Spacecraft Footprints and Ground-Based Instruments:
   High-Lat + Mid-Tail 2 hours
   Polar 2 hours (old)

   Conjunction Event Finder

CAUTION!! Figures are NOT for publication.

Postscript File: PWS+VLF+RDM 20140731 2200-0000 UT

• PWS
  • Contact: A. Kumamoto (Tohoku University)
  • Reference: Oya et al., JGG, 42, 411-442, doi:10.5636/jgg.42.411, 1990.
  • Website at DARTS/ISAS/JAXA

• VLF
  • PI: I. Nagano (Kanazawa University)
  • Contact: Y. Kasahara (Kanazawa University)
  • Reference: Kimura et al., JGG, 42, 459-478, doi:10.5636/jgg.42.459, 1990.
  • Website at Kanazawa University

• RDM
  • PI/Contact: T. Nagai (Tokyo Institute of Technology)
  • References: Nagai et al., Geophys. Monogr. Ser., vol. 199, pp. 177-187, doi:10.1029/2012GM001281, AGU, 2012. and Takagi et al., IEEE Trans. Nucl. Sci., 40, 1491-1497, doi:10.1109/23.273513, 1993.
  • Website at DARTS/ISAS/JAXA

• The data are for quick look. Please do not use the plots for publication.
• Both PWS and VLF data may include artificial noise due to the internal calibration etc. Please contact the PI(s) before detailed analysis.
• The white line in the PWS panel indicates the local electron cyclotron frequency. The lines in the VLF panels indicate the local proton cyclotron frequency. These frequencies are calculated from the dipole field.
• The L-value is the McIlwain L derived from the IGRF model.

Links

• DARTS/Akebono at ISAS/JAXA
• Akebono Official Site at ISAS/JAXA

If you have any problems, questions, or comments, please contact the ERG Science Center ("ergsc-help (at) isee.nagoya-u.ac.jp") or Y. Miyoshi ("miyoshi (at) isee.nagoya-u.ac.jp") at ISEE, Nagoya University.

This page is produced by Y. Miyoshi, Y. Miyashita, and T. Hori.

Last Modified: 2023/04/21