Coordinated optical and radio studies of ionospheric disturbances - Initial results from Millstone Hill

Details Coordinated optical and radio studies of ionospheric disturbances - Initial results from Millstone Hill Coordinated optical and radio studies of ionospheric disturbances - Initial results from Millstone Hill

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987angeo...5..543m&link_type=abstract

(URSI and High Altitude Observatory, International Symposium on Large-Scale Processes in the Ionospheric-Thermospheric System, B

Physics

5

F Region, Incoherent Scatter Radar, Ionospheric Disturbances, Magnetic Storms, Satellite Imagery, Solar Terrestrial Interactions, Field Of View, Radio Observation, Red Arcs

Scientific paper

Boston University's Mobile Ionospheric Observatory (MIO) was located at the Millstone Hill site during several active experiments conducted during 1983-1985. On nights when background data were taken, or when active experiments were postponed, the all-sky imaging system in the MIO recorded a broad variety of natural geophysical disturbances: several cases of stable auroral red (SAR) arcs, variations in the location of the diffuse aurora, ripples in the diffuse aurora, detached arcs and patches of 6300 A emission. Simultaneous incoherent scatter observations were taken. Satellite radio beacon signals recorded by AFGL provided simultaneous total electron content and scintillation observations within the optical field of view. The single radio-ray-path plasma observations and the all-sky images of large-scale energy input offer a unified approach to understanding solar-terrestrial disturbance patterns at mid-latitudes.

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