Contribution of charge exchange loss to the storm time ring current decay: IMAGE/HENA observations

  • K. Keika
    Department of Geophysics, Graduate School of Science Kyoto University Kyoto Japan
  • M. Nosé
    Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science Kyoto University Kyoto Japan
  • P. C. Brandt
    Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA
  • S. Ohtani
    Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA
  • D. G. Mitchell
    Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA
  • E. C. Roelof
    Johns Hopkins University Applied Physics Laboratory Laurel Maryland USA

書誌事項

公開日
2006-11
権利情報
  • http://onlinelibrary.wiley.com/termsAndConditions#vor
DOI
  • 10.1029/2006ja011789
公開者
American Geophysical Union (AGU)

この論文をさがす

説明

<jats:p>The present study addresses the contribution of charge exchange loss of the ring current ions to the decay of the storm time ring current, based on measurements of energetic neutral atoms (ENAs) made by the High Energy Neutral Atom (HENA) imager on board the Imager for Magnetopause‐to‐Aurora Global Exploration (IMAGE) satellite. The energy range of ENA fluxes examined in the present study is from 27 to 119 keV for hydrogen and from 79 to 264 keV for oxygen. This is the first statistical estimate of the charge exchange contribution made with dedicated measurements of both neutral hydrogen and oxygen. We estimate charge exchange energy losses of the ring current ions, employing two independent methods. The decay rate of the ring current is derived from the temporal variations of the Dst index. Our estimates show that the rate of the charge exchange energy losses is comparable to the ring current decay rate for the intervals of the slow decay, while the loss rate is much smaller than the decay rate in the rapid decay phase in particular for the early stage of a storm recovery. The logarithm of the energy loss rate is well correlated with the simultaneous Dst index, increasing as Dst decreases. Utilizing the high correlations, we simulate a Dst recovery due to charge exchange loss alone. Pressure‐corrected Dst (Dst<jats:sub>0</jats:sub>) recoveries derived from measured Dst cannot be reproduced by charge exchange loss alone. We conclude that the charge exchange loss is not primarily responsible for the rapid decay of the storm time ring current.</jats:p>

収録刊行物

被引用文献 (9)*注記

もっと見る

問題の指摘

ページトップへ