| Project/Area Number |
06640568
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| Research Category |
Grant-in-Aid for General Scientific Research (C)
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| Allocation Type | Single-year Grants |
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| Research Field |
Space and upper atmospheric physics
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| Research Institution | Nagoya University |
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Principal Investigator |
TAKAHASHI Kazue Nagoya University, Solar-Terrestrial Environment Laboratory, Associate Professor, 太陽地球環境研究所, 助教授 (70252294)
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| Co-Investigator(Kenkyū-buntansha) |
YUMOTO Kiyohumi Nagoya University, Solar-Terrestrial Environment Laboratory, Associate Professor, 太陽地球環境研究所, 助教授 (20125686)
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| Project Period (FY) |
1994 – 1995
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| Project Status |
Completed (Fiscal Year 1995)
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| Budget Amount *help |
¥2,100,000 (Direct Cost: ¥2,100,000)
Fiscal Year 1995: ¥1,000,000 (Direct Cost: ¥1,000,000)
Fiscal Year 1994: ¥1,100,000 (Direct Cost: ¥1,100,000)
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| Keywords | Geomagnetic pulsations / Magnetospheric substorms / MHD waves |
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| Research Abstract |
The spatial variation of the properties of magnetospheric Pi 2 pulsations is studied using magnetic field records acquired simultaneously by the Active Magnetospheric Particle Tracer Explorers Charge Composition Explorer (AMPTE CCE) satellite at radial distances less than 6.6 Earth radii (RE) and at geomagnetic latitudes from -16ﾟ to 16ﾟ and at the Kakioka ground station located at magnetic shell of L=1.23. Pi 2 magnetic pulsations are identified from the Kakioka data acquired within 3 hours of midnight, but no restriction is imposed on the local time of CCE.An automated Pi 2 selection procedure resulted in 249 events from the Kakioka data. We have characterized magnetic field variations in the radial (b_x), azimuthal (b_y), and compressional (b_z) components at CCE in terms of their spectral density, coherence, and phase relative to those of the Pi 2 pulsation in the horizontal (H) component of the Kakioka data and then examined how these parameters depend on the location of CCE.It is
… More
found that high-coherence events (coherence between CCE and Kakioka>0.6) are observed primarily when CCE is on the nightside and at L<4. For these events the magnetic field perturbations at CCE are dominated by the ploidal components b_x and b_z and these components exhibit a ground to satellite cross phase of either -0 or -180ﾟ, depending on the location of the satellite. The spatial phase structure is consistent with the eigenmode structure of a compressional cavity-mode type resonance excited between two reflecting boundaries. We find no evidence supporting the view that ground Pi 2 are mid-latitude toroidal field line resonances excited in response to source waves on auroral zone field lines. Rather, the results imply that mid-latitude (2<L<5) Pi 2 pulsations observed on the ground originate from a cavity-mode type resonance excited in the inner magnetosphere bounded below by the ionosphere and at high altitudes by an Alfven velocity gradient. The cavity resonance is probably excited by earthward propagating fast mode waves launched at substorm onset by the large scale magnetic reconfiguration associated with cross-tail current disruption. Less
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