Solar spectrum from 170 to 3200 nanometers

Astronomy and Astrophysics – Astronomy

Scientific paper

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Radiant Flux Density, Solar Constant, Solar Cycles, Solar Radio Emission, Solar Spectra, Spectral Emission, Astronomical Spectroscopy, Radiation Measurement, Radiation Spectra, Solar Flux Density, Spacelab Payloads, Sunspots, Wavelengths

Scientific paper

The spectral irradiance of the Sun between 170 and 3200 nanometers was measured to determine accurately the solar constant, its possible variation with the solar cycle, and the wavelength range responsible for the observed variations. It is pointed out that measurements over very long time periods (10 years) involving flights of the same instrument on future Spacelab missions will be required. Few spectral solar irradiation measurements ranging from the near ultraviolet to the near infrared have been performed yet. The most extensive solar irradiation measurements were obtained by a spectrometer onboard an aircraft or from high altitude observatories. The full disk irradiation flux was measured, corrections for atmospheric absorption are applied in all of the measurements.

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