Asset Details

  • Description:
  • (left column) The time lags in days for the highest correlation coefficients between radiation belt electron PSD and (a) solar wind speed, (c) southward IMF Bz, and (e) solar wind proton density, as a function of the first adiabatic invariant μ and L*; (right column) The corresponding highest correlation coefficients between radiation belt electron PSD with time lag and (b) solar wind speed, (d) southward IMF Bz, and (f) solar wind proton density.
  • License:
  • Rights Managed
  • Rights Holder:
  • John Wiley & Sons, Inc.
  • License Rights Holder:
  • ©2017. American Geophysical Union. All Rights Reserved.
  • Asset Type:
  • Image
  • Asset Subtype:
  • Figure
  • Image Orientation:
  • Portrait
  • Image Dimensions:
  • 2128 x 2133
  • Image File Size:
  • 2.16 MB
  • Creator:
  • H. Zhao, D. N. Baker, A. N. Jaynes, X. Li, S. R. Elkington, S. G. Kanekal, H. E. Spence, A. J. Boyd, C.‐L. Huang, C. Forsyth
  • Credit:
  • Zhao, H., Baker, D. N., Jaynes, A. N., Li, X., Elkington, S. R., Kanekal, S. G., Spence, H. E., Boyd, A. J., Huang, C.-L., & Forsyth, C. (2017). On the relation between radiation belt electrons and solar wind parameters/geomagnetic indices: Dependence on the first adiabatic invariant and L*. Journal of Geophysical Research: Space Physics, 122(2), 1624-1642. https://doi.org/10.1002/2016JA023658.
  • Collection:
  • Keywords:
  • Restrictions:
  • Property Release:
  • No
  • Model Release:
  • No
  • Purchasable:
  • Yes
  • Sensitive Materials:
  • No
  • Article Authors:
  • H. Zhao, D. N. Baker, A. N. Jaynes, X. Li, S. R. Elkington, S. G. Kanekal, H. E. Spence, A. J. Boyd, C.‐L. Huang, C. Forsyth
  • Article Copyright Year:
  • 2017
  • Publication Volume:
  • 122
  • Publication Issue:
  • 2
  • Publication Date:
  • 02/01/2017
  • DOI:

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