Cyclic variation in the temperature minimum region of solar atmosphere.

Details Cyclic variation in the temperature minimum region of solar atmosphere. Cyclic variation in the temperature minimum region of solar atmosphere.

Feb 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000acasn..41...44z&link_type=abstract

Acta Astron. Sin., Vol. 41, No. 1, p. 44 - 50

Other

Solar Atmosphere: Temperatures, Solar Spectrum: Calcium Lines, Solar Spectrum: Line Profiles, Solar Spectrum: Variability

Scientific paper

Calcium K line as well as some other solar spectral lines have been measured regularly nearly every month since 1974 at Kitt Peak. It is now widely accepted that K1 is formed in the temperature minimum region (TMR) and that the distance of the component K1 from the line center and the intensity of K1 is well related to the position and temperature of TMR, respectively. The authors' study on the data of K line profiles and on the sunspot numbers over decades shows: in full disc integrated spectra the distance of K1 from the line center fluctuates in the same way as the sunspot number does, indicating a solar cyclic variation.

Affiliated with

Also associated with

No associations

Rating

Cyclic variation in the temperature minimum region of solar atmosphere. 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 Cyclic variation in the temperature minimum region of solar atmosphere., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cyclic variation in the temperature minimum region of solar atmosphere. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1491917