HR: 1340h
AN: SM23A-0466    [Abstracts]
TI: Local Electron Density Measurements from Sounding Experiments by RPI on IMAGE
AU: Proddaturi, R
EM: ftrkp@uaf.edu
AF: University of Alaska Fairbanks, 306 Tanana Drive, Duckering 203, P.O.Box 755915, Fairbanks, AK 99775-5915 United States
AU: * Sonwalkar, V S
EM: ffvss@uaf.edu
AF: University of Alaska Fairbanks, 306 Tanana Drive, Duckering 203, P.O.Box 755915, Fairbanks, AK 99775-5915 United States
AU: Li, J
EM: fsjl3@uaf.edu
AF: University of Alaska Fairbanks, 306 Tanana Drive, Duckering 203, P.O.Box 755915, Fairbanks, AK 99775-5915 United States
AU: Venkatasubramanian, A
EM: ftav@uaf.edu
AF: University of Alaska Fairbanks, 306 Tanana Drive, Duckering 203, P.O.Box 755915, Fairbanks, AK 99775-5915 United States
AU: Carpenter, D
EM: dlc@nova.stanford.edu
AF: Stanford University, STAR laboratory, Packard Building, Stanford, CA 94305-9515 United States
AU: Benson, R
EM: robert.f.benson@nasa.gov
AF: NASA Goddard Space Flight Center, Code 692, Greenbelt, MD 20771 United States
AU: Reinisch, B
EM: bodo_reinisch@uml.edu
AF: University of Massachusetts, Center for Atmospheric Research, 600 Suffolk Street, Lowell, MA 01845 United States
AB: RPI sounding experiments lead to a variety of echoes, propagating in various plasma wave modes, and local resonances. Characteristic frequencies of these echoes and resonances can be used to determine the local plasma frequency and thus the local electron density. In this work we have estimated plasma frequency by two methods: (1) using upper hybrid frequency measured from the diffuse Z mode echo upper cutoff and gyro-frequency measured from a gap in the diffuse Z mode echo or from resonances at the multiples of gyrofrequency, (2) upper hybrid frequency from the diffuse Z mode and the free space cutoff frequency $f_{R=0}$ from the $R-X$ mode echo. Broadband diffuse Z-mode echoes occur 90$%$ of the time at high latitudes ($\lambda$m$>$45$^\circ$S) near perigee in the southern hemisphere, where $f_{pe} << f_{ce}$. In the middle and low latitudes ($\lambda$m$<$45$^\circ$S), where $f_{pe} >> f_{ce}$, Z-mode echoes are narrowband and are often accompanied by Qn and Dn resonances. The free space $R-X$ mode echoes are commonly observed at both high and low latitudes. Multiples of gyrofrequency are typically observed at mid- to low-latitude in both the northern and southern hemisphere and at high latitude in the northern hemisphere. RPI plasmagrams were analyzed for three orbits (apogee to apogee) in the year 2002. These three orbits were selected because suitable sounding programs, those that can cover Z mode bandwidth over a wide range of latitude, were used, and also because a large number of diffuse Z mode echoes were actually observed. Electron densities as low as 10 el/cc and as high as 9000 el/cc were measured. The transmission frequencies place a limitation on the upper and lower limits of measurable $f_{pe}$. The measured $f_{pe}$ values showed good agreement with measurements made from the thermal noise but showed large deviations when compared with model $f_{pe}$ values. For a particular orbit on August 26, 2002, $N_e$ measured was as low as $\sim$20 el/cc at higher altitudes outside the plasmasphere ($\lambda$m $>$ 60$^\circ$N, altitude $>$7000 km, MLT=1.89) and increased as IMAGE approached the plasmasphere. A maximum of $\sim$8900 el/cc was measured well within the plasmasphere (L = 1.56, $\lambda$m = 17$^\circ$N, altitude $=$2700 km, MLT = 2.44). As the satellite left the plasmasphere, measured electron density decreased to a minimum of about 55 el/cc near the auroral zone (L = 6.83, $\lambda$m = 57$^\circ$S, altitude = 6277 km, MLT=13.66) and then started to rise again. A sharper change in $N_e$ was seen at both the inbound and outbound crossings of the plasmapause. As the satellite again entered the plasmasphere (L = 3.94, $\lambda$m = 21$^\circ$S, altitude = 15500 km, MLT = 14.34) at a higher altitude the maximum value of Ne measured was lower ($\sim$520 el/cc) as expected. Our results demonstrate that magnetospheric sounding experiments employing Z mode and free space modes provide a powerful means of making local plasma density measurements.
DE: 2403 Active experiments
DE: 2407 Auroral ionosphere (2704)
DE: 2443 Midlatitude ionosphere
DE: 2481 Topside ionosphere
DE: 2487 Wave propagation (6934)
SC: SPA-Magnetospheric Physics [SM]
MN: 2004 AGU Fall Meeting