The ACRIM data in the context of stellar variability

Details The ACRIM data in the context of stellar variability The ACRIM data in the context of stellar variability

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nascp3086..280h&link_type=abstract

In NASA, Goddard Space Flight Center, Climate Impact of Solar Variability p 280-286 (SEE N91-12456 03-92)

Other

Irradiance, Luminosity, Radiometers, Solar Activity, Solar Cycles, Solar Magnetic Field, Stellar Spectrophotometry, Sun, Variability, Monitors, Solar Maximum Mission

Scientific paper

The Active Cavity Radiometer Irradiance Monitor (ACRIM) total-irradiance data from the Solar Maximum Mission have given a first comprehensive view of solar variability in the stellar sense. Five types of solar variability have been identified thus far. These have small amplitudes, less than a few tenths of one percent, and are at levels generally not yet detectable on other stars. The possible stellar analogs are interesting physically, and in particular may help us to understand solar behavior on longer time scales. The ACRIM data is described from the stellar point of view. The present state of stellar time-series photometry is discussed.

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