Center-to-limb observations of the lambda 285.2 NM MgI UV resonance line

Details Center-to-limb observations of the lambda 285.2 NM MgI UV resonance line Center-to-limb observations of the lambda 285.2 NM MgI UV resonance line

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...282..621b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 282, no. 2, p. 621-633

Astronomy and Astrophysics

Astronomy

3

Line Spectra, Magnesium, Resonance Lines, Ultraviolet Astronomy, Ultraviolet Spectra, Absorption Spectra, Doppler Effect, Emission Spectra, Solar Limb, Spatial Resolution, Spectral Resolution

Scientific paper

We present here new results about the 285.212 nm Mg I resonance line. The spectra have been obtained from the RASOLBA balloon experiment of the LPSP launched in 1986 from France. The data have both high spectral (1.5 pm) and spatial (1 sec) resolution. Spectra of either the Sun center and the solar limb have been recorded in the 280 nm range. We paid a careful attention on the spatial evolution of the Mg I absorption line with the hope to find predicted but not confirmed emission feature in the central core. The very faint emission detected at Sun center becomes bright when observed off-limb. We give some measurements of the Mg I core Doppler shifts.

Affiliated with

Also associated with

No associations

Rating

Center-to-limb observations of the lambda 285.2 NM MgI UV resonance line 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 Center-to-limb observations of the lambda 285.2 NM MgI UV resonance line, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Center-to-limb observations of the lambda 285.2 NM MgI UV resonance line will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1013093