論文

2006年1月1日

Plasma/radio wave observations at mercury by the bepicolombo mmo spacecraft

Advances in Geosciences: Volume 3: Planetary Science (PS)
  • H. Matsumoto
  • BEPICOLOMBO MMO PWI TEAM
  • J. L. Bougeret
  • L. G. Blomberg
  • H. Kojima
  • S. Yagitani
  • Y. Omura
  • M. Moncuquet
  • G. Chanteur
  • Y. Kasaba
  • J. G. Trotignon
  • Y. Kasahara
  • 全て表示

3
開始ページ
83
終了ページ
84
記述言語
英語
掲載種別
論文集(書籍)内論文
DOI
10.1142/9789812707192_0008
出版者・発行元
World Scientific Publishing Co.

The BepiColombo Mercury Magnetospheric Orbiter (MMO) spacecraft comprises the plasma and radio wave observation system called PlasmaWave Investigation (PWI). The PWI is designed and developed in collaboration between Japanese and European scientists. Since plasma/radio wave receivers were not installed in the former spacecraft, Mariner 10, which observed the planet Mercury, the PWI onboard the MMO spacecraft will provide the first plasma/radio wave data from Mercury orbit. It will give important information for studies of energy exchange processes in the unique magnetosphere of Mercury characterized by the interaction between the relatively large planet without ionosphere and the solar wind with high dynamic pressure. The PWI consists of three sets of receivers (EWO, SORBET, and AM2P), connected to two sets of electric field sensors (MEFISTO and WPT) and two kinds of magnetic field sensors (LF-SC and DB-SC). The PWI will observe both waveforms and frequency spectra in the frequency range from DC to 10MHz for the electric field

リンク情報
DOI
https://doi.org/10.1142/9789812707192_0008
Scopus
https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84971012498&origin=inward 本文へのリンクあり
Scopus Citedby
https://www.scopus.com/inward/citedby.uri?partnerID=HzOxMe3b&scp=84971012498&origin=inward
ID情報
  • DOI : 10.1142/9789812707192_0008
  • SCOPUS ID : 84971012498

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