Observations of low-degree solar oscillations with few detector elements

Details Observations of low-degree solar oscillations with few detector elements Observations of low-degree solar oscillations with few detector elements

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..128...91a&link_type=abstract

(IAU, The Inside the Sun Colloquium, 121st, Versailles, France, May 22-26, 1989) Solar Physics (ISSN 0038-0938), vol. 128, July

Physics

18

Irradiance, Solar Gravitation, Solar Oscillations, Stellar Luminosity, Gravity Waves, P Waves, Soho Mission, Spacecraft Instruments

Scientific paper

The detection of low-degree solar oscillation modes with a specific low-resolution detector configuration is investigated. The detector is part of an instrument (the Luminosity Oscillations Imager) in the VIRGO package, to be flown on SOHO. Various problems such as p- and g-mode sensitivity, B and roll angle effects, modes isolation, cross-talk and guiding effects are treated for a given detector configuration. The computed sensitivity will enable the instrument to detect any type of modes for l less than 6.B and roll angle effects can be compensated by using adequate filters for mode isolation. Guiding effects are small for p-modes. Also some other complex high-degree mode effects are treated.

Affiliated with

Also associated with

No associations

Rating

Observations of low-degree solar oscillations with few detector elements 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 Observations of low-degree solar oscillations with few detector elements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of low-degree solar oscillations with few detector elements will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1096799