文献
J-GLOBAL ID:201702217052053748
整理番号:17A1210147
火星ミッションの安全性のための高エネルギー太陽陽子の発生の予測の可能性【Powered by NICT】
Possibilities of the forecast of generation of the high energy solar protons for the safety of Mars mission
著者 (6件):
Avakyan S.V.
(All-Russian Scientific Center “S.I.Vavilov State Optical Institute”, 12, Line Birgevaya, Saint-Petersburg 199034, Russia)
,
Avakyan S.V.
(Peter the Great St. Petersburg Polytechnical University, 29, Polytechnicheskaya street, Saint-Petersburg, 195251, Russia)
,
Avakyan S.V.
(Russian State Scientific Center for Robotics and Technical Cybernetics, 21, Tikhoretsky pr., Saint-Petersburg 194064, Russia)
,
Gaponov V.A.
(Russian State Scientific Center for Robotics and Technical Cybernetics, 21, Tikhoretsky pr., Saint-Petersburg 194064, Russia)
,
Nicol’skii G.A.
(Saint-Petersburg State Universiity, 196105, per. Jakovlevskii, 10/16, Saint-Petersburg, Russia)
,
Solov’ev A.A.
(Central (Pulkovo) astronomical observatory of RAS, 196140, Pulkovskoe shausse, 65/1, Saint-Petersburg, Russia)
資料名:
Acta Astronautica
(Acta Astronautica)
巻:
135
ページ:
187-191
発行年:
2017年
JST資料番号:
B0035B
ISSN:
0094-5765
資料種別:
逐次刊行物 (A)
記事区分:
原著論文
発行国:
オランダ (NLD)
言語:
英語 (EN)