Asset Details

  • Description:
  • Correlation Coefficients Between the Corrected GW Amplitudes and Upper Thermospheric Temperature (T0), SZA Where NGIMS Measured N(Ar) = 105 cm−3, Solar EUV Irradiances Measured in Channel A (17–22 nm), Channel B (0.1–7 nm), and Channel C (121–122 nm), Solar Wind Dynamic Pressure, Solar Wind Density, and Solar Wind Velocity for the Inbound, Outbound, and All Legs
  • License:
  • Rights Managed
  • Rights Holder:
  • John Wiley & Sons, Inc.
  • License Rights Holder:
  • ©2017. American Geophysical Union. All Rights Reserved.
  • Asset Type:
  • Image
  • Asset Subtype:
  • Table
  • Image Orientation:
  • Landscape
  • Image Dimensions:
  • 1024 x 653
  • Image File Size:
  • 208 KB
  • Creator:
  • Naoki Terada, François Leblanc, Hiromu Nakagawa, Alexander S. Medvedev, Erdal Yiğit, Takeshi Kuroda, Takuya Hara, Scott L. England, Hitoshi Fujiwara, Kaori Terada, Kanako Seki, Paul R. Mahaffy, Meredith Elrod, Mehdi Benna, Joseph Grebowsky, Bruce M. Jakosky
  • Credit:
  • Terada, N. (2017). Global distribution and parameter dependences of gravity wave activity in the Martian upper thermosphere derived from MAVEN/NGIMS observations. Journal of Geophysical Research: Space Physics, 122(2), 2374-2397. https://doi.org/10.1002/2016JA023476.
  • Collection:
  • Keywords:
  • Restrictions:
  • Property Release:
  • No
  • Model Release:
  • No
  • Purchasable:
  • Yes
  • Sensitive Materials:
  • No
  • Article Authors:
  • Naoki Terada, François Leblanc, Hiromu Nakagawa, Alexander S. Medvedev, Erdal Yiğit, Takeshi Kuroda, Takuya Hara, Scott L. England, Hitoshi Fujiwara, Kaori Terada, Kanako Seki, Paul R. Mahaffy, Meredith Elrod, Mehdi Benna, Joseph Grebowsky, Bruce M. Jakosky
  • Article Copyright Year:
  • 2017
  • Publication Volume:
  • 122
  • Publication Issue:
  • 2
  • Publication Date:
  • 02/01/2017
  • DOI:

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