Bulk Properties of Solar Wind Protons: Inter-comparison of Observations From STEREO, SOHO, ACE, and WIND

Details Bulk Properties of Solar Wind Protons: Inter-comparison of Observations From STEREO, SOHO, ACE, and WIND Bulk Properties of Solar Wind Protons: Inter-comparison of Observations From STEREO, SOHO, ACE, and WIND

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agusmsh41a..10s&link_type=abstract

American Geophysical Union, Spring Meeting 2007, abstract #SH41A-10

Physics

2164 Solar Wind Plasma, 2194 Instruments And Techniques

Scientific paper

The twin STEREO observatories were launched in October 2006. The PLASTIC experiment onboard both spacecraft analyzes ions with energies between 0.25 and 80 keV/charge, including solar wind protons. Information on bulk properties such as density, speed, and temperature are obtained. In early 2007 STEREO A was separated from SOHO, ACE, WIND, and STEREO B by hundreds of earth radii within the ecliptic plane, and by tens of earth radii out of the ecliptic plane. We report on comparisons of bulk parameters between these spacecraft, and what they show us about small-scale temporal and spatial variations in the solar wind.

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