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Titan airglow during eclipse

Geophysical research letters, 2012-09, Vol.39 (18), p.n/a

2012

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Constraining the Upper Level Vibrational Populations of the N2 Lyman‐Birge‐Hopfield Band System Using GOLD Mission's Dayglow Observations

Journal of geophysical research. Space physics, 2022-09, Vol.127 (9), p.n/a

2022

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Atomic Carbon in the Upper Atmosphere of Titan

Astrophysical journal. Letters, 2010-01, Vol.708 (1), p.L18-L21

2010

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Lyman–Birge–Hopfield emissions from electron-impact excited N2

Journal of physics. B, Atomic, molecular, and optical physics, 2010-07, Vol.43 (13), p.135201

2010

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UV Study of the Fourth Positive Band System of CO and O i 135.6 nm From Electron Impact on CO and CO2

Journal of geophysical research. Space physics, 2019-04, Vol.124 (4), p.2954-2977

2019

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Decades-Long Changes of the Interstellar Wind Through Our Solar System

Science (American Association for the Advancement of Science), 2013-09, Vol.341 (6150), p.1080-1082

2013

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Jovian auroral spectroscopy with FUSE: analysis of self-absorption and implications for electron precipitation

Icarus (New York, N.Y. 1962), 2004-10, Vol.171 (2), p.336-355

2004

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Cassini UVIS observations of Titan ultraviolet airglow intensity dependence with solar zenith angle

Geophysical research letters, 2017-01, Vol.44 (1), p.88-96

2017

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Electron impact study of the 100 eV emission cross section and lifetime of the Lyman‐Birge‐Hopfield band system of N2: Direct excitation and cascade

Journal of geophysical research. Space physics, 2017-06, Vol.122 (6), p.6776-6790

2017

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Dissociative excitation of NO2 by electron impact

Journal of physics. B, Atomic, molecular, and optical physics, 2009-09, Vol.42 (18), p.185201-185201 (10)

2009

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Enhanced transport in the polar mesosphere of Jupiter: Evidence from Cassini UVIS helium 584 Å airglow

Journal of Geophysical Research - Planets, 2006-02, Vol.111 (E2), p.E02002-n/a

2006

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Lyman–Birge–Hopfield emissions from electron-impact excited N 2

Journal of physics. B, Atomic, molecular, and optical physics, 2010-07, Vol.43 (13), p.135201

2010

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Electron impact dissociative excitation of O2: 2. Absolute emission cross sections of the OI(130.4 nm) and OI(135.6 nm) lines

Journal of Geophysical Research - Planets, 2003-11, Vol.108 (E11), p.5126-n/a

2003

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Constraining the Upper Level Vibrational Populations of the N 2 Lyman‐Birge‐Hopfield Band System Using GOLD Mission's Dayglow Observations

Journal of geophysical research. Space physics, 2022-09, Vol.127 (9)

2022

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Constraints on Jupiter's hydrogen corona from Galileo UVS observations

Planetary and space science, 2004-04, Vol.52 (5-6), p.415-421

2004

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Middle ultraviolet and visible spectrum of SO2 by electron impact

Journal of Geophysical Research - Space Physics, 2002-07, Vol.107 (A7), p.SIA 2-1-SIA 2-7

2002

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Solar minimum Lyman α sky background observations from Pioneer Venus Orbiter Ultraviolet Spectrometer: Solar wind latitude variation

Journal of Geophysical Research, 1990-09, Vol.95 (A9), p.14855-14861

Ajello, J. M.

1990

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Dissociative excitation of N2O by electron impact

Journal of physics. B, Atomic, molecular, and optical physics, 2008-05, Vol.41 (9), p.095201-095201 (9)

2008

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Electron impact dissociative excitation of O 2 : 2. Absolute emission cross sections of the OI(130.4 nm) and OI(135.6 nm) lines

Journal of Geophysical Research: Planets, 2003-11, Vol.108 (E11)

2003

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Electron impact dissociative excitation of O2: 1. Kinetic energy distributions of fast oxygen atoms

Journal of Geophysical Research - Planets, 2003-11, Vol.108 (E11), p.5125-n/a

2003

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Electron-impact-induced emission cross sections of neon in the extreme ultraviolet

Journal of physics. B, Atomic, molecular, and optical physics, 1996-06, Vol.29 (11), p.2355-2366

1996

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Latitude variations in interplanetary Lyman-α data from the Galileo EUVS modeled with solar He 1083 nm images

Geophysical research letters, 1996-07, Vol.23 (15), p.1893-1896

1996

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UV Study of the Fourth Positive Band System of CO and O i 135.6 nm From Electron Impact on CO and CO 2

Journal of geophysical research. Space physics, 2019-04, Vol.124 (4), p.2954-2977

2019

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High-Resolution Electron-Impact Emission Spectrum of H2. I. Cross Sections and Emission Yields 900-1200 Å

The Astrophysical journal. Supplement series, 2000-07, Vol.129, p.247

2000

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The Galileo and Pioneer Venus ultraviolet spectrometer experiments - Solar Lyman-alpha latitude variation at solar maximum from interplanetary Lyman-alpha observations

The Astrophysical journal, 1992-07, Vol.394 (1, Ju), p.363-377

1992

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Titan airglow during eclipse

Constraining the Upper Level Vibrational Populations of the N2 Lyman‐Birge‐Hopfield Band System Using GOLD Mission's Dayglow Observations

Atomic Carbon in the Upper Atmosphere of Titan

Lyman–Birge–Hopfield emissions from electron-impact excited N2

UV Study of the Fourth Positive Band System of CO and O i 135.6 nm From Electron Impact on CO and CO2

Decades-Long Changes of the Interstellar Wind Through Our Solar System

Jovian auroral spectroscopy with FUSE: analysis of self-absorption and implications for electron precipitation

Cassini UVIS observations of Titan ultraviolet airglow intensity dependence with solar zenith angle

Electron impact study of the 100 eV emission cross section and lifetime of the Lyman‐Birge‐Hopfield band system of N2: Direct excitation and cascade

Dissociative excitation of NO2 by electron impact

Enhanced transport in the polar mesosphere of Jupiter: Evidence from Cassini UVIS helium 584 Å airglow

Lyman–Birge–Hopfield emissions from electron-impact excited N 2

Electron impact dissociative excitation of O2: 2. Absolute emission cross sections of the OI(130.4 nm) and OI(135.6 nm) lines

Constraining the Upper Level Vibrational Populations of the N 2 Lyman‐Birge‐Hopfield Band System Using GOLD Mission's Dayglow Observations

Constraints on Jupiter's hydrogen corona from Galileo UVS observations

Middle ultraviolet and visible spectrum of SO2 by electron impact

Solar minimum Lyman α sky background observations from Pioneer Venus Orbiter Ultraviolet Spectrometer: Solar wind latitude variation

Dissociative excitation of N2O by electron impact

Electron impact dissociative excitation of O 2 : 2. Absolute emission cross sections of the OI(130.4 nm) and OI(135.6 nm) lines

Electron impact dissociative excitation of O2: 1. Kinetic energy distributions of fast oxygen atoms

Electron-impact-induced emission cross sections of neon in the extreme ultraviolet

Latitude variations in interplanetary Lyman-α data from the Galileo EUVS modeled with solar He 1083 nm images

UV Study of the Fourth Positive Band System of CO and O i 135.6 nm From Electron Impact on CO and CO 2

High-Resolution Electron-Impact Emission Spectrum of H2. I. Cross Sections and Emission Yields 900-1200 Å

The Galileo and Pioneer Venus ultraviolet spectrometer experiments - Solar Lyman-alpha latitude variation at solar maximum from interplanetary Lyman-alpha observations

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