Prediction of geomagnetic disturbances by interplanetary scintillation

Details Prediction of geomagnetic disturbances by interplanetary scintillation Prediction of geomagnetic disturbances by interplanetary scintillation

Nov 1978

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

In AGARD Operational Modelling of the Aerospace Propagation Environ., Vol. 1 and 2 7 p (SEE N79-18094 09-31)

Astronomy and Astrophysics

Astronomy

Geomagnetism, Interplanetary Medium, Magnetic Disturbances, Radio Sources (Astronomy), Radio Waves, Scintillation, Solar Terrestrial Interactions, Electron Density (Concentration), Forecasting, Mathematical Models, Plasma Density, Solar Wind Velocity

Scientific paper

Daily observations of the scintillation of a number of radio sources lying at widely separated positions are used to predict geomagnetic activity associated with large scale features of the solar wind. By observing suitable sources lying to the east of the Sun it is possible to forecast, up to six days in advance, geomagnetic storms associated with corotating solar wind streams. Geomagnetic disturbances caused by interplanetary shock waves associated with solar flares may be predicted some 8 - 24 hours in advance, when using observations at UHF frequencies (300-400 Mhz).

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