Horizontal motion of the solar granulation - Mesogranulation and eddy structure

Details Horizontal motion of the solar granulation - Mesogranulation and eddy structure Horizontal motion of the solar granulation - Mesogranulation and eddy structure

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990s%26w....29..164b&link_type=abstract

Sterne und Weltraum (ISSN 0039-1263), vol. 29, March 1990, p. 164-168. In German. Research supported by DFG.

Computer Science

Computerized Simulation, Solar Granulation, Solar Observatories, Stellar Oscillations, Charge Coupled Devices, Spacelab, Stellar Motions

Scientific paper

The main problems related to solar observations are reviewed, and recent advances in the technology of observation and analysis are reviewed. Recent findings on the convection dependency of the motion of solar granules are discussed. These convective cells are 5000-6000 km in breadth and are called mesogranulation. They are intermediate in size between those resulting from granulation and from supergranulation. The observation of an eddy in the mesogranulation is reported.

Affiliated with

Also associated with

No associations

Rating

Horizontal motion of the solar granulation - Mesogranulation and eddy 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 Horizontal motion of the solar granulation - Mesogranulation and eddy structure, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Horizontal motion of the solar granulation - Mesogranulation and eddy structure will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1250743