Large-scale propagation properties of interplanetary disturbances revealed from IPS and spacecraft observations

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Extraterrestrial Radio Waves, Interplanetary Space, Shock Wave Propagation, Solar Wind, Electron Density Profiles, Satellite Observation, Solar Prominences, Velocity Distribution

Scientific paper

Interplanetary scintillation (IPS) observations may be used to study large-scale propagation properties of transient interplanetary disturbances in a three-dimensional manner, although current IPS observations have several limitations, e.g., poor time resolution and line-of-sight integration. Comparative studies with spacecraft solar wind and white-light coronal mass ejection observations are quite helpful in interpretation of IPS observations. An interplanetary disturbance apparently in association with a disappearing solar filament, which took place near the central meridian of the sun on late April 22, 1979, is discussed to examine previous deductions from IPS observations. Three-station IPS observations of the flow speed and spacecraft observations suggest that a quasi-spherical interplanetary disturbance was formed around the sun-earth line, whereas the center of the disturbance derived from the distribution of enhanced IPS across the sky (g-maps) is located to the east of the sun-earth line.

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