Structure and physics of solar faculae. IV - Chromospheric granular structure

Details Structure and physics of solar faculae. IV - Chromospheric granular structure Structure and physics of solar faculae. IV - Chromospheric granular structure

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...91...61f&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 91, March 1984, p. 61-70.

Physics

5

Chromosphere, Faculae, Solar Corona, Solar Magnetic Field, Fine Structure, Solar Granulation, Spectroheliographs

Scientific paper

The methods used and the results obtained in the measurement of the distances between the centers of chromospheric granules are described. A coincidence of these structures at two different altitudes was observed. Observations made in the K2v, or in the K3 and CN lines permit the comparison of two different altitudes: the upper and the lower chromosphere. These results include flocculi on the edge of the supergranules as well as plages. Two main results are obtained: (1) the most likely distance between two neighboring granules is, at the minimum of the solar cycle, of about 2.60 arc sec for K3 and 2,45 arc sec for CN, and (2) this distance is decreasing with growing solar activity.

Affiliated with

Also associated with

No associations

Rating

Structure and physics of solar faculae. IV - Chromospheric granular structure 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 Structure and physics of solar faculae. IV - Chromospheric granular structure, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure and physics of solar faculae. IV - Chromospheric granular structure will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-906033