Award Number: N0001408AF00002 http://www.nrl.navy.mil
LONG-TERM GOALSThe ultimate goal of this research is the development of an operational algorithm for retrieving daytime ionospheric hmF2 from the measurement of the O II 83.4 nm emission feature. This algorithm will provide data for ingestion into ionospheric models. The reward of a successful algorithm is very high, as no capability presently exists to measure the global variation of hmF2 within the F-region of the ionosphere during the day. Further, this work will provide a new assessment of the state of the ionosphere during significant space weather events, which is critical to the use of GPS and other operational systems that rely on the propagation of radio waves within the near-Earth space environment. In addition, this research could lead to a method for global monitoring of the ionosphere and its response to solar, geomagnetic and lower atmospheric waves and tides.
OBJECTIVESThe technological objective of this research is to develop a new algorithm that can be used to obtain routine, global ionospheric measurements for incorporation into operational codes and assimilative ionospheric models, including the Global Assimilation of Ionospheric Measurements (GAIM) model. GAIM, used at AFWA as the state-of-the-art ionospheric predictive model for Navy and DoD needs, currently is limited by the absence of data that can be ingested to constrain the daytime hmF2 parameter. The hmF2 specifies the height of the peak of the ionosphere and is used as both a metric for the ionosphere and a parameter to specify the ionospheric density profile. The software to be developed will be directly applicable to dayside data from the Special Sensor Ultraviolet Limb Imager (SSULI) sensors on the DMSP F18-20 satellites. The proposed additional capability of the SSULI Ground Data Analysis Software (GDAS) to generate operational hmF2 values from 83.4 nm measurements would provide data that could be used as hmF2 parameter constraints with GAIM at AFWA. The scientific objective of this effort is to develop an understanding of the ionospheric response to variability in solar and geomagnetic forcing. In addition, this effort will lead to pioneering research in the fundamental physics behind the dayside 83.4 nm emission and the conditions under which it presents a viable measure of this ionospheric variability.