NIMBUS-7 SBUV (Solar Backscatter Ultraviolet) Observations of Solar UV Spectral Irradiance Variations Caused by Solar Rotation and Active-Region Evolution for the Period November 7, 1978-November 1, 1980

摘要

NIMBUS-7 SBUV observations of temporal variations of the solar UV spectral irradiance over several days to a few weeks in the 160-400 nm wavelength range are presented in detail for the period Nov. 7, 1978 to Nov. 1, 1980. Larger 28-day variations and a second episode of 13-day variations occurred during the second year of measurements. The thirteen day periodicity is not a harmonic of the 28-day periodicity. The 13-day periodicity dominates certain episodes of solar activity while others are dominated by 28-day periods accompanied by a weak 14-day harmonic. Techniques for removing noise and long-term trends are described. Time series analysis results are presented for the Si II lines near 182 nm, the Al I continuum in the 190 -205 nm range, the Mg I continuum in the 210 -250 nm range, the Mg II H & K lines at 280 nm, the Mg I line at 285 nm, and the Ca II K & H lines at 393 and 397 nm.