Observations of large fluxes of He/+/ in the solar wind following an interplanetary shock

Details Observations of large fluxes of He/+/ in the solar wind following an interplanetary shock Observations of large fluxes of He/+/ in the solar wind following an interplanetary shock

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jgr....85.3431g&link_type=abstract

Journal of Geophysical Research, vol. 85, July 1, 1980, p. 3431-3434. Research sponsored by the U.S. Department of Energy and N

Physics

21

Helium Ions, Interplanetary Medium, Shock Waves, Solar Flux, Solar Wind, Proton Density (Concentration), Solar Corona, Solar Prominences

Scientific paper

Los Alamos Scientific Laboratory instrumentation on Imp 7 has detected large fluxes of He(+) within that volume of solar wind plasma believed to be the solar ejecta driving the interplanetary shock wave disturbance of July 29, 1977. The very high He(+)/He(++) abundance ratio of 0.3 measured during this event suggests that this was solar prominence material only partially ionized by its passage through the corona.

Affiliated with

Also associated with

No associations

Rating

Observations of large fluxes of He/+/ in the solar wind following an interplanetary shock 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 Observations of large fluxes of He/+/ in the solar wind following an interplanetary shock, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of large fluxes of He/+/ in the solar wind following an interplanetary shock will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-804301