Radiation loss and mechanical heating in the solar chromosphere

Details Radiation loss and mechanical heating in the solar chromosphere Radiation loss and mechanical heating in the solar chromosphere

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...39..327u&link_type=abstract

Solar Physics, vol. 39, Dec. 1974, p. 327-336.

Computer Science

Sound

38

Atmospheric Heating, Chromosphere, Radiative Heat Transfer, Solar Atmosphere, Sound Waves, Atmospheric Heat Budget, Energy Dissipation, Reference Atmospheres, Solar Temperature

Scientific paper

The radiation loss of the solar chromosphere is evaluated on the basis of the Harvard Smithsonian Reference Atmosphere. The total radiative flux is found to be between 2.5 and 3.3. E6 erg/sq cm/sec. A discussion of possible heating mechanisms shows that the short-period acoustic wave theory is the only one able to balance the chromospheric radiation loss and is consistent with observation.

Affiliated with

Also associated with

No associations

Rating

Radiation loss and mechanical heating in the solar chromosphere 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 Radiation loss and mechanical heating in the solar chromosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiation loss and mechanical heating in the solar chromosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1339512