IPS Observations of the Solar Wind

Solar Wind Data Obtained from STE Lab. IPS Observations

• IPS Data Archives

  • Solar Wind Speed (undeconloved) Data - VLIST,g-value,IPSCDF-format data, etc (Text Format)

  • Synoptic Maps derived from CAT Analysis

  • Synoptic Maps derived from CAT Analysis (http menu)

  • Real-time Data (Text Format)

  • Solar Wind Data at Planets, produced by MHD IPS Tomography

    • Mercury
    • Venus
    • Mars
    • Jupiter

  • Real-Time Data

    • Near-Realtime Display of All-Sky g-Map

    • Space Weather Forecast from Heliospheric Tomography of ISEE IPS Data
      • UCSD Version

  Note:
  When one wrote a paper using ISEE IPS data, he/she should include the following acknowledgement.
  "IPS observations were made under the solar wind program of the Institute for Space-Earth Environmental Research, Nagoya University."
  When the paper is published, please let us know. We would appreciate that he/her sends us a copy of the paper.
  

• ISEE Multi-Station IPS System

  • 327 MHz Radio Telescope Array Dedicated for IPS Observations

  • Solar WInd Observatories (PDF)

  • Today's Picture of IPS Antennas

References:

Kojima, M. and T. Kakinuma, Solar cycle dependence of global distribution of the solar wind speed, Space Sci. Rev., 53, 173-222, 1990.

Asai, K., Y. Ishida, M. Kojima, K. Maruyama, H. Misawa, and N. Yoshimi, Multi-station system for solar wind observations using the interplanetary scintillation method, J. Geomag. Geoelectr., 47, 1107-1112, 1995.

Tokumaru, M., M. Kojima, K. Fujiki, K. Maruyama, Y. Maruyama, H. Ito, and T. Iju, A newly-developed UHF radio telescope for interplanetary scintillation observations; Solar Wind Imaging Facility, Radio Sci., 46, RS0F02, 2011 (doi:10.1029/2011RS004694).

Tokumaru,Three-dimensional exploration of the solar wind using observations of interplanetary scintillation, Proceedings of the Japan Academy, Series B, 89, 2, 67-79, 2014.

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