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

Remote sensing of ionosphere by using ultraviolet and visible emissions

Technical Report ·
OSTI ID:6267801
The ability to remotely sense ionospheric conditions for improved operation of communications and radar systems has been a long term goal of some DOD programs. This capability now appears to be possible through improvements in computer models of the ionosphere and in UV remote-sensing methods. The approach is to use passive ultraviolet optical measurements and in-situ ion-density measurements as inputs to a comprehensive ionospheric model, which will calculate the electron-density measurements as inputs to a comprehensive ionospheric model which will calculate the electron-density profile. A novel feature of this approach is the use of naturally occurring airglow and auroral ultraviolet radiation. This method can be used for the mid-latitude day ionosphere (90 to 800 km) and the night auroral E layer. Eventually, extensions of the technique will cover the night mid-latitude as well. The remote-sensing measurement can also be used to locate regions of ionospheric irregularity, and hence probable phase scintillation, in both equatorial and polar-cap regions and to locate the real-time position of the auroral-oval particle precipitation.
Research Organization:
Air Force Geophysics Lab., Hanscom AFB, MA (USA)
OSTI ID:
6267801
Report Number(s):
AD-A-181730/3/XAB; AFGL-TR-87-0166
Country of Publication:
United States
Language:
English