Cross-correlation of solar wind parameters with sunspots (`Long-term variations') at 1 AU during cycles 21 and 22

Details Cross-correlation of solar wind parameters with sunspots (`Long-term variations') at 1 AU during cycles 21 and 22 Cross-correlation of solar wind parameters with sunspots (`Long-term variations') at 1 AU during cycles 21 and 22

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.245...81k&link_type=abstract

Astrophysics and Space Science, Volume 245, Issue 1, pp.81-88

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Long-term variations of solar wind parameters at 1 AU are correlated with sunspots for the time interval 1973 to 1993 (solar cycles 21, 22). Using theNear-Earth Heliosphere Data ‘OMNI’ the plasma density, the magnitude of the interplanetary magnetic field, the solar wind velocity and the solar wind temperature show consistent long-term variations in each cycle (21 and 22) — pointing to specifictime-lags in the coupling between sunspots (and the underlying convection zone), the solar corona and the solar wind parameters at 1 AU (ecliptic).

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