HR: 10:55h
AN: SA22A-03 [Abstracts]
TI: Multi-Platform Ground-Based Observations of Meso-Scale Waves and Spread F at Midlatitudes
AU: * Earle, G
EM: earle@utdallas.edu
AF: University of Texas at Dallas, 2601 N. Floyd Road, Richardson, TX 75083, United States
AU: Bullett, T
EM: Terry.Bullett@noaa.gov
AF: Air Force Research Laboratory, 325 Broadway E/GC2, Boulder, CO 80305, United States
AU: Groves, K
EM: Keith.Groves@hanscom.af.mil
AF: Air Force Research Laboratory, 325 Broadway E/GC2, Boulder, CO 80305, United States
AU: Bishop, R
EM: Rebecca.L.Bishop@aero.org
AF: Aerospace Corporation, POB 92957, Los Angeles, CA 90009, United States
AU: Crowley, G
EM: gcrowley@astraspace.net
AF: Astra-Space Corporation, 12703 Spectrum Drive, San Antonio, TX 78249, United States
AU: Bust, G
EM: gbust@astraspace.net
AF: Astra-Space Corporation, 12703 Spectrum Drive, San Antonio, TX 78249, United States
AU: Tolman, B
EM: btolman@arlut.utexas.edu
AF: University of Texas, ARL, Austin, TX 78758, United States
AU: Calfas, R
EM: rcalfas@arlut.utexas.edu
AF: University of Texas, ARL, Austin, TX 78758, United States
AU: Garner, T
EM: tgarner@arlut.utexas.edu
AF: University of Texas, ARL, Austin, TX 78758, United States
AU: Munton, D
EM: dmunton@arlut.utexas.edu
AF: University of Texas, ARL, Austin, TX 78758, United States
AB:
Three distinctly different midlatitude spread F events were observed on separate nights during a two week period
in the fall of 2006. One of the events occurred after a period of increased activity in several high latitude
geomagnetic storm indices, another occurred during an extended period of magnetically quiescent conditions,
and the third occurred during a moderately active period. The ionospheric and thermospheric conditions during
these events were simultaneously monitored by a suite of ground-based instruments, including the Wallops
Island Digisonde, a tri-static radar sensitive to traveling
ionospheric disturbances (TIDs), scintillation detectors, and
a network of ground-based GPS receivers. We present data from
each of these systems, and contrast the observations on each night in order to investigate the ionospheric
morphologies associated with
each type of spreading event. Evidence of TIDs and plasma
density variations are evident during the quiet-time event, while the geomagnetically active event shows a more
impulsive density perturbation in the TEC data. Smaller scale turbulence and associated scintillations are
evident only in two of the three cases. Plausible scenarios to explain the disparate observations will be
discussed in light of these new data.
DE: 2435 Ionospheric disturbances
DE: 2443 Midlatitude ionosphere
DE: 2772 Plasma waves and instabilities (2471)
SC: SPA-Aeronomy [SA]
MN: 2007 Joint Assembly