Uneven compression levels of Earth's magnetic fields by shocked solar wind

Author:

Shue J.-H.1,Chen Y.-S.1,Hsieh W.-C.1,Nowada M.1,Lee B. S.1,Song P.2,Russell C. T.3,Angelopoulos V.3,Glassmeier K. H.4,McFadden J. P.5,Larson D.5

Affiliation:

1. Institute of Space Science; National Central University; Jhongli Taiwan

2. Center for Atmospheric Research; University of Massachusetts Lowell; Lowell Massachusetts USA

3. Institute of Geophysics and Planetary Physics; University of California; Los Angeles California USA

4. Institute of Geophysics and Extraterrestrial Physics; Technical University Braunschweig; Braunschweig Germany

5. Space Sciences Laboratory; University of California; Berkeley California USA

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

Reference25 articles.

1. The THEMIS mission;Angelopoulos;Space Sci. Rev.,2008

2. Modeling the size and shape of Saturn's magnetopause with variable dynamic pressure;Arridge;J. Geophys. Res.,2006

3. Inward motion of the magnetopause before a substorm;Aubry;J. Geophys. Res.,1970

4. The THEMIS fluxgate magnetometer;Auster;Space Sci. Rev.,2008

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