In Which Magnetotail Hemisphere is a Satellite? Problems Using in Situ Magnetic Field Data
Author:
Affiliation:
1. Department of Physics Umeå University Umeå Sweden
2. Space Physics and Astronomy Research Unit University of Oulu Oulu Finland
Funder
Swedish National Space Agency
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1029/2020JA028923
Reference25 articles.
1. Bursty bulk flows in the inner central plasma sheet
2. The Cluster Magnetic Field Investigation: overview of in-flight performance and initial results
3. Average plasma properties in the central plasma sheet
4. Birn J.(1984).Three‐dimensional computer modeling of dynamic reconnection in the magnetotail: Plasmoid signatures in the near and distant tail. InMagnetic reconnection in space and laboratory plasmas(pp.264–271).American Geophysical Union (AGU). Retrieved fromhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/GM030p0264
5. Bursty bulk flows and dipolarization in MHD simulations of magnetotail reconnection
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