HR: 0800h
AN: SM41B-1182 [Abstracts]
TI: Pc 1-2 waves and associated ion distributions observed during three extended conjunctions between the
Polar satellite and Antarctic ground stations
AU: * Argall, M
EM: argall@augsburg.edu
AF: Augsburg College, 2211 Riverside Ave, Minneapolis, MN 55454
United States
AU: Engebretson, M J
EM: engebret@augsburg.edu
AF: Augsburg College, 2211 Riverside Ave, Minneapolis, MN 55454
United States
AU: Johnson, J E
EM: johnson9@augsburg.edu
AF: Augsburg College, 2211 Riverside Ave, Minneapolis, MN 55454
United States
AU: Posch, J L
EM: posch@augsburg.edu
AF: Augsburg College, 2211 Riverside Ave, Minneapolis, MN 55454
United States
AU: Rowland, D E
EM: drowland@lepvax.gsfc.nasa.gov
AF: NASA/Goddard Space Flight Center, Code 696, Greeenbelt, MD 20771
United States
AU: Chen, S -
EM: schen@pop600.gsfc.nasa.gov
AF: NASA/Goddard Space Flight Center, Code 696, Greeenbelt, MD 20771
United States
AU: Moore, T E
EM: thomas.e.moore@nasa.gov
AF: NASA/Goddard Space Flight Center, Code 696, Greeenbelt, MD 20771
United States
AU: Peterson, W K
EM: bill.peterson@lasp.colorado.edu
AF: University of Colorado - LASP, 1234 Innovation Dr, Boulder, CO 80303
United States
AU: Onsager, T G
EM: Terry.Onsager@noaa.gov
AF: NOAA, Space Environment Center, Boulder, CO 80303
United States
AU: Johnson, J R
EM: jrj@pppl.gov
AF: Princeton University, Plasma Physics Lab, Princeton, NJ 08543
United States
AU: Lessard, M R
EM: marc.lessard@unh.edu
AF: University of New Hampshire, Space Science Center, Durham, NH 03824
United States
AU: Arnoldy, R L
EM: roger.arnoldy@unh.edu
AF: University of New Hampshire, Space Science Center, Durham, NH 03824
United States
AU: Russell, C T
EM: ctrussell@igpp.ucla.edu
AF: University of California- Los Angeles, IGPP, Los Angeles, CA 90024
United States
AB:
We present ground and satellite observations of Pc 1 and 2 waves and
associated ion distributions that occurred during three extended
intervals in spring 2003 when the Polar satellite traveled northward
across the magnetic equator near local noon along outer magnetospheric
flux tubes (L = 9 - 11) that mapped to near the location of an array
of search coil magnetometers in Antarctica. Observations of < 1 eV to
25 keV ions by the TIDE, TIMAS, and Hydra instruments on Polar provide
information on the ion populations associated with these waves. Steady,
enhanced fluxes of anisotropic > 5 keV protons were observed throughout
each of the intervals shown. Their presence appears to be a "necessary
but not sufficient" condition for ion cyclotron instability, suggesting
that the outer dayside magnetosphere is near marginal stability but
needs an additional trigger to cause rapid wave growth. During each of
these three intervals, bursts of ~ 0.5 ± 0.2 Hz Pc 1 waves often
coincided with short-lived increases in the flux of < 1 keV ions. Pc 2
waves, with frequency below the inferred equatorial He+ gyrofrequency,
also occurred on February 11, 2003 in association with an inferred
strong enhancement in trapped < 200 eV He+ ions. During the other two
passes compressions and/or twists of the magnetic field were also
associated with several wave bursts. Our observations thus suggest that
either additional lower energy ions or compressions/twists of the
magnetic field can often be sufficient to cause rapid wave growth in the
outer dayside magnetosphere. Poynting vectors calculated along the
satellite trajectory indicate mixed equatorward/poleward wave
propagation below ± 20 ° magnetic latitude, but consistently poleward
propagation at higher latitudes.
DE: 2720 Energetic particles: trapped
DE: 2731 Magnetosphere: outer
DE: 2752 MHD waves and instabilities (2149, 6050, 7836)
SC: SPA-Magnetospheric Physics [SM]
MN: Fall Meeting 2005