Computer Science
Scientific paper
Sep 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978clus.nasa..159b&link_type=abstract
In JPL A Close-up of the Sun p 159-169 (SEE N78-32964 23-92)
Computer Science
High Resolution, Magnetic Flux, Magnetic Signatures, Solar Activity, Solar Magnetic Field, Solar Probes, Magnetic Disturbances, Photosphere, Solar Atmosphere, Sun
Scientific paper
Ground-based solar magnetograms are frequently in error by as much as twenty percent and contribute to the poor correlation between magnetic changes and solar flares. High resolution measurement of the magnetic field component, which is normal to the photosphere and measured at photospheric height, can be used to construct a magnetic flux partition function F. Therefore, dF/dt is an EMF which drives atmospheric currents in reconnecting solar active regions. With a high quality magnetograph, the solar probe can be used to obtain good estimates of F and dF/dt and thereby the energy stored as induced solar atmospheric currents during quiescent interflare periods. Should a flare occur during a favorable observing period, the present method of analysis should show characteristic signatures in F, DF/dt, and especially, in the stored flux computed from dF/dt.
Baum P. J.
Bratenahl A.
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