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JOURNAL OF GEOPHYSICAL RESEARCH,
VOL. 110,
A11212,
doi:10.1029/2005JA011043,
2005
Multiple spacecraft observations of energetic ions during a high solar wind pressure event
Jiasheng Chen
Center for Space Physics, Boston University, Boston, Massachusetts, USA
Theodore A. Fritz
Center for Space Physics, Boston University, Boston, Massachusetts, USA
Robert B. Sheldon
National Space Science and Technology Center, NASA Marshall Space Flight Center, Huntsville, Alabama, USA
Abstract
On 28 June 1999 the Wind spacecraft (near the forward libration point) observed a large solar wind pressure spike from 0445
UT to 0600 UT. The Polar satellite at 7 hours magnetic local time detected an energetic particle event in the high-altitude
region associated with turbulent diamagnetic cavities from 0512 UT to 0627 UT. The particles and cavities are very similar
to those that were previously found in the high-altitude dayside cusp region. They are independent of both the solar wind
velocity and the interplanetary magnetic field (IMF) vectors. The enhancements of the magnetic field fluctuations in the ultra-low
frequency range measured by the Wind were also observed by the Polar. Most of the time, during the event period, the IMF had
a duskward component, suggesting that cusp diamagnetic cavities also existed in the postnoon sector in the Northern Hemisphere.
Energetic ions of both ionospheric origin and solar wind origin were observed by the Polar spacecraft during this event period.
The He++/H+ ratio in the diamagnetic cavities was a factor of four higher than in the quasi-trapping region before the event onset, while
the He+/He++ ratio in the cavities was more than one order of the magnitude lower. In this event, the measured cusp ions had energies
up to 4 MeV. No clear relationship between the cusp energetic ion flux and the IMF cone angle was found. The Interball 1 spacecraft
located just upstream of the bow shock in the prenoon sector measured an upstream ion event from about 0516 UT to 0600 UT.
The onset of the energetic ions observed by Interball 1 in the upstream event was the same for different energies; the ion
energy spectra were independent of the solar wind velocity and their intensities were independent of the bow shock geometry
and the solar wind density. The energetic ion event onset was first detected in the cusp by Polar at 0512 UT, then near the
bow shock in the prenoon by Interball 1 at 0516 UT, and then in the far upstream by Wind at 0523 UT. The measured energetic
ion intensity decreased with increasing distance from the cusp diamagnetic cavities. These observational facts together with
the IMF directions suggest that (1) this large solar wind pressure event produced an extremely large diamagnetic cavity (>10
R
E
) within the magnetosphere, (2) the bow shock was not the main source of both the cusp and upstream energetic ions, and (3)
the upstream energetic ions most likely came from the cusp.
Received 2
February
2005;
accepted 9
August
2005;
published 11
November
2005.
Keywords: cusp energetic particles;
upstream ion events;
wave/particle interaction;
magnetospheric configuration and dynamics;
bow shock;
interplanetary magnetic fields.
Index Terms: 2784 Magnetospheric Physics: Solar wind/magnetosphere interactions; 2706 Magnetospheric Physics: Cusp; 2740 Magnetospheric Physics: Magnetospheric configuration and dynamics; 2134 Interplanetary Physics: Interplanetary magnetic fields; 2720 Magnetospheric Physics: Energetic particles: trapped.
Full Article (Nonsubscribers may purchase for $9.00, Includes print PDF, file size: 525661 bytes)
Citation: Chen, J., T. A. Fritz, and R. B. Sheldon
(2005),
Multiple spacecraft observations of energetic ions during a high solar wind pressure event,
J. Geophys. Res.,
110,
A11212,
doi:10.1029/2005JA011043.
Copyright 2005 by the American Geophysical Union.
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