TC1 FGM and HIA Prime Parameters: 2 hours
   QL Summary: 6 hours (DSDSWeb at OEAW)

   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 Figures are NOT for publication.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: FGM 080531 1800-2000 UT

• We thank C. P. Escoubet, Z. X. Liu, and R. Nakamura for the permission to use DSP prime parameter data and their support for this page.
• The PI of TC2 FGM is T. Zhang at IWF/OEAW (see Carr et al. [Ann. Geophys., 23, 2713-2732, 2005] for details of the instrument).
• The time resolution of the FGM data is 4 sec (one spin period).
• The data and TC2 locations are in GSM coordinates.
• See DSDS Users Guide for post processing caveats. CAUTION: FGM data might be affected by magnetic field disturbance. The data have been processed using a preliminary calibration of the instrument. The spacecraft disturbance has not been removed. The data are presented for context and information only. They are not suitable for detailed analysis.
• Data are plotted even if the status is "Use with caution" (Status[0]=1).
• The final data for publications must be checked by the PI.
• dB²/B² denotes the variance of the magnetic field magnitude normalized by the squared field magnitude.

Links

• Double Star at ESA

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

This page was originally produced by Y. Miyashita, T. Takada, M. Fujimoto, H. Hasegawa, and I. Shinohara
and moved from DARTS at C-SODA, ISAS, JAXA in Japan.

Last Modified: 2023/04/21