Solar-Terrestrial Data Analysis and Reference System (STARS) - Its High Potentiality for Collaborative Research

M Kunitake; K Yamamoto; S Watari; K Ukawa; H Kato; E Kimura; Y Murayama; K T Murata

doi:10.2481/dsj.WDS-040

Proceedings of the 1st WDS Conference in Kyoto 2011

Solar-Terrestrial Data Analysis and Reference System (STARS) - Its High Potentiality for Collaborative Research

M Kunitake, K Yamamoto, S Watari, K Ukawa, H Kato, E Kimura, Y Murayama, K T Murata

著者情報

M Kunitake
Space Weather and Environment Informatics Lab., National Institute of Information and Communications Technology (NICT), Tokyo, Japan
K Yamamoto
Space Weather and Environment Informatics Lab., National Institute of Information and Communications Technology (NICT), Tokyo, Japan
S Watari
Space Weather and Environment Informatics Lab., National Institute of Information and Communications Technology (NICT), Tokyo, Japan
K Ukawa
Space Weather and Environment Informatics Lab., National Institute of Information and Communications Technology (NICT), Tokyo, Japan
Systems Engineering Consultants Co. Ltd., Tokyo, Japan
H Kato
Space Weather and Environment Informatics Lab., National Institute of Information and Communications Technology (NICT), Tokyo, Japan
E Kimura
Dept. Medical Informatics of Medical School of Ehime Univ., Toon City, Ehime, Japan
Y Murayama
Integrated Science Data System Research Lab., NICT, Tokyo, Japan
K T Murata
Space Weather and Environment Informatics Lab., National Institute of Information and Communications Technology (NICT), Tokyo, Japan

キーワード: Cross-sectional studies, Cooperative work, Combined plot, XML, Collaborative analysis, Common knowledge, Experience sharing, Solar-terrestrial physics, Common use

ジャーナルフリー

2013 年 12 巻 p. WDS225-WDS228

DOI https://doi.org/10.2481/dsj.WDS-040

Browse “Advance online publication” version

詳細

抄録

Cross-sectional studies have become important for an improved understanding of various Solar-Terrestrial Physics (STP) fields, given the great variety and different types of observations from the Sun to the Earth. In order to better combine, compare, and analyze different types of data together, a system named STARS (Solar-Terrestrial data Analysis and Reference System) has been developed. Cross-sectional study requires cooperative work. STARS has two functions for cooperative work, the "Stars Project List (SPL)" and the "Event Listing". The SPL is used for exchanges of plotting information by cooperating persons. The event list database provides all users of STARS hints for recognizing typical occurrences of STP phenomena.

責任著者(Corresponding author)

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