Possible Origin of the Secondary Stream of Neutral Fluxes at 1 AU

Details Possible Origin of the Secondary Stream of Neutral Fluxes at 1 AU Possible Origin of the Secondary Stream of Neutral Fluxes at 1 AU

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..719..195w&link_type=abstract

PHYSICS OF THE OUTER HELIOSPHERE. AIP Conference Proceedings, Volume 719, pp. 195-200 (2004).

Physics

6

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind, Planetary Bow Shocks, Interplanetary Shocks

Scientific paper

The existence of a secondary stream of neutral atoms inside the heliosphere arriving from about 285° ecliptic longitude, which is about 30° higher than the nominal upstream direction of the inflowing interstellar gas, has been proposed recently based on a wide variety of observations from many different missions. We will discuss the LENA/IMAGE measurements in detail and conclude that the secondary stream is composed mainly of hydrogen atoms at an energy of about 1 keV. We will discuss some possible explanations for the origin of the secondary stream, with the most likely source being the region upstream of the termination shock.

Affiliated with

Also associated with

No associations

Rating

Possible Origin of the Secondary Stream of Neutral Fluxes at 1 AU 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 Possible Origin of the Secondary Stream of Neutral Fluxes at 1 AU, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Possible Origin of the Secondary Stream of Neutral Fluxes at 1 AU will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1059959