Solar analysis of solar-constant monitoring package (SMM)

Details Solar analysis of solar-constant monitoring package (SMM) Solar analysis of solar-constant monitoring package (SMM)

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ucsd.rept.....h&link_type=abstract

Final Report California Univ., San Diego, La Jolla. Center for Astrophysics and Space Sciences.

Astronomy and Astrophysics

Astrophysics

Radiation Measurement, Solar Constant, Solar Maximum Mission, Variations, Darkness, Data Reduction, Faculae, Luminance, Nyquist Frequencies, Solar Interior, Sunspots

Scientific paper

The activity cavity radiometer irradiance monitor is supplying the first high precision data on solar total irradiance at the Earth. Thee classes of variability were discovered: large variations of amplitudes up to 0.2%; small high frequency variations in the form of a continuum in the periodogram, extending up to the Nyquist frequency; and sharp spikes at frequencies corresponding to the individual p modes already known from radial velocity measurements. The observed variations (up to 0.3%, on time scales of several days) were identified with sunspot darkness. The data analysis is expected to give information about the solar interior, as well as about the solar input to the terrestrial climate.

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