Magnetosheath for almost-aligned solar wind magnetic field and flow vectors: Wind observations across the dawnside magnetosheath at X = −12 Re

Author:

Farrugia C. J.1,Erkaev N. V.23,Torbert R. B.1,Biernat H. K.45,Gratton F. T.6,Szabo A.7,Kucharek H.1,Matsui H.1,Lin R. P.89,Ogilvie K. W.7,Lepping R. P.7,Smith C. W.1

Affiliation:

1. Space Science Center and Department of Physics; University of New Hampshire; Durham New Hampshire USA

2. Institute for Computational Modeling; Russian Academy of Sciences; Krasnoyarsk Russia

3. Siberian Federal University; Krasnoyarsk Russia

4. Space Research Institute; Austrian Academy of Sciences; Graz Austria

5. Institute for Theoretical Physics; University of Graz; Graz Austria

6. Instituto de Física del Plasma; Consejo Nacional de Investigaciones Científicas y Técnicas; Buenos Aires Argentina

7. Space Weather Laboratory; NASA Goddard Space Flight Center; Greenbelt Maryland USA

8. Physics Department and Space Sciences Laboratory; University of California; Berkeley California USA

9. School of Space Research; Kyung Hee University; Korea

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference34 articles.

1. ULF Signals Observed Near the Magnetopause

2. Flux transfer events on the magnetopause: Spatial distribution and controlling factors;Berchem;J. Geophys. Res.,1984

3. Quasi-parallel shock structure and processes;Burgess;Space Sci. Rev.,2005

4. Successive CMEs and complex ejecta;Burlaga;J. Geophys. Res.,2002

5. Results of the investigation of MHD flow around the magnetosphere;Erkaev;Geomagn. Aeron.,1988

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