Chromospheric fine structures in the solar corona

Details Chromospheric fine structures in the solar corona Chromospheric fine structures in the solar corona

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977jrasc..71..373r&link_type=abstract

Journal of the Royal Astronomical Society of Canada, vol. 71, Oct. 1977, p. 373-376. In French.

Astronomy and Astrophysics

Astronomy

1

Astronomical Photography, Chromosphere, H Alpha Line, Solar Corona, Solar Prominences, Stellar Structure, Coronagraphs, Fine Structure, Magnetohydrodynamic Flow, Plasma Temperature

Scientific paper

Leroy (1972) predicted the existence of possible fine prominence
features to explain the presence of faint luminous chromospheric
emission in the corona. This paper draws attention to the existence of
very fine structures of the order of 200 km in width seen at H-alpha and
extending from the center of a sunspot into the corona.

Affiliated with

Also associated with

No associations

Rating

Chromospheric fine structures in the solar corona 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 Chromospheric fine structures in the solar corona, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chromospheric fine structures in the solar corona will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-746771