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View article: New insights into the mesosphere of Venus from MERTIS measurements during the two BepiColombo flybys
New insights into the mesosphere of Venus from MERTIS measurements during the two BepiColombo flybys Open
Analyses of measurements made by MERTIS1 (MErcury Radiometer and Thermal Infrared Spectrometer) during the BepiColombo mission's close flyby 2 of Venus (FB2) have already demonstrated the instrument's capacity to explore the planet's mesos…
View article: Spectroscopic studies of Venusian atmosphere by BepiColombo's MERTIS instrument during the two Venus flybys
Spectroscopic studies of Venusian atmosphere by BepiColombo's MERTIS instrument during the two Venus flybys Open
<p><strong>Introduction</strong></p> <p>The MErcury Radiometer and Thermal Infrared Spectrometer (MERTIS) onboard BepiColombo is designed to study and map Mercury surface mineralogy and temperatures. It combin…
View article: Martian Atmospheric Thermal Structure and Dust Distribution During the MY 34 Global Dust Storm From ACS TIRVIM Nadir Observations
Martian Atmospheric Thermal Structure and Dust Distribution During the MY 34 Global Dust Storm From ACS TIRVIM Nadir Observations Open
The Thermal InfraRed channel in honor of professor Vassili Ivanovich Moroz (TIRVIM) of the Atmospheric Chemistry Suite onboard ExoMars Trace Gas Orbiter has continuously monitored the Martian atmosphere from 13 March 2018 until 2 December …
View article: Martian surface-atmosphere properties obtained with ExoMars infrared instrument TIRVIM and HP3 on InSight
Martian surface-atmosphere properties obtained with ExoMars infrared instrument TIRVIM and HP3 on InSight Open
ESA’s ExoMars program comprises two missions including the Trace Gas Orbiter (TGO), launched in 2016, and a rover and surface platform, to be launched in 2022. The main scientific objectives of the program are to investigate the Martian en…
View article: Sensitivity of net thermal flux to the abundance of trace gases in the lower atmosphere of Venus
Sensitivity of net thermal flux to the abundance of trace gases in the lower atmosphere of Venus Open
We calculated the net thermal flux in the atmosphere of Venus from the surface to 100 km altitude. Our atmospheric model was carefully constructed especially for altitudes below the clouds (<48 km), using recent CO 2 absorption data. It in…
View article: VEM on VERITAS - Retrieval of global infrared surface emissivity maps of Venus and expectable retrieval uncertainties
VEM on VERITAS - Retrieval of global infrared surface emissivity maps of Venus and expectable retrieval uncertainties Open
Even though Venus is in many respects the most Earth-like planet we know today, its surface composition and
\ngeology are not well understood yet. The major obstacle is the extremely dense, hot, and opaque atmosphere
\nthat complicates bot…
View article: Retrieval and study of near-infrared surface emissivity maps of Themis Regio on Venus with VIRTIS-M (Venus Express)
Retrieval and study of near-infrared surface emissivity maps of Themis Regio on Venus with VIRTIS-M (Venus Express) Open
Surface emissivity maps of Themis Regio on Venus
\nhave been derived from nightside radiance spectra
\nacquired by VIRTIS-M-R aboard Venus Express to
\nexplore the region’s geology. The emissivity retrieval
\nbases on a new approach combin…
View article: Analyses of spectroscopic and atmospheric parameter influences on radiative heating and cooling rates in the middle and lower atmosphere of Venus
Analyses of spectroscopic and atmospheric parameter influences on radiative heating and cooling rates in the middle and lower atmosphere of Venus Open
Radiative fluxes and temperature change rates in the
\nmiddle and lower atmosphere of Venus (0-100 km)
\nare calculated over the broad spectral range 0.125-
\n1000 μm applying a radiative transfer model.
\nResponses of these quantities to …