Solar Wind Temporal and Latitudinal Variations from Soho-Swan

Details Solar Wind Temporal and Latitudinal Variations from Soho-Swan Solar Wind Temporal and Latitudinal Variations from Soho-Swan

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmsh21a0487l&link_type=abstract

American Geophysical Union, Fall Meeting 2002, abstract #SH21A-0487

Physics

2100 Interplanetary Physics, 2124 Heliopause And Solar Wind Termination, 2144 Interstellar Gas, 2152 Pickup Ions, 2154 Planetary Bow Shocks

Scientific paper

Full-sky maps of backscattered solar Ly-alpha radiation recorded routinely by SOHO-SWAN between 1996 and 2002 are compared with models allowing for any latitude dependence of the ionization of the interstellar hydrogen flow by the solar wind. Recent work on the calibration of the SWAN sensors for this period of time (Quémerais and Bertaux, 2002) as well as on the cleaning of the data and correction from stellar contamination allow to quantify the anisotropy degree of the solar wind mass flux, north-south asymetries and the temporal evolution of the fluxes.

Affiliated with

Also associated with

No associations

Rating

Solar Wind Temporal and Latitudinal Variations from Soho-Swan 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 Solar Wind Temporal and Latitudinal Variations from Soho-Swan, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar Wind Temporal and Latitudinal Variations from Soho-Swan will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1435678