Solar Flares and the Zeeman Effect

Details Solar Flares and the Zeeman Effect Solar Flares and the Zeeman Effect

Aug 1949

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1949natur.164..280e&link_type=abstract

Nature, Volume 164, Issue 4163, pp. 280-281 (1949).

Computer Science

Scientific paper

MR. BRUCE believes that the short-lived broadening which we observe in the Balmer emission lines during the ``flash'' phase of an intense flare arises from a temporary magnetic field of the order of 105 gauss. If this is so, some explanation is needed of the fact that no comparable Zeeman broadening has been recorded in the emission lines of iron, calcium and silicon as photographed by C. W. Allen1 and myself2. Most of these lines show (in absorption) the normal Zeeman effect in sunspot spectra, where the fields are of the order of only 103 gauss.

Affiliated with

Also associated with

No associations

Rating

Solar Flares and the Zeeman Effect 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 Solar Flares and the Zeeman Effect, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar Flares and the Zeeman Effect will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1892826