Temporal evolution of the solar wind in the ecliptic between Venus and Mars orbits

Details Temporal evolution of the solar wind in the ecliptic between Venus and Mars orbits Temporal evolution of the solar wind in the ecliptic between Venus and Mars orbits

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010eguga..12.3973o&link_type=abstract

EGU General Assembly 2010, held 2-7 May, 2010 in Vienna, Austria, p.3973

Computer Science

Scientific paper

The twin STEREO spacecraft separate in longitude by about 45 degrees per year providing a unique tool to study the temporal evolution of the solar wind. Now we are approaching the 180-degree spacecraft separation, which allows a complete time scan of the solar wind evolution in the ecliptic. We compare solar wind plasma measurements from the two spacecraft for timelags of 0.1 day up to several Carrington rotations. Using STEREO/IMPACT/SWEA electron and STEREO/PLASTIC, VEX/ASPERA-4/IMA and MEX/ASPERA-3/IMA ion observations we scan the whole heliosphere in the ecliptic between Venus and Mars orbits. We show how the different plasma parameters evolve on different time scales.

Affiliated with

Also associated with

No associations

Rating

Temporal evolution of the solar wind in the ecliptic between Venus and Mars orbits does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Temporal evolution of the solar wind in the ecliptic between Venus and Mars orbits, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Temporal evolution of the solar wind in the ecliptic between Venus and Mars orbits will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-917138