Rules for Data Usage
Scientists who want to engage in collaboration with SERC
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: firstname.lastname@example.org) and
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:
Yumoto, K., and the 210MM Magnetic Observation Group, The STEP
210 magnetic meridian network project, J. Geomag. Geoelectr.,
48, 1297-1310., 1996.
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.
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.
Yumoto K. and the MAGDAS Group, Space weather activities at SERC for IHY: MAGDAS,
Bull. Astr. Soc. India, 35, pp. 511-522, 2007.
In all circumstances, if anything is published you must send
a hardcopy to the following address:
Dr. A. Yoshikawa
PI of MAGDAS/CPMN Project
International Center for Space Weather Science and Education,
Kyushu University 53
6-10-1 Hakozaki, Higashi-ku Fukuoka 812-8581, JAPAN
TEL/FAX:+81-92-642-4403, e-mail: email@example.com