Asset Details

  • Description:
  • Probability density as in Figure 9 relevant to Alfvénic Mach number (Ma) versus sound Mach number (MS) and dynamic pressure (PSW) for the three subsets of HSS, MC, and NCDE. As in Figure 9, results are displayed in the same range of values in order to easily identify the probability peak position but with different color scale.
  • License:
  • Rights Managed
  • Rights Holder:
  • John Wiley & Sons, Inc.
  • License Rights Holder:
  • ©2020. American Geophysical Union. All Rights Reserved.
  • Asset Type:
  • Image
  • Asset Subtype:
  • Chart/Graph
  • Image Orientation:
  • Portrait
  • Image Dimensions:
  • 2128 x 2971
  • Image File Size:
  • 18.1 MB
  • Creator:
  • P. Diego, M. Piersanti, M. Laurenza, U. Villante
  • Credit:
  • Diego, P., Piersanti, M., Laurenza, M., & Villante, U. (2020). Properties of Solar Wind Structures at Mercury's Orbit. Journal of Geophysical Research: Space Physics, 125(9), n/a. https://doi.org/10.1029/2020JA028281.
  • Collection:
  • Keywords:
  • Restrictions:
  • Property Release:
  • No
  • Model Release:
  • No
  • Purchasable:
  • Yes
  • Sensitive Materials:
  • No
  • Article Authors:
  • P. Diego, M. Piersanti, M. Laurenza, U. Villante
  • Article Copyright Year:
  • 2020
  • Publication Volume:
  • 125
  • Publication Issue:
  • 9
  • Publication Date:
  • 09/01/2020
  • DOI:
  • https://doi.org/10.1029/2020JA028281

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