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Found 5 entries in the Bibliography.
Showing entries from 1 through 5
2018 |
Inversion of space-borne remote sensing measurements of the resonantly scattered solar Lyman alpha (121.6-nm) emission in planetary atmospheres is the most promising means of quantifying the H density in a vast volume of space near terrestrial planets. Owing to the highly nonlinear nature of the inverse problem and the lack of sufficient data constraints over the large volume of space where H atoms are present, previous inversion methods relied on physics-based parametric formulations of the H density distributions to gua ... Qin, Jianqi; Harding, Brian; Waldrop, Lara; Published by: Journal of Geophysical Research: Space Physics Published on: 09/2018 YEAR: 2018   DOI: 10.1029/2018JA025954 |
2017 |
Redistribution of H atoms in the upper atmosphere during geomagnetic storms Geocoronal H emission data acquired by NASA\textquoterights Thermosphere Ionosphere Mesosphere Energetics and Dynamics mission are analyzed to quantify the H density distribution over the entire magnetosphere-ionosphere-thermosphere region in order to investigate the response of the atmospheric system as a whole to geomagnetic storms. It is shown that at low and middle latitudes the H density averaged over storm times in the thermosphere-exosphere transition region decreases by \~30\%, while the H density at exospheric al ... Qin, Jianqi; Waldrop, Lara; Makela, Jonathan; Published by: Journal of Geophysical Research: Space Physics Published on: 08/2017 YEAR: 2017   DOI: 10.1002/jgra.v122.1010.1002/2017JA024489 |
2016 |
Non-thermal hydrogen atoms in the terrestrial upper thermosphere Model predictions of the distribution and dynamical transport of hydrogen atoms in the terrestrial atmosphere have long-standing discrepancies with ultraviolet remote sensing measurements, indicating likely deficiencies in conventional theories regarding this crucial atmospheric constituent. Here we report the existence of non-thermal hydrogen atoms that are much hotter than the ambient oxygen atoms in the upper thermosphere. Analysis of satellite measurements indicates that the upper thermospheric hydrogen temperature, m ... Published by: Nature Communications Published on: 12/2016 YEAR: 2016   DOI: 10.1038/ncomms13655 |
2015 |
Radiative transfer modeling of the OI 135.6~nm emission in the nighttime ionosphere Remote sensing of the nighttime OI 135.6\ nm emissions has been a widely used method for measuring the\ F\ region ionospheric plasma densities. In this work, we first develop a comprehensive radiative transfer model from first principles to investigate the effects of different physical processes on the production and transport of the 135.6\ nm photons in the ionosphere and then propose a new approach for estimating electron densities from the nightglow. The forward modeling investigation indic ... Qin, Jianqi; Makela, Jonathan; Kamalabadi, Farzad; Meier, R.; Published by: Journal of Geophysical Research: Space Physics Published on: 11/2015 YEAR: 2015   DOI: 10.1002/jgra.v120.1110.1002/2015JA021687 OI 135.6-nm Emission; onosphere; Radiative transfer; remote sensing |
2012 |
Optical System Design of a Spaceborne Broadband Far Ultraviolet Hyperspectral Imager According to the application requirements for remote sensing of upper atmosphere,a reflective optical system of spaceborne far ultraviolet hyperspectral imager is designed.Which is composed of a scan mirror,an off-axis parabolic telescope and a toroidal grating spectrometer.An aberration-correction method for concave toroidal grating is developed.The initial parameters are solved based on the geometrical aberration theory of concave grating and then optimized using the optical design software Zemax,and the toroidal gating ... Published by: Acta Optica Sinica Published on: optical design hyperspectral imager toroidal grating far ultraviolet geometrical aberration |
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