Search Results - "Jain, Sonal Kumar"
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Monte Carlo model of electron energy degradation in a CO2 atmosphere
Published in Journal of Geophysical Research. A. Space Physics (01-11-2009)“…A Monte Carlo model has been developed to study the degradation of ≤1000 eV electrons in an atmosphere of CO2, which is one of the most abundant species in…”
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CO Cameron band and UV doublet emissions in the dayglow of Venus: Role of CO in the Cameron band production
Published in Journal of geophysical research. Space physics (01-06-2013)“…The present study deals with the model calculations of CO Cameron band and ultraviolet doublet emissions in the dayglow of Venus. The overhead and limb…”
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Forbidden atomic oxygen emissions in the martian dayside upper atmosphere
Published in Icarus (New York, N.Y. 1962) (01-05-2021)“…Recently, Nadir and Occultation for Mars Discovery (NOMAD) ultraviolet and visible spectrometer instrument on board the European Space Agency’s ExoMars Trace…”
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Model calculation of N2 Vegard-Kaplan band emissions in Martian dayglow
Published in Journal of Geophysical Research: Planets (01-07-2011)“…A model for N2 Vegard‐Kaplan (VK) band (A3Σu+ − X1Σg+) emissions in Martian dayglow has been developed to explain the recent observations made by the…”
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CO Cameron band and CO 2 + UV doublet emissions in the dayglow of Venus: Role of CO in the Cameron band production
Published in Journal of geophysical research. Space physics (01-06-2013)“…The present study deals with the model calculations of CO Cameron band and CO 2 + ultraviolet doublet emissions in the dayglow of Venus. The overhead and limb…”
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Production of N2 Vegard–Kaplan and Lyman–Birge–Hopfield emissions on Pluto
Published in Icarus (New York, N.Y. 1962) (15-01-2015)“…•Detail model calculations of N2 triplet and singlet bands emissions on Pluto.•Prediction of N2 VK band LBH Limb intensities for New Horizons mission…”
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Model calculation of N 2 Vegard-Kaplan band emissions in Martian dayglow
Published in Journal of Geophysical Research (28-07-2011)Get full text
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CO Cameron band and CO2+ UV doublet emissions in the dayglow of Venus: Role of CO in the Cameron band production
Published in Journal of geophysical research. Space physics (01-06-2013)“…The present study deals with the model calculations of CO Cameron band and CO2+ ultraviolet doublet emissions in the dayglow of Venus. The overhead and limb…”
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Production of N 2 Vegard–Kaplan and Lyman–Birge–Hopfield emissions on Pluto
Published in Icarus (New York, N.Y. 1962) (15-01-2015)Get full text
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Impact of solar EUV flux on CO Cameron band and CO2+ UV doublet emissions in the dayglow of Mars
Published in Planetary and space science (01-04-2012)“…This study is aimed at making a calculation about the impact of the two most commonly used solar EUV flux models – SOLAR2000 (S2K) of Tobiska (2004) and EUVAC…”
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Production of Vegard-Kaplan and Lyman-Birge-Hopfield emissions on Pluto
Published in Icarus (New York, N.Y. 1962) (01-01-2015)“…We have developed a model to calculate the emission intensities of various vibrational transitions of triplet band and Lyman-Birge-Hopfield (LBH) band…”
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Calculations of N 2 triplet states vibrational populations and band emissions in venusian dayglow
Published in Icarus (New York, N.Y. 1962) (01-02-2012)“…► Steady state photoelectron fluxes calculated using Analytical Yield Spectra technique are compared with the observations. ► Vibrational populations of N 2…”
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Production of N2 Vegard–Kaplan and other triplet band emissions in the dayglow of Titan
Published in Icarus (New York, N.Y. 1962) (01-04-2012)“…► Detailed model calculations of N2 triplet band emissions in Titan’s dayglow. ► Calculated photoelectron flux agrees with the Cassini-CAPS measurements. ►…”
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Calculations of N2 triplet states vibrational populations and band emissions in venusian dayglow
Published in Icarus (New York, N.Y. 1962) (01-02-2012)“…A model for N2 triplet states band emissions in the venusian dayglow has been developed for low and high solar activity conditions. Steady state photoelectron…”
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Variability of D and H in the Martian upper atmosphere observed with the MAVEN IUVS echelle channel
Published in Journal of geophysical research. Space physics (01-02-2017)“…The MAVEN IUVS instrument contains an echelle spectrograph channel designed to measure D and H Ly α emissions from the upper atmosphere of Mars. This channel…”
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Correction to “Monte Carlo model of electron energy degradation in a CO 2 atmosphere”
Published in Journal of Geophysical Research: Space Physics (01-12-2009)Get full text
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Correction to "Monte Carlo model of electron energy degradation in a CO2 atmosphere"
Published in Journal of Geophysical Research. A. Space Physics (01-12-2009)Get full text
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Monte Carlo model of electron energy degradation in a CO 2 atmosphere
Published in Journal of Geophysical Research: Space Physics (01-11-2009)“…A Monte Carlo model has been developed to study the degradation of ≤1000 eV electrons in an atmosphere of CO 2 , which is one of the most abundant species in…”
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Journal Article -
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Nitric oxide nightglow and Martian mesospheric circulation from MAVEN/IUVS observations and LMD‐MGCM predictions
Published in Journal of geophysical research. Space physics (01-05-2017)“…We report results from a study of nitric oxide nightglow over the northern hemisphere of Mars during winter, the southern hemisphere during fall equinox, and…”
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