Radial dependence of solar wind parameters in the ecliptic (1.1 R &sun;-61 AU)

Details Radial dependence of solar wind parameters in the ecliptic (1.1 R &sun;-61 AU) Radial dependence of solar wind parameters in the ecliptic (1.1 R &sun;-61 AU)

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996soph..169..209k&link_type=abstract

Solar Physics, Volume 169, Issue 1, pp.209-213

Physics

11

Scientific paper

The radial dependencies of four solar wind parameters (plasma density N, velocity V, temperature T, and magnitude of the interplanetary magnetic field B) are derived from remote sensing data of the solar corona and from in situ measurements in the heliosphere (Helios-1, 2, Pioneer-10, 11, and Voyager-1, 2). Using doubly logarithmic scaling (‘solar wind parameter vs radial distance from the Sun’) one finds two distinct intervals in the ecliptic, i.e., an exponential section within, approximately, the inner heliosphere and a linear section - up to at least 61 AU - in the outer heliosphere.

Affiliated with

Also associated with

No associations

Rating

Radial dependence of solar wind parameters in the ecliptic (1.1 R &sun;-61 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 Radial dependence of solar wind parameters in the ecliptic (1.1 R &sun;-61 AU), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radial dependence of solar wind parameters in the ecliptic (1.1 R &sun;-61 AU) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1752766