Radiation damping in acoustically heated atmospheres of late-type stars

Details Radiation damping in acoustically heated atmospheres of late-type stars Radiation damping in acoustically heated atmospheres of late-type stars

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...197..223u&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 197, no. 1-2, May 1988, p. 223, 224.

Astronomy and Astrophysics

Astrophysics

16

Acoustic Attenuation, Atmospheric Heating, Chromosphere, Elastic Damping, Late Stars, Giant Stars, Line Spectra, Photosphere, Stellar Rotation, Supergiant Stars

Scientific paper

It is shown that radiation damping of acoustic waves propagating through
a stellar photosphere is much larger in giant stars than in dwarfs. This
could remove a major argument against acoustic waves as possible heating
mechanism for the chromospheres of slowly rotating stars.

Affiliated with

Also associated with

No associations

Rating

Radiation damping in acoustically heated atmospheres of late-type stars 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 damping in acoustically heated atmospheres of late-type stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiation damping in acoustically heated atmospheres of late-type stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-853632