HR: 1340h
AN: SA43A-1103 [Abstracts]
TI: Day Side Observations of the Equatorial Anomaly
AU: * Coakley, H
EM: jhcoakley@cc.usu.edu
AF: Utah State University, 4120 Old Main Hill, Logan, UT 84322
United States
AU: Swenson, C M
EM: charles.swenson@engineering.usu.edu
AF: Utah State University, 4120 Old Main Hill, Logan, UT 84322
United States
AU: Moon, T
EM: todd.moon@usu.edu
AF: Utah State University, 4120 Old Main Hill, Logan, UT 84322
United States
AU: Meier, R R
EM: meier@uap2.nrl.navy.mil
AF: School of Computational Sciences, George Mason University
4400 University Drive, MS 5C3, Fairfax, VA 22030
United States
AU: Paxton, L
EM: larry.paxton@jhuapl.edu
AF: Applied Physics Laboratory, The Johns Hopkins University
Applied Physics Laboratory, Laurel, MD 20723
United States
AU: Christensen, A
EM: andrew.b.christensen@aero.org
AF: Aerospace Corporation, The Aerospace Corporation, Los Angeles, CA 900009
United States
AB:
The Global Ultraviolet Imager (GUVI) is located on the NASA TIMED space craft. It is in a 630 km circular orbit with an
inclination of 74 degrees. GUVI collects images of the disk and cold side limb in the UV range using a Rowland spectrograph.
These UV emissions can come from several sources including radiative recombination of oxygen ions and electron and day glow
due to solar excitation. These observations of the TIMED spacecraft provide a data set that can be used to study the day time
equatorial anomaly. Three years of data collected by GUVI on the TIMED spacecraft have quality observations of the
equatorial region in high altitude limb scans on the dayside. The combination of the space craft altitude and mirror look
angle make these observations unique. In this paper we present an initial review of these data and their suitability for
observing the day side anomaly and their use in observing the strength of the zonal electric field that creates the
equatorial anomaly.
DE: 0300 ATMOSPHERIC COMPOSITION AND STRUCTURE
DE: 2400 IONOSPHERE (6929)
DE: 3300 ATMOSPHERIC PROCESSES
DE: 7538 Solar irradiance
SC: SPA-Aeronomy [SA]
MN: Fall Meeting 2005