An update to the Horizontal Wind Model (HWM): The quiet time thermosphere
DP Drob, JT Emmert, JW Meriwether… - Earth and Space …, 2015 - Wiley Online Library
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 …
observations and formulation changes. These new data are ground‐based 630 nm Fabry …
Neutral winds from mesosphere to thermosphere—past, present, and future outlook
The Earth's upper atmosphere (85–550 km) is the nearest region of geospace and is highly
dynamic in nature. Neutral winds impact a large portion of the dynamics in this region. They …
dynamic in nature. Neutral winds impact a large portion of the dynamics in this region. They …
Studies of thermospheric dynamics with a Fabry–Perot interferometer network: A review
JW Meriwether - Journal of Atmospheric and Solar-Terrestrial Physics, 2006 - Elsevier
Advances in Fabry–Perot interferometer (FPI) technology implemented within the past
decade have been extensive achieving improvements in sensitivity by one or two orders of …
decade have been extensive achieving improvements in sensitivity by one or two orders of …
Development of optical mesosphere thermosphere imagers (OMTI)
K Shiokawa, Y Katoh, M Satoh, MK Ejiri, T Ogawa… - Earth, Planets and …, 1999 - Springer
Abstract The Optical Mesosphere Thermosphere Imagers (OMTI) have been developed to
investigate the dynamics of the upper atmosphere through nocturnal airglow emissions. The …
investigate the dynamics of the upper atmosphere through nocturnal airglow emissions. The …
Spatial structure in the thermospheric horizontal wind above Poker Flat, Alaska, during solar minimum
M Conde, RW Smith - Journal of Geophysical Research: Space …, 1998 - Wiley Online Library
A new all‐sky imaging, wavelength scanning Fabry‐Perot spectrometer was used to record
high‐resolution (R≃ 200,000) spectra of the λ630 nm thermospheric optical emission above …
high‐resolution (R≃ 200,000) spectra of the λ630 nm thermospheric optical emission above …
Characterization of the thermospheric mean winds and circulation during solstice using ICON/MIGHTI observations
E Yiğit, M Dhadly, AS Medvedev… - Journal of …, 2022 - Wiley Online Library
Using the horizontal neutral wind observations from the Michelson Interferometer for Global
High‐resolution Thermospheric Imaging (MIGHTI) instrument onboard NASA's Ionospheric …
High‐resolution Thermospheric Imaging (MIGHTI) instrument onboard NASA's Ionospheric …
An investigation comparing ground‐based techniques that quantify auroral electron flux and conductance
SR Kaeppler, DL Hampton, MJ Nicolls… - Journal of …, 2015 - Wiley Online Library
We present three case studies that examine optical and radar methods for specifying
precipitating auroral flux parameters and conductances. Three events were chosen …
precipitating auroral flux parameters and conductances. Three events were chosen …
Assimilated observations of thermospheric winds, the aurora, and ionospheric currents over Alaska
We present simultaneous measurements of thermospheric winds, auroral emissions, and
ionospheric currents over Alaska, obtained from four separate instruments. Thermospheric …
ionospheric currents over Alaska, obtained from four separate instruments. Thermospheric …
Seasonal dependence of northern high‐latitude upper thermospheric winds: A quiet time climatological study based on ground‐based and space‐based …
This paper investigates the large‐scale seasonal dependence of geomagnetically quiet
time, northern high‐latitude F region thermospheric winds by combining extensive …
time, northern high‐latitude F region thermospheric winds by combining extensive …
Seasonal dependence of geomagnetic active‐time northern high‐latitude upper thermospheric winds
MS Dhadly, JT Emmert, DP Drob… - Journal of …, 2018 - Wiley Online Library
This study is focused on improving the poorly understood seasonal dependence of northern
high‐latitude F region thermospheric winds under active geomagnetic conditions. The gaps …
high‐latitude F region thermospheric winds under active geomagnetic conditions. The gaps …