Computer Science
Scientific paper
May 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989em%26p...45..161d&link_type=abstract
Earth, Moon, and Planets (ISSN 0167-9295), vol. 45, May 1989, p. 161-173.
Computer Science
5
Geomagnetism, Interplanetary Medium, Magnetic Storms, Satellite Observation, Space Plasmas, Interplanetary Magnetic Fields, Prediction Analysis Techniques, Solar Wind, Time Dependence
Scientific paper
An MHD 2-1/2D, time-dependent model is used, together with observations of six solar flares during February 3-7, 1986, to demonstrate global, large-scale, compound disturbances in the solar wind over a wide range of heliolongitudes. This scenario is one that is likely to occur many times during the cruise, possibly even encounter, phases of the Multi-Comet Mission. It is suggested that a model such as this one should be tested with multi-spacecraft data (such as the MCM and earth-based probes) with several goals in view: (1) utility of the model for operational real-time forecasting of geomagnetic storms, and (2) scientific interpretation of certain forms of cometary activities and their possible association with solar-generated activity.
Dryer Murray
Smith Zdenka Kopal
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