Toward Zeeman Magnetometry in the Corona: Line-of-Sight Effects

Details Toward Zeeman Magnetometry in the Corona: Line-of-Sight Effects Toward Zeeman Magnetometry in the Corona: Line-of-Sight Effects

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997spd....28.0144r&link_type=abstract

American Astronomical Society, SPD meeting #28, #01.44; Bulletin of the American Astronomical Society, Vol. 29, p.887

Astronomy and Astrophysics

Astronomy

Scientific paper

One of the motivations for a large-aperture ground-based coronagraph is the possibility of measuring magnetic flux in the solar corona using the Zeeman sensitivity (Lande g = 1.5) of emission lines such as Fe XIV 530.3 nm, Fe X 637.4 nm, and Fe XIII 1074.7 nm. However, because the corona is optically thin, it is necessary to consider the effects of superposition along the line-of-sight on the interpretation of a detected Zeeman signal. Simple models are used to explore and illustrate the likely importance of line-of-sight confusion.

Affiliated with

Also associated with

No associations

Rating

Toward Zeeman Magnetometry in the Corona: Line-of-Sight Effects 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 Toward Zeeman Magnetometry in the Corona: Line-of-Sight Effects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Toward Zeeman Magnetometry in the Corona: Line-of-Sight Effects will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1146539