Kyoto/SYMASY

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Contents

  1. Development Notes
  2. Summary
  3. Acknowledgement
  4. Data
    1. Merged Plots and Files
    2. Data Subsets

1. Development Notes

Note that the SPASE metadata links are not yet active.

2. Summary

From: swdcwww.kugi.kyoto-u.ac.jp/figs/logoh.gif
From: swdcwww.kugi.kyoto-u.ac.jp/figs/logoh.gif

For more information on these data, see asy.pdf from original data source: Kyoto WDC. Related works (referenced in asy.pdf above):

  • Storm-time magnetospheric currents inferred from mid-latitude geomagnetic field variations, Iyemori, 1990
  • On the distinction between the auroral electrojet and partial ring current systems, Crooker and McPherron, 1972
  • High-Time Resolution of the Low-Latitude Asymmetric Disturbance in the Geomagnetic Field, Crooker, 1972
  • Decay of the Dst field of geomagnetic disturbance after substorm onset and its implication to storm-substorm relation, Iyemori, 1996
  • The relative importance of the interplanetary electric field and magnetospheric substorms on partial ring current development Clauer and McPherron, 1980
  • Solar wind control of the low-latitude asymmetric magnetic disturbance field, Clauer et al. 1983
  • Low-Latitude DS Component of Geomagnetic Storm Field, Kawasaki and Akasofu

Other references:

3. Acknowledgement

From: http://swdcwww.kugi.kyoto-u.ac.jp/wdc/Sec3.html

The rules for the data use and exchange are defined by the Guide on the World Data Center System (ICSU Panel on World Data Centers, 1996). Note that information on the appropriate institution(s) is also supplied with the WDC data sets. If the data are used in publications and presentations, the data suppliers and the WDC for Geomagnetism, Kyoto must properly be acknowledged.

Commercial use and re-distribution of WDC data are, in general, not allowed. Please ask for the information of each observatory to the WDC.

The construction of this database has been supported in part (as "Solar-Terrestrial Physics Database") by grant 127008, 168069, 178061, 188071, 198053 and 208041 under the Japan Society for Promotion of Science (JSPS). We also thank many geomagnetic observatories, institutions and international organizations which kindly supply the data to our data center.

4. Data

4.1. Merged Plots and Files

  • Overview data coverage plot: | png | pdf | eps |

4.2. Data Subsets

data/Kyoto/SYMASY/xml/Kyoto SYMASY-ORDER-0.htm - ViRBO

data/Kyoto/SYMASY/xml/Kyoto SYMASY-ORDER-0.htm

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