Detector configurations for observations of gravity modes in solar radiance

Details Detector configurations for observations of gravity modes in solar radiance Detector configurations for observations of gravity modes in solar radiance

Publishing date

Dec 1988

URL

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..381a&link_type=abstract

Journals

In ESA, Seismology of the Sun and Sun-Like Stars p 381-383 (SEE N89-25819 19-92)

Science

Physics

Field

Optics

Additional info 3

Satellite-Borne Instruments, Solar Constant, Solar Gravitation, Solar Instruments, Solar Radiation, Geometrical Optics, Soho Mission, Solar Physics, Stellar Luminosity, Systems Engineering

Type

Scientific paper

Abstract

The VIRGO (Variability in IRradiance and Gravity Oscillations) investigation was selected to fly on the SOHO mission. One of the components of VIRGO is a small imaging instrument with limited spatial resolution. Calculations were carried out in an attempt to find an optimal geometrical detector configuration for the observation of low degree g-modes in the solar luminosity. The constraints are given as a wish of having the largest possible sensitivity and redundancy with the smallest number of detectors. In addition the crosstalk for different modes at same frequency should be minimized.

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