Search Results - "López‐Valverde, M. A."
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Strong Localized Pumping of Water Vapor to High Altitudes on Mars During the Perihelion Season
Published in Geophysical research letters (28-07-2024)“…Here we present water vapor vertical profiles observed with the ExoMars Trace Gas Orbiter/Nadir and Occultation for MArs Discovery instrument during the…”
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First Observation of the Oxygen 630 nm Emission in the Martian Dayglow
Published in Geophysical research letters (28-04-2021)“…Following the recent detection of the oxygen green line airglow on Mars, we have improved the statistical analysis of the data recorded by the NOMAD/UVIS…”
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Carbon Dioxide Retrievals From NOMAD‐SO on ESA's ExoMars Trace Gas Orbiter and Temperature Profiles Retrievals With the Hydrostatic Equilibrium Equation: 1. Description of the Method
Published in Journal of geophysical research. Planets (01-03-2023)“…The Solar Occultation (SO) channel of the Nadir and Occultation for Mars Discovery (NOMAD) instrument has been scanning the Martian atmosphere for almost…”
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Water Vapor Vertical Distribution on Mars During Perihelion Season of MY 34 and MY 35 With ExoMars‐TGO/NOMAD Observations
Published in Journal of geophysical research. Planets (01-11-2023)“…The water vapor in the Martian atmosphere plays a significant role in the planet's climate, being crucial in most of the chemical and radiative transfer…”
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An extremely high-altitude plume seen at Mars’ morning terminator
Published in Nature (London) (26-02-2015)“…Examination of amateur observations of Mars shows atmospheric plumes 200 to 250 kilometres high that are observed in the morning but not in the evening over a…”
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Carbon Dioxide Retrievals From NOMAD‐SO on ESA's ExoMars Trace Gas Orbiter and Temperature Profile Retrievals With the Hydrostatic Equilibrium Equation: 2. Temperature Variabilities in the Mesosphere at Mars Terminator
Published in Journal of geophysical research. Planets (01-03-2023)“…The Solar Occultation (SO) channel of the Nadir and Occultation for Mars Discovery (NOMAD) instrument scans the Martian atmosphere since 21 April 2018. In this…”
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Detection of green line emission in the dayside atmosphere of Mars from NOMAD-TGO observations
Published in Nature astronomy (01-11-2020)“…The oxygen emission at 557.7 nm is a ubiquitous component of the spectrum of the terrestrial polar aurora and the reason for its usual green colour 1 . It is…”
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Limb observations of CO2 and CO non-LTE emissions in the Venus atmosphere by VIRTIS/Venus Express
Published in Journal of Geophysical Research - Planets (07-03-2009)“…We report and analyze here observations of strong infrared emissions from the limb of the Venus upper atmosphere during daytime, taken by the Visible and…”
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Aeronomy of the Venus Upper Atmosphere
Published in Space science reviews (01-11-2017)“…We present aeronomical observations collected using remote sensing instruments on board Venus Express, complemented with ground-based observations and…”
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Three-dimensional Martian ionosphere model: I. The photochemical ionosphere below 180 km
Published in Journal of geophysical research. Planets (01-10-2013)“…We describe the Mars ionosphere with unprecedented detail in 3‐D, as simulated by a Mars general circulation model (the Laboratoire de Météorologie Dynamique…”
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CO2 non‐LTE limb emissions in Mars' atmosphere as observed by OMEGA/Mars Express
Published in Journal of geophysical research. Planets (01-06-2016)“…We report on daytime limb observations of Mars upper atmosphere acquired by the OMEGA instrument on board the European spacecraft Mars Express. The strong…”
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Gravity waves, cold pockets and CO2 clouds in the Martian mesosphere
Published in Geophysical research letters (01-01-2012)“…Many independent measurements have shown that extremely cold temperatures are found in the Martian mesosphere. These mesospheric “cold pockets” may result from…”
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Venus's major cloud feature as an equatorially trapped wave distorted by the wind
Published in Geophysical research letters (16-02-2015)“…The superrotation of the atmospheres of slowly rotating bodies is a long‐standing problem yet unsolved in atmospheric dynamics. On Venus, the most extreme case…”
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A ground‐to‐exosphere Martian general circulation model: 1. Seasonal, diurnal, and solar cycle variation of thermospheric temperatures
Published in Journal of Geophysical Research (01-04-2009)“…We present the extension to the thermosphere of a Martian general circulation model, the first able to self‐consistently study the whole Martian atmosphere…”
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Observation of the Mars O2 visible nightglow by the NOMAD spectrometer onboard the Trace Gas Orbiter
Published in Nature astronomy (01-01-2024)“…On Mars, atomic oxygen controls the carbon dioxide radiative cooling of the upper atmosphere and the presence of an ozone layer near the poles. To remotely…”
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Variability of the Martian thermosphere during eight Martian years as simulated by a ground-to-exosphere global circulation model
Published in Journal of geophysical research. Planets (01-11-2015)“…Using a ground‐to‐exosphere general circulation model for Mars we have simulated the variability of the dayside temperatures at the exobase during eight…”
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Polar warming in the Mars thermosphere: Seasonal variations owing to changing insolation and dust distributions
Published in Geophysical research letters (01-01-2006)“…Warming of the martian lower thermosphere (100–130 km) at north polar latitudes near the perihelion/winter solstice (Ls = 270) was recently observed. No…”
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A ground-to-exosphere Martian general circulation model: 2. Atmosphere during solstice conditions—Thermospheric polar warming
Published in Journal of Geophysical Research - Planets (01-08-2009)“…A ground‐to‐exosphere Martian general circulation model is applied to study the thermal and dynamical structure of the upper Martian atmosphere during…”
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Global Vertical Distribution of Water Vapor on Mars: Results From 3.5 Years of ExoMars‐TGO/NOMAD Science Operations
Published in Journal of geophysical research. Planets (01-09-2022)“…We present water vapor vertical distributions on Mars retrieved from 3.5 years of solar occultation measurements by Nadir and Occultation for Mars Discovery…”
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Rotational temperatures of Venus upper atmosphere as measured by SOIR on board Venus Express
Published in Planetary and space science (01-08-2015)“…SOIR is a powerful infrared spectrometer flying on board the Venus Express spacecraft since mid-2006. It sounds the Venus atmosphere above the cloud layer…”
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