Ground-based observations of solar intensity oscillations

Details Ground-based observations of solar intensity oscillations Ground-based observations of solar intensity oscillations

Publishing date

Jun 1984

URL

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mmsai..55..231s&link_type=abstract

Journals

(European Physical Society, Ministero della Pubblica Istruzione, and Universita di Catania, EPS Study Conference on Oscillations

Science

Astronomy and Astrophysics

Field

Astronomy

Additional info 2

1

Additional info 3

Astronomical Photometry, Solar Flux Density, Solar Oscillations, Atmospheric Attenuation, Atmospheric Pressure, Error Analysis, H Beta Line, Power Spectra, Solar Instruments, Solar Spectra

Type

Scientific paper

Abstract

Inexpensive, ground-based photometric measurements of full solar disk radiation are presently undertaken by means of the ESO La Silla diffraction telescope in the H-beta, V and B spectral domains. The random error of the photometric device employed has been reduced to 0.00008 for 1-min averages; systematic errors over 20-min periods were accordingly not detectable. The 1983 observations were accompanied by simultaneous air pressure monitoring by means of a microbarograph, in order to ascertain the influence of air mass variations on the measured solar intensities.

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