Asset Details

  • Description:
  • The scatterplot of (a) solar wind speed, (b) southward IMF Bz, (c) SYM‐H index, and (d) AL index with the μ = 1000 MeV/G electron PSD enhancements at L* = 4.5.
  • 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:
  • Landscape
  • Image Dimensions:
  • 2128 x 1778
  • Image File Size:
  • 616 KB
  • 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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