An improved expected temperature formula for identifying interplanetary coronal mass ejections-Reference-Cited by-同舟云学术

An improved expected temperature formula for identifying interplanetary coronal mass ejections

Published:2005-04 Issue:A4 Volume:110 Page:
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res.

Author:

Elliott H. A.¹,McComas D. J.¹,Schwadron N. A.¹,Gosling J. T.²,Skoug R. M.²,Gloeckler G.³,Zurbuchen T. H.⁴

Affiliation:

1. Space Science and Engineering; Southwest Research Institute; San Antonio Texas USA

2. Los Alamos National Laboratory; Los Alamos New Mexico USA

3. Department of Physics; University of Maryland; College Park Maryland USA

4. Department of Atmospheric, Oceanic, and Space Science; University of Michigan; Ann Arbor Michigan 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

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1029/2004JA010794/fullpdf

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5. Investigation of the composition of solar and interstellar matter using solar wind and pickup ion measurements with SWICS and SWIMS on ACE;Gloeckler;Space Sci. Rev.,1998

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