Articles | Volume 39, issue 1
https://doi.org/10.5194/angeo-39-239-2021
© 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-39-239-2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Regular paper
| 
25 Feb 2021
Regular paper |
| 25 Feb 2021
| 25 Feb 2021
Statistical study of linear magnetic hole structures near Earth
Space Research Institute, Austrian Academy of Sciences, Graz, Austria
David Mautner
Space Research Institute, Austrian Academy of Sciences, Graz, Austria
Cyril Simon Wedlund
Space Research Institute, Austrian Academy of Sciences, Graz, Austria
Charlotte Goetz
ESTEC, European Space Agency, Keplerlaan 1, 2201AZ Noordwijk, the Netherlands
Ferdinand Plaschke
Space Research Institute, Austrian Academy of Sciences, Graz, Austria
Tomas Karlsson
Department of Space and Plasma Physics, School of Electrical Engineering and Computer Science, Royal Institute of Technology, Stockholm, Sweden
Daniel Schmid
Space Research Institute, Austrian Academy of Sciences, Graz, Austria
Diana Rojas-Castillo
Space Research Institute, Austrian Academy of Sciences, Graz, Austria
Instituto de Geofísica, UNAM, Ciudad Universitaria, Coyoacán, CP 04510, Mexico City, Mexico
Owen W. Roberts
Space Research Institute, Austrian Academy of Sciences, Graz, Austria
Ali Varsani
Space Research Institute, Austrian Academy of Sciences, Graz, Austria
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Cited
15 citations as recorded by crossref.
- Magnetic holes between Earth and Mercury: BepiColombo cruise phase M. Volwerk et al. 10.1051/0004-6361/202345879
- Electron-scale Magnetic Peaks Upstream of Mercury’s Bow Shock: MESSENGER Observations Y. Chen et al. 10.3847/1538-4357/ac80c0
- 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
- Solar Orbiter’s first Venus flyby: Observations from the Radio and Plasma Wave instrument L. Hadid et al. 10.1051/0004-6361/202140934
- Solar wind magnetic holes can cross the bow shock and enter the magnetosheath T. Karlsson et al. 10.5194/angeo-40-687-2022
- Statistical Study of Small-scale Magnetic Holes in the Upstream Regime of the Martian Bow Shock G. Wang et al. 10.3847/1538-4357/ac1c07
- Fluxgate Magnetometer Offset Vector Determination Using Current Sheets in the Solar Wind G. Wang & Z. Pan 10.3847/1538-4357/ac3d8f
- A New Method of Fluxgate Magnetometer Offset Vector Determination in the Solar Wind Using Any Magnetic Field Variations G. Wang 10.3847/1538-4357/ac822c
- A New Method to Calculate the Fluxgate Magnetometer Offset in the Interplanetary Magnetic Field: 2. Using Mirror Mode Structures G. Wang & Z. Pan 10.1029/2021JA029781
- Statistical Properties of Electron-scale Magnetic Peaks in the Solar Wind at 1 au G. Wang et al. 10.3847/1538-4357/ac1c6c
- A kinetic-scale magnetic hole in the magnetopause reconnection separatrix region Z. Li & M. Zhang 10.1093/mnras/stad1083
- Electron‐Scale Current Sheet as the Boundary of a Linear Magnetic Hole in the Terrestrial Current Sheet Observed by the Magnetospheric Multiscale Mission G. Wang et al. 10.1029/2021JA029707
- Study of the Electron‐Scale Magnetic Peaks in the Magnetotail Current Sheet Observed by the Magnetospheric Multiscale Mission Y. Chen et al. 10.1029/2021JA030135
- High-precision Calibration of the Fluxgate Magnetometer Offset Vector in the Terrestrial Magnetosheath G. Wang 10.3847/1538-4357/ac5907
- Scale‐Dependent Kurtosis of Magnetic Field Fluctuations in the Solar Wind: A Multi‐Scale Study With Cluster 2003–2015 O. Roberts et al. 10.1029/2021JA029483
14 citations as recorded by crossref.
- Magnetic holes between Earth and Mercury: BepiColombo cruise phase M. Volwerk et al. 10.1051/0004-6361/202345879
- Electron-scale Magnetic Peaks Upstream of Mercury’s Bow Shock: MESSENGER Observations Y. Chen et al. 10.3847/1538-4357/ac80c0
- 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
- Solar Orbiter’s first Venus flyby: Observations from the Radio and Plasma Wave instrument L. Hadid et al. 10.1051/0004-6361/202140934
- Solar wind magnetic holes can cross the bow shock and enter the magnetosheath T. Karlsson et al. 10.5194/angeo-40-687-2022
- Statistical Study of Small-scale Magnetic Holes in the Upstream Regime of the Martian Bow Shock G. Wang et al. 10.3847/1538-4357/ac1c07
- Fluxgate Magnetometer Offset Vector Determination Using Current Sheets in the Solar Wind G. Wang & Z. Pan 10.3847/1538-4357/ac3d8f
- A New Method of Fluxgate Magnetometer Offset Vector Determination in the Solar Wind Using Any Magnetic Field Variations G. Wang 10.3847/1538-4357/ac822c
- A New Method to Calculate the Fluxgate Magnetometer Offset in the Interplanetary Magnetic Field: 2. Using Mirror Mode Structures G. Wang & Z. Pan 10.1029/2021JA029781
- Statistical Properties of Electron-scale Magnetic Peaks in the Solar Wind at 1 au G. Wang et al. 10.3847/1538-4357/ac1c6c
- A kinetic-scale magnetic hole in the magnetopause reconnection separatrix region Z. Li & M. Zhang 10.1093/mnras/stad1083
- Electron‐Scale Current Sheet as the Boundary of a Linear Magnetic Hole in the Terrestrial Current Sheet Observed by the Magnetospheric Multiscale Mission G. Wang et al. 10.1029/2021JA029707
- Study of the Electron‐Scale Magnetic Peaks in the Magnetotail Current Sheet Observed by the Magnetospheric Multiscale Mission Y. Chen et al. 10.1029/2021JA030135
- High-precision Calibration of the Fluxgate Magnetometer Offset Vector in the Terrestrial Magnetosheath G. Wang 10.3847/1538-4357/ac5907
Latest update: 19 Apr 2024
Short summary
The magnetic field in the solar wind is not constant but varies in direction and strength. One of these variations shows a strong local reduction of the magnetic field strength and is called a magnetic hole. These holes are usually an indication that there is, or has been, a temperature difference in the plasma of the solar wind, with the temperature along the magnetic field lower than perpendicular. The MMS spacecraft data have been used to study the characteristics of these holes near Earth.
The magnetic field in the solar wind is not constant but varies in direction and strength. One...
