Hysteresis of a solar EUV flux and the relation of its characteristics to the solar cycle amplitude

Details Hysteresis of a solar EUV flux and the relation of its characteristics to the solar cycle amplitude Hysteresis of a solar EUV flux and the relation of its characteristics to the solar cycle amplitude

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996r%26qe...39..830n&link_type=abstract

Radiophysics and Quantum Electronics, Volume 39, Issue 10, pp.830-832

Physics

Scientific paper

The phenomenon of a difference between solar EVV fluxes I λ (λ<130 nm) measured for the same solar indices but in cycles of different amplitudes is studied. The difference can reach 15 20%. The phenomenon is explained in terms of a two-component model of solar EUV variations (from the active regions and the “undisturbed” solar surface). It follows from this model that in powerful cycles the fluxes I λ must be greater than in weak cycles for the same solar index F10.7. The results of the H I α line measurements from SME are presented as an example of the possibility of solar cycle amplitude prediction about two years before the solar maximum epoch.

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