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U.S. Department of Energy
Office of Scientific and Technical Information

Investigation of methods for updating ionospheric scintillation models using topside in-situ plasma-density measurements. Rept. for 1 May 90-30 Apr 91

Technical Report ·
OSTI ID:5862213
Modern military communication, navigation, and surveillance systems depend on reliable, noise-free transionospheric radio-frequency channels. They can be severely impacted by small-scale electron-density irregularities in the ionosphere, which cause both phase and amplitude scintillation. Basic tools used in planning and mitigation schemes are climatological in nature and thus may greatly over- and under-estimate the effects of scintillation in a given scenario. This report summarizes the results of the first year of a three-year investigation into the methods for updating ionospheric scintillation models using observations of ionospheric plasma-density irregularities measured by 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 UHF radio link in the early-evening auroral zone were calculated from DMSP SM data and compared to the levels actually observed.
Research Organization:
Northwest Research Associates, Inc., Bellevue, WA (United States)
OSTI ID:
5862213
Report Number(s):
AD-A-243378/7/XAB; NWRA-CR--91-R072; CNN: F19628-90-C-0072
Country of Publication:
United States
Language:
English