The prediction of fast stream front arrivals at the earth on the basis of solar wind measurements at smaller solar distances

Details The prediction of fast stream front arrivals at the earth on the basis of solar wind measurements at smaller solar distances The prediction of fast stream front arrivals at the earth on the basis of solar wind measurements at smaller solar distances

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978omap....1r....r&link_type=abstract

In AGARD Operational Modelling of the Aerospace Propagation Environ., Vol. 1 and 2 5 p (SEE N79-18094 09-31)

Mathematics

Geomagnetism, Magnetic Disturbances, Prediction Analysis Techniques, Solar Wind Velocity, Auroral Zones, Ionospheric Disturbances, Mathematical Models, Radio Communication, Solar Corona

Scientific paper

The problems involved in the prediction of the arrival of fast solar wind streams at the earth on the basis of measurements made by space probes in the region between 0.3 and 1 AU are discussed. It is shown that arrival time predictions accurate to within a few hours that can be made at least as long as the large scale conditions on the Sun are relatively stationary as observed near the time of solar minimum. However, the latitudinal extent of the respective high speed streams is found to be important for making quantitative predictions. Coronal data sufficient for locating the sources of high speed streams can improve the precision of these predictions.

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