Multispacecraft Observations of Solar Wind Gradients Near L1: VHO Case Studies

Details Multispacecraft Observations of Solar Wind Gradients Near L1: VHO Case Studies Multispacecraft Observations of Solar Wind Gradients Near L1: VHO Case Studies

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsh51b1271s&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #SH51B-1271

Physics

[1916] Informatics / Data And Information Discovery, [2134] Interplanetary Physics / Interplanetary Magnetic Fields, [2164] Interplanetary Physics / Solar Wind Plasma

Scientific paper

The Virtual Heliospheric Observatory (VHO) will be demonstrated as a powerful scientific tool to identify interesting spacecraft configurations of the near-Earth L1 fleet. In particular, solar wind plasma and interplanetary magnetic field gradient investigations will be used to demonstrate the utility of the VHO data query capability. VHO is particularly useful to identify time periods of extreme solar wind conditions of either very low or high solar wind densities or velocities. It will be demonstrated that identified periods of steady solar wind conditions are very useful for in-flight calibration of the various in-situ instruments.

Affiliated with

Also associated with

No associations

Rating

Multispacecraft Observations of Solar Wind Gradients Near L1: VHO Case Studies 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 Multispacecraft Observations of Solar Wind Gradients Near L1: VHO Case Studies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multispacecraft Observations of Solar Wind Gradients Near L1: VHO Case Studies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1877205