Properties of the white-light corona polarization during maximum of the solar cycle.

Details Properties of the white-light corona polarization during maximum of the solar cycle. Properties of the white-light corona polarization during maximum of the solar cycle.

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991sopo.work..318s&link_type=abstract

Solar Polarimetry, Proceedings of the 11th Sacramento Peak Summper Workshop. Edited by L.J. November. Sunspot, NM: National Sola

Physics

Scientific paper

The results of measuring the polarization of the white-light corona, carried out during the February 16, 1980 solar eclipse, are presented. The degree of polarization was observed to be relatively high all round the sun, with the exception of a coronal hole near the south pole. Together with the well-expressed streamers, the high degrees of polarization were observed in the narrow ray at P = 210° and also in the broad region P = 310° - 350°. The general increase of coronal density characteristic for solar cycle maximum and accidental concentration of the coronal structures to the plane of sky could be responsible for such peculiarities.

Affiliated with

Also associated with

No associations

Rating

Properties of the white-light corona polarization during maximum of the solar cycle. 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 Properties of the white-light corona polarization during maximum of the solar cycle., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Properties of the white-light corona polarization during maximum of the solar cycle. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1896087