discrete ion signature on energy time spectrogram
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Discrete Ion Signature on Energy-Time Spectrogram Maxwellian - PowerPoint PPT Presentation

-- -- Importance of Heavy Ion Species Insufficient Data from Ion


  1. 極域・ 赤道域磁気圏における重イ オン観測 -- エネルギー分散と ピッ チ角・ 速度分布 -- 平原 聖文 ( 立教大学理学部物理学科) Importance of Heavy Ion Species Insufficient Data from Ion Energy-Mass Spectrometers ↓ Discrete Ion Signature on Energy-Time Spectrogram Maxwellian Fitting for Velocity Distribution Function

  2. Data Source Region Akebono Geotail Polar magnetosphere Interball-Aurora Lobe/mantle FAST Magnetopause Plasma sheet Interpretation Dayside magnetosphere Ionospheric origin Plasma sheet acceleration Magnetic field oscillation (Pc 5)

  3. Akebono LEP (Ele. & Ion) Log Ion Energy (eV/q) Log Ele. Energy (eV)

  4. Energy-Dispersing Cause due to Convection

  5. Akebono LEP (Ele. & Ion) December 9, 1989 Energy Ratios of Multiple Energy Dispersions Log Energy (eV/q)

  6. Akebono LEP (Ele. & Ion) & IMS November 8, 1989 Log Energy (eV/q) Log Energy (eV/q)

  7. Sauvaud et al., 1999

  8. Sauvaud et al., 1999

  9. Akebono LEP (Ele. & Ion) & IMS January 30, 1990 UT 13:40 13:48

  10. Akebono & FAST January 19, 1997 Ele. H + O +

  11. Ele. H + O +

  12. Geotail LEP (Ele. & Ion) December 9, 1994

  13. What should be done in future missions? ・ Full Coverages of … Energy (from 0.1 up to 10,000,000 eV) Mass (H + , He 2+ , He + , O + , molecular ions) Pitch angle (0-180 deg) Acceptance Solid angle (~4 π sr) ・ Sufficient Resolutions of … Energy (5-20 %) Angle (1-5 deg) Time (Ele.: 10 msec, Ion: 3 sec)

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