データアーカイブ

MAGDAS/CPMN

MAGnetic Data Acquisition System/
Circum-pan Pacific Magnetmeter Network Data

Our data archives consist of the following four databases.

MAGDAS-II (MAGnetic Data Acquisition System II)
MAGDAS (MAGnetic Data Acquisition System)

(About the MAGDAS and MAGDAS-II)

1 sec. and 1 min. sampling data from August, 2005.
This network is the integrated latter three networks.
The principal investigator (PI) is Dr. A. Yoshikawa.

(Supporting Information)

This MAGDAS observation was made by the financial supports of Japan Society for the Promotion of Science (JSPS) as Grant-in-Aid for Overseas Scientific Survey (15253005, 18253005). This database was made by the financial supports of Japan Society for the Promotion of Science (JSPS) as Grant-in-Aid for Publication of Scientific Research Results(188068, 198055, 208043), and National Institute of Information and Communications Technology(NiCT) as the funded research.

CPMN (The Circum-pan Pacific Magnetometer Network)

(About the Circum-pan Pacific Magnetometer Network)

1 sec., 3 sec. and 1 min. sampling data from January, 1996.
This network is the integrated latter two networks.
The principal investigator (PI) is Dr. A. Yoshikawa.

(Supporting Information)

This database was made by the financial supports of Japan Society for the Promotion of Science (JSPS) as Grant-in-Aid for Publication of Scientific Research Results (128068,138059,148071,158068,168066, 188068, 198055, 208043).

The 210 MM Magnetic Observation Network

(About the 210 MM Magnetic Observation Network)

1 sec. and 1 min. sampling data from May, 1990 to December, 1995.
The PI is Dr. A. Yoshikawa.

The Equatorial Magnetometer Network

(About the Equatorial Magnetometer Network)

3 sec. sampling data from December, 1985 to December, 1996.
The PI is Prof. T-.I. Kitamura who retired in 1995.

*) These databases were funded in part by the Japan Society for the Promotion of Science (JSPS)
as Grant-in-Aid for Publication of Scientific Research Results (128068,138059,148071,158068,168066,188068,198055, 208043).

important Rules for data usage

Scientists who want to engage in collaboration with ICSWSE
should contact the project leader of MAGDAS/CPMN
observations, Dr. A. Yoshikawa, Kyushu Univ., who will
organize such collaborations.

There is a possibility that the PI of MAGDAS will arrange offers
so that there is less overlapping of themes between MAGDAS research groups

Before you use MAGDAS/CPMN data for your papers,
you must agree to the following points;

Before you submit your paper, you must contact the PI
(Dr. A. Yoshikawa: yoshi@geo.kyushu-u.ac.jp) and
discuss authorship.
When you submit your paper after doing the above item 1, you must mention
the source of the data in the acknowledgment section of your paper.
In general, you must use the following references:
1. Yumoto, K., and the 210MM Magnetic Observation Group, The STEP
  210 magnetic meridian network project, J. Geomag. Geoelectr.,
  48, 1297-1310., 1996. [PDF]
2. Yumoto, K. and the CPMN Group, Characteristics of Pi 2 magnetic
  pulsations observed at the CPMN stations: A review of the STEP
  results, Earth Planets Space, 53, 981-992, 2001. [PDF]
3. Yumoto K. and the MAGDAS Group, MAGDAS project and its application
  for space weather, Solar Influence on the Heliosphere and Earth's
  Environment: Recent Progress and Prospects, Edited by N. Gopalswamy
  and A. Bhattacharyya, ISBN-81-87099-40-2, pp. 309-405, 2006. [PDF]
4. Yumoto K. and the MAGDAS Group, Space weather activities at SERC for IHY: MAGDAS,
  Bull. Astr. Soc. India, 35, pp. 511-522, 2007. [PDF]
In all circumstances, if anything is published you must send
a hardcopy to the following address:

MAGDAS/CPMN

MAGnetic Data Acquisition System/ Circum-pan Pacific Magnetmeter Network Data

*important* Rules for data usage

MAGnetic Data Acquisition System/
Circum-pan Pacific Magnetmeter Network Data

important Rules for data usage