Modeling the meridional solar wind flow in the midcorona

Details Modeling the meridional solar wind flow in the midcorona Modeling the meridional solar wind flow in the midcorona

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977jgr....82..593r&link_type=abstract

Journal of Geophysical Research, vol. 82, Feb. 1, 1977, p. 593-602.

Physics

3

Atmospheric Models, Meridional Flow, Solar Atmosphere, Solar Corona, Solar Wind Velocity, Electron Density Profiles, Far Ultraviolet Radiation, H Alpha Line, Photosphere, Solar Magnetic Field, Solar Temperature, Velocity Distribution

Scientific paper

For a selected region of the sun during Carrington rotation 1527 (November 1967) synoptic photospheric magnetic field, H alpha, and coronal EUV observations and associated calculations are combined together with solar wind and interplanetary magnetic field observations of three different space probes with a maximum latitudinal separation of about 13 degrees. From this a simplified but refined meridional coronal-hole-type field geometry for the lower solar atmosphere is constructed and the magnetic field and the temperature-density dependence at coronal heights above the transition layer are calculated. Questions about coronal heating and the validity of the equations of motion in the lower solar corona are discussed.

Affiliated with

Also associated with

No associations

Rating

Modeling the meridional solar wind flow in the midcorona 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 Modeling the meridional solar wind flow in the midcorona, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeling the meridional solar wind flow in the midcorona will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-800197