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U.S. Department of Energy
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Investigation of methods for updating ionospheric scintillation models using topside in situ plasma density measurements. Final report, 1 May 1990-30 April 1993

Technical Report ·
OSTI ID:5633582
Modern military communication, navigation, and surveillance systems depend on reliable, noise free transionospheric radio-frequency channels and can be severely impacted by small-scale electron-density irregularities in the ionosphere. This report summarizes the results of a three year investigation into the methods for updating ionospheric scintillation models using observations of ionospheric plasma-density irregularities measured by the DMSP Scintillation Meter (SM) sensor. Results are reported from the analysis of data from a campaign conducted in January 1990 near Tromso, Norway, in which near coincident in-situ plasma-density and transionospheric scintillation measurements were made. Estimates for the level of intensity and phase scintillation on a transionospheric UBF radio link in the early-evening auroral zone were calculated from DMSP SM data and compared to the levels actually observed. Results are also presented from a comparison with scintillation observations made with a coincident DNA Polar BEAR satellite pass. Ionosphere, Ionospheric Scintillation, Radiowave Scintillation, Defense Meteorology Satellite Program (DMSP).
Research Organization:
Northwest Research Associates, Inc., Bellevue, WA (United States)
OSTI ID:
5633582
Report Number(s):
AD-A-269872/8/XAB; NWRA-CR--93-R096; CNN: F19628-90-C-0072
Country of Publication:
United States
Language:
English