu23-12906
Autor:
Daniel Heyner, Kristin Pump, David Hercik, Willi Exner, Yasuhito Narita, Ferdinand Plaschke, Daniel Schmid, Jim Slavin, Martin Volwerk
Mercury possesses a weak planetary dipole moment and is subject to a strong solar wind inflow. Thus, a small magnetosphere is formed. On the nightside, a neutral current sheet elongates the magnetic field lines to form a magnetotail. From hybrid simu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2350ccba225ca29b0ae366600b8864f4
https://doi.org/10.5194/egusphere-egu23-11546
https://doi.org/10.5194/egusphere-egu23-11546
Autor:
Martin Volwerk, Cyril Simon Wedlund, David Mautner, Sebastian Rojas Mata, Gabriella Stenberg Wieser, Yoshifumi Futaana, Markus Fraenz, Christian Mazelle, Diana Rojas-Castillo, Cesar Bertucci, Magda Delva
Temperature anisotropy-driven instabilities such as the mirror mode and ion cyclotron instabilities are responsible for the generation of waves in the turbulent magnetosheath of planets. We present here a statistical study of mirror mode-like structu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::54903f9149994fe1d7e8bc2fea0669db
https://doi.org/10.5194/egusphere-egu23-1532
https://doi.org/10.5194/egusphere-egu23-1532
Autor:
Ferdinand Plaschke, Martin Volwerk, Tomas Karlsson, Charlotte Götz, Daniel Heyner, Heli Hietala, Johannes Z. D. Mieth, Daniel Schmid, Cyril Simon-Wedlund, Zoltan Vörös
Magnetic holes are significant depressions of the interplanetary magnetic field (IMF) that can be found embedded in the solar wind everywhere within the heliosphere. They resemble mirror mode magnetic structures that form as a response to excess perp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3469ff5f680f7f9cd87d5b17e7065c6e
https://doi.org/10.5194/egusphere-egu23-4366
https://doi.org/10.5194/egusphere-egu23-4366
Autor:
Adriana Settino, Rumi Nakamura, Kevin A. Blasl, Takuma Nakamura, Denise Perrone, Francesco Valentini, Owen Wyn Roberts, Evgeny Panov, Zoltan Vörös, Martin Volwerk, Daniel Schmid, Martin Hosner, Daniel B. Graham, Yuri V. Khotyaintsev
The Kelvin-Helmholtz (KH) instability is a shear-driven instability commonly observed at the Earth’s magnetopause under different solar wind conditions. The evolution of the KH instability is characterised by the nonlinear coupling of different mod
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b7e64cbcbd4a66c5dc1e57d73a93a6cd
https://doi.org/10.5194/egusphere-egu23-12262
https://doi.org/10.5194/egusphere-egu23-12262