IMF direction derived from cycloid-like ion distributions observed by mars express
- M. Yamauchi*
- , Y. Futaana
- , A. Fedorov
- , E. Dubinin
- , R. Lundin
- , J. A. Sauvaud
- , D. Winningham
- , R. Frahm
- , S. Barabash
- , M. Holmstrom
- , J. Woch
- , M. Fraenz
- , E. Budnik
- , H. Borg
- , J. R. Sharber
- , A. J. Coates
- , Y. Soobiah
- , H. Koskinen
- , E. Kallio
- , K. Asamura
*Awdur cyfatebol y gwaith hwn
- Swedish Institute of Space Physics
- Japan Aerospace Exploration Agency
- Centre d'Etudes Supérieures de la Renaissance
- Max Planck Institute for Solar System Research
- Southwest Research Institute
- University College London
- Finnish Meteorological Institute
- University of Helsinki
- University of Arizona
- Rutherford Appleton Laboratory
- University of Bern
- INAF-Istituto di Fisica dello Spazio Interplanetario
- Johns Hopkins University
- National University of Ireland, Maynooth
- University of Michigan
- University of California, Berkeley
Allbwn ymchwil: Cyfraniad at gyfnodolyn › Erthygl › adolygiad gan gymheiriaid
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Dyfyniadau
(Scopus)