VARIATIONS OF SOLAR IRRADIANCE, 10.7 CM RADIO FLUX, HE-I 10830 ANGSTROM EQUIVALENT WIDTH, AND GLOBAL MAGNETIC-FIELD INTENSITY AND THEIR RELATION TO LARGE-SCALE SOLAR MAGNETIC-FIELD STRUCTURE

Variations of total solar irradiance, 10.7 cm radio emission, the He I 10830 Angstrom equivalent width and the solar magnetic field flux mea sured for the entire Sun are compared with variations of the energy in dex of the global solar magnetic field and the index of the effective solar multipole for years 1979-1992. It is shown that photospheric rad iation and that generated in the upper chromosphere and corona display different relationships with the global magnetic field of the Sun, an d that interaction between the magnetic field and the solar irradiance is much more complicated than the traditional blocking effect.