An update to the Horizontal Wind Model (HWM): The quiet time thermosphere

D. P. Drob(United States Naval Research Laboratory), J. T. Emmert(United States Naval Research Laboratory), J. W. Meriwether(Clemson University), J. J. Makela(University of Illinois Urbana-Champaign), Eelco Doornbos(Delft University of Technology), M. Conde(University of Alaska Fairbanks), G. Hernández(University of Washington), J. Noto(Scientific Solutions (United States)), Kate Zawdie(United States Naval Research Laboratory), S. E. McDonald(United States Naval Research Laboratory), Joe D. Huba(United States Naval Research Laboratory), J. Klenzing(Goddard Space Flight Center)
Earth and Space Science
April 23, 2015
Cited by 693Open Access
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Abstract

The Horizontal Wind Model (HWM) has been updated in the thermosphere with new observations and formulation changes. These new data are ground‐based 630 nm Fabry‐Perot Interferometer (FPI) measurements in the equatorial and polar regions, as well as cross‐track winds from the Gravity Field and Steady State Ocean Circulation Explorer (GOCE) satellite. The GOCE wind observations provide valuable wind data in the twilight regions. The ground‐based FPI measurements fill latitudinal data gaps in the prior observational database. Construction of this reference model also provides the opportunity to compare these new measurements. The resulting update (HWM14) provides an improved time‐dependent, observationally based, global empirical specification of the upper atmospheric general circulation patterns and migrating tides. In basic agreement with existing accepted theoretical knowledge of the thermosphere general circulation, additional calculations indicate that the empirical wind specifications are self‐consistent with climatological ionosphere plasma distribution and electric field patterns.


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