HR: 11:50h
AN: SM42A-07 [Abstracts]
TI: Further Advances in Formula Representation of High-Latitude O+ Ionospheric Outflows Based on DyFK Simulations
AU: * Horwitz, J L
EM: horwitz@uta.edu
AF: Department of Physics, The University of Texas at Arlington, Arlington, TX 76019, United
States
AU: Zeng, W
EM: zengw@uta.edu
AF: Department of Physics, The University of Texas at Arlington, Arlington, TX 76019, United
States
AB:
Considerable interest exists in the magnetospheric community in obtaining compact representations of the
ionospheric outflow fluxes and their relationships to putative drivers. Recent satellite data analyses by
Strangeway et al.[2005] and Zheng et al.[2005] have obtained formula fits for the measurement-based
relationships of the outflows levels to parameterizations for electron precipitation and Poynting fluxes, which are
expected to be among the principal drivers, or closely related to them, for the ionospheric outflows. In this
presentation, we shall use the results of an extensive set of systematic simulation runs with our Dynamic Fluid
Kinetic (DyFK) simulation code for ionospheric plasma field-aligned transport to obtain O+ outflow flux levels
versus precipitation electron energy flux levels, characteristic energy levels of the precipitating electron, and the
peak spectral wave densities for BBELF waves which transversely heat ionospheric ions, and other geophysical
conditions. We shall present spectrograms of the relationship of the ion outflow values to these electron energy
flux and BBELF wave levels. A preliminary approximate formula representation at this time is: FluxO+ =
3.03*(3.0x105 + 0.02x109 fe1.4)(tanh(8Dwave)+0.2Dwave0.6)*exp([500-
En]/390)2.6 where FluxO+ is the O+ number flux in cm-2s-1 at 3RE mapped to 1000
km altitude, fe is the electron precipitation energy flux in ergs cm-2 s-1, and Dwave is the wave
spectral density at 6.5 Hz in (mV)2 m-2 Hz-1m and En is the characteristic energy of the precipitating
electrons. Strangeway, R. J., R. E. Ergun, Y.-J. Su, C. W. Carlson, and R. C. Elphic, Factors controlling
ionospheric outflows as observed at intermediate altitudes, J. Geophys. Res., 110, A03221,
doi:10.1029/2004JA010829, 2005. Zheng, Y., T. E. Moore, F. S. Mozer, C. T. Russell, and R. J. Strangeway, Polar
study of ionospheric ion outflow versus energy input, J. Geophys. Res., 110, A07210, doi:10.1029/2004JA010995,
2005.
DE: 2407 Auroral ionosphere (2704)
DE: 2431 Ionosphere/magnetosphere interactions (2736)
DE: 2704 Auroral phenomena (2407)
DE: 2736 Magnetosphere/ionosphere interactions (2431)
SC: SPA-Magnetospheric Physics [SM]
MN: 2007 Joint Assembly