Concentration of interstellar pickup H(+) and He(+) in the solar wind

Details Concentration of interstellar pickup H(+) and He(+) in the solar wind Concentration of interstellar pickup H(+) and He(+) in the solar wind

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994georl..21.1565g&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 21, no. 14, p. 1565-1568

Astronomy and Astrophysics

Astronomy

20

Astronomical Models, Concentration (Composition), Correlation, Flux (Rate), Helium Ions, Interstellar Matter, Protons, Solar Wind, Astronomical Spectroscopy, Mathematical Models, Ulysses Mission

Scientific paper

We present observations of interstellar pickup hydrogen and helium in the solar wind which show large, highly-correlated fluctuations in flux which are not correlated significantly with the solar-wind hydrogen flux. The correlation of the fluctuations in the two species implies that the fluctuations are caused by transport after ionization. The lack of correlation with the thermal flux means they are not caused by compressions of the wind. We present a new model which can naturally produce the observed fluctuations in the pickup ions.

Affiliated with

Also associated with

No associations

Rating

Concentration of interstellar pickup H(+) and He(+) in the solar wind 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 Concentration of interstellar pickup H(+) and He(+) in the solar wind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Concentration of interstellar pickup H(+) and He(+) in the solar wind will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1255008