Coronal holes as sources of solar wind

Details Coronal holes as sources of solar wind Coronal holes as sources of solar wind

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...46..303n&link_type=abstract

Solar Physics, vol. 46, Feb. 1976, p. 303-322.

Astronomy and Astrophysics

Astronomy

135

Skylab Program, Solar Corona, Solar Wind Velocity, Solar X-Rays, Data Correlation, Far Ultraviolet Radiation, Hole Distribution, Plasma Generators, Solar Radio Emission, Spaceborne Astronomy

Scientific paper

We investigate the association of high-speed solar wind with coronal holes during the Skylab mission by: (1) direct comparison of solar wind and coronal X-ray data; (2) comparison of near-equatorial coronal hole area with maximum solar wind velocity in the associated streams; and (3) examination of the correlation between solar and interplanetary magnetic polarities. We find that all large near-equatorial coronal holes seen during the Skylab period were associated with high-velocity solar wind streams observed at 1 AU.

Affiliated with

Also associated with

No associations

Rating

Coronal holes as sources of 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 Coronal holes as sources of solar wind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Coronal holes as sources of solar wind will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1299090