Latitudinal gradients of the solar wind parameters during 1976 and 1977: HELIOS 1, 2 and IMP in-situ observations

Details Latitudinal gradients of the solar wind parameters during 1976 and 1977: HELIOS 1, 2 and IMP in-situ observations Latitudinal gradients of the solar wind parameters during 1976 and 1977: HELIOS 1, 2 and IMP in-situ observations

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985stin...8628902b&link_type=abstract

Unknown

Other

Helios 1, Helios 2, Imp, Solar Wind, Wind Measurement, Current Sheets, Solar Corona, Solar Cycles, Solar Protons, Temperature Measurement

Scientific paper

Interplanetary observations from Helios 1, Helios 2 and IMP spacecraft during the early portion of solar cycle 21 were used to investigate the latitudinal gradients of solar wind parameters with respect to the angular displacement from the current sheet inferred from synoptic white-light maps of the solar corona at 1.75 solar radii. Large latitudinal gradients for solar wind flow speed, proton density, and temperature are found. All these gradients become smoother towards the solar cycle maximum. Neither latitudinal nor temporal variations for magnetic flow and thermal energy density are identified.

Affiliated with

Also associated with

No associations

Rating

Latitudinal gradients of the solar wind parameters during 1976 and 1977: HELIOS 1, 2 and IMP in-situ observations 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 Latitudinal gradients of the solar wind parameters during 1976 and 1977: HELIOS 1, 2 and IMP in-situ observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Latitudinal gradients of the solar wind parameters during 1976 and 1977: HELIOS 1, 2 and IMP in-situ observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1291157