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Variability of Atomic Hydrogen Brightness in the Martian Exosphere: Insights From the Emirates Ultraviolet Spectrometer on Board Emirates Mars Mission.
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- Journal of Geophysical Research. Space Physics, 2024, v. 129, n. 6, p. 1, doi. 10.1029/2024JA032525
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Seasonal Enhancement in Upper Atmospheric D/H at Mars Driven by Both Thermospheric Temperature and Mesospheric Water.
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- Geophysical Research Letters, 2024, v. 51, n. 4, p. 1, doi. 10.1029/2023GL106793
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MAVEN/IUVS Observations of OH Prompt Emission: Daytime Water Vapor in the Thermosphere of Mars.
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- Journal of Geophysical Research. Planets, 2024, v. 129, n. 1, p. 1, doi. 10.1029/2023JE007982
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Evidence of Non‐Thermal Hydrogen in the Exosphere of Mars Resulting in Enhanced Water Loss.
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- Journal of Geophysical Research. Planets, 2023, v. 128, n. 8, p. 1, doi. 10.1029/2023JE007801
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Dayside Temperature Maps of the Upper Mesosphere and Lower Thermosphere of Mars Retrieved From MAVEN IUVS Observations of O I 297.2 nm Emission.
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- Journal of Geophysical Research. Planets, 2023, v. 128, n. 2, p. 1, doi. 10.1029/2022JE007325
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Reappraising the Production and Transfer of Hydrogen Atoms From the Middle to the Upper Atmosphere of Mars at Times of Elevated Water Vapor.
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- Journal of Geophysical Research. Planets, 2022, v. 127, n. 5, p. 1, doi. 10.1029/2022JE007217
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Higher Martian Atmospheric Temperatures at All Altitudes Increase the D/H Fractionation Factor and Water Loss.
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- Journal of Geophysical Research. Planets, 2020, v. 125, n. 12, p. 1, doi. 10.1029/2020JE006626
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Martian Oxygen and Hydrogen Upper Atmospheres Responding to Solar and Dust Storm Drivers: Hisaki Space Telescope Observations.
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- Journal of Geophysical Research. Planets, 2020, v. 125, n. 12, p. 1, doi. 10.1029/2020JE006500
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MARS CLIMATE CONTROLS ATMOSPHERIC ESCAPE: DUST-DRIVEN ESCAPE FROM SURFACE TO SPACE WITH MRO/MCS, TGO/NOMAD, TGO/ACS, AND MAVEN/IUVS.
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- LPI Contribution, 2019, p. 1
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VARIABILITY OF THE MARTIAN HOT OXYGEN CORONA OBSERVED BY MAVEN/IUVS AND IMPLICATIONS FOR ATMOSPHERIC EVOLUTION.
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- LPI Contribution, 2019, p. 1
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Martian Thermospheric Response to an X8.2 Solar Flare on 10 September 2017 as Seen by MAVEN/IUVS.
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- Geophysical Research Letters, 2018, v. 45, n. 15, p. 7312, doi. 10.1029/2018GL077731
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Global Aurora on Mars During the September 2017 Space Weather Event.
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- Geophysical Research Letters, 2018, v. 45, n. 15, p. 7391, doi. 10.1029/2018GL077772
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Mars H Escape Rates Derived From MAVEN/IUVS Lyman Alpha Brightness Measurements and Their Dependence on Model Assumptions.
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- Journal of Geophysical Research. Planets, 2018, v. 123, n. 8, p. 2192, doi. 10.1029/2018JE005574
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Seasonal Changes in Hydrogen Escape From Mars Through Analysis of HST Observations of the Martian Exosphere Near Perihelion.
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- Journal of Geophysical Research. Space Physics, 2017, v. 122, n. 11, p. 11,756, doi. 10.1002/2017JA024572
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Detection of a persistent meteoric metal layer in the Martian atmosphere.
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- Nature Geoscience, 2017, v. 10, n. 6, p. 401, doi. 10.1038/ngeo2958
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Martian mesospheric cloud observations by IUVS on MAVEN: Thermal tides coupled to the upper atmosphere.
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- Geophysical Research Letters, 2017, v. 44, n. 10, p. 4709, doi. 10.1002/2017GL072717
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Nitric oxide nightglow and Martian mesospheric circulation from MAVEN/IUVS observations and LMD-MGCM predictions.
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- Journal of Geophysical Research. Space Physics, 2017, v. 122, n. 5, p. 5782, doi. 10.1002/2016JA023523
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Elevated atmospheric escape of atomic hydrogen from Mars induced by high-altitude water.
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- Nature Geoscience, 2017, v. 10, n. 3, p. 174, doi. 10.1038/ngeo2887
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Variability of D and H in the Martian upper atmosphere observed with the MAVEN IUVS echelle channel.
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- Journal of Geophysical Research. Space Physics, 2017, v. 122, n. 2, p. 2336, doi. 10.1002/2016JA023479
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Three-dimensional structure in the Mars H corona revealed by IUVS on MAVEN.
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- Geophysical Research Letters, 2015, v. 42, n. 21, p. 9001, doi. 10.1002/2015GL065287
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MAVEN IUVS observation of the hot oxygen corona at Mars.
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- Geophysical Research Letters, 2015, v. 42, n. 21, p. 9009, doi. 10.1002/2015GL065487
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The structure and variability of Mars upper atmosphere as seen in MAVEN/IUVS dayglow observations.
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- Geophysical Research Letters, 2015, v. 42, n. 21, p. 9023, doi. 10.1002/2015GL065419
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Study of the Martian cold oxygen corona from the OI 130.4nm by IUVS/MAVEN.
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- Geophysical Research Letters, 2015, v. 42, n. 21, p. 9031, doi. 10.1002/2015GL065341
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Retrieval of CO<sub>2</sub> and N<sub>2</sub> in the Martian thermosphere using dayglow observations by IUVS on MAVEN.
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- Geophysical Research Letters, 2015, v. 42, n. 21, p. 9040, doi. 10.1002/2015GL065489
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New observations of molecular nitrogen in the Martian upper atmosphere by IUVS on MAVEN.
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- Geophysical Research Letters, 2015, v. 42, n. 21, p. 9050, doi. 10.1002/2015GL065319
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Probing the Martian atmosphere with MAVEN/IUVS stellar occultations.
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- Geophysical Research Letters, 2015, v. 42, n. 21, p. 9064, doi. 10.1002/2015GL065294
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MAVEN IUVS observations of the aftermath of the Comet Siding Spring meteor shower on Mars.
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- Geophysical Research Letters, 2015, v. 42, n. 12, p. 4755, doi. 10.1002/2015GL063863
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