The morphology of solar granulations and dark networks

Details The morphology of solar granulations and dark networks The morphology of solar granulations and dark networks

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..106..249g&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 106, Aug. 1986, p. 249, 250.

Physics

1

Solar Granulation, Stellar Spectrophotometry, Dark Matter, Morphology

Scientific paper

Solar granules are classified into four groups based on shape and splitting by sharp rifts crossing them. Grains are classified as: single granules varying in size from 1/8 to 3 in., single granules embayed by a broad dark area or possessing a central darkening, single granules split by very narrow rifts which are significantly narrower than the intergranular lanes, and complexes of granules displaying a daisy pattern. The formation and growth of 'white-light dark networks' are also discussed

Affiliated with

Also associated with

No associations

Rating

The morphology of solar granulations and dark networks 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 The morphology of solar granulations and dark networks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The morphology of solar granulations and dark networks will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-895538