Search Publications

One-dimensional Microphysics Model of Venusian Clouds from 40 to 100 km: Impact of the Middle-atmosphere Eddy Transport and SOIR Temperature Profile on the Cloud Structure
DOI: 10.3847/PSJ/ad25f3 Bibcode: 2024PSJ.....5...57K

Vandaele, Ann Carine; Terada, Naoki; Imamura, Takeshi +4 more

We conducted a simulation of H2SO4 vapor, H2O vapor, and H2SO4–H2O liquid aerosols from 40 to 100 km, using a 1D Venus cloud microphysics model based on the one detailed in Imamura & Hashimoto. The cloud distribution obtained is in good agreement with in situ observations by Pio…

2024 The Planetary Science Journal
VenusExpress 2
The Influence of Cloud Condensation Nucleus Coagulation on the Venus Cloud Structure
DOI: 10.3847/PSJ/acbdf8 Bibcode: 2023PSJ.....4...50M

Barth, Erika L.; McGouldrick, Kevin

We present the Venus version of PlanetCARMA and demonstrate the significance of coagulation properties on the structure of the Venus cloud system. The composition of the smallest mode of particles in the Venus atmosphere, which likely serve as cloud condensation nuclei (CCN), is unknown. Here we demonstrate that a change in the ability of CCN to g…

2023 The Planetary Science Journal
VenusExpress 3
Local-time Dependence of Chemical Species in the Venusian Mesosphere
DOI: 10.3847/PSJ/ac3bd3 Bibcode: 2022PSJ.....3....3S

Shao, Wencheng D.; Zhang, Xi; Mendonça, João +1 more

Observed chemical species in the Venusian mesosphere show local-time variabilities. SO2 at the cloud top exhibits two local maxima over local time, H2O at the cloud top is uniformly distributed, and CO in the upper atmosphere shows a statistical difference between the two terminators. In this study, we investigated these loca…

2022 The Planetary Science Journal
VenusExpress 4
Idunn Mons: Evidence for Ongoing Volcano-tectonic Activity and Atmospheric Implications on Venus
DOI: 10.3847/PSJ/ac2258 Bibcode: 2021PSJ.....2..215D

D'Incecco, P.; Filiberto, J.; López, I. +2 more

In 2010 the ESA Venus Express Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) instrument first observed 1 µm emissivity anomalies over the top and eastern flank of Idunn Mons (46° S; 146° W), a 200 km wide volcano located in Imdr Regio, a volcano-dominated large volcanic rise of Venus. The anomalies suggest the presence of chemica…

2021 The Planetary Science Journal
VenusExpress 17
Using VIRTIS on Venus Express to Constrain the Properties of the Giant Dark Cloud Observed in Images of Venus by IR2 on Akatsuki
DOI: 10.3847/PSJ/ac0e39 Bibcode: 2021PSJ.....2..153M

Tsang, Constantine C. C.; Barstow, Joanna K.; McGouldrick, Kevin +1 more

A cloud opacity contrast feature that has been called a "long-lived sharp disruption" has been seen in the atmosphere of Venus in the near-infrared using Akatsuki's IR2 camera, most clearly at equatorial latitudes. This feature was found to have a consistent planet-circling period of 4.9 days, and subsequent searches of past imagery revealed that …

2021 The Planetary Science Journal
VenusExpress 8
Experimental Investigation of Oxidation of Pyroxene and Basalt: Implications for Spectroscopic Analyses of the Surface of Venus and the Ages of Lava Flows
DOI: 10.3847/PSJ/ab8faf Bibcode: 2020PSJ.....1...21C

Filiberto, J.; Cutler, K. S.; Treiman, A. H. +1 more

Alteration of basalt on the surface of Venus should be dominated by nanophase hematite and sulfate coatings, but the timescale of oxidation and how that affects spectroscopic measurements has not been extensively studied. The oxidation rate and the effect on reflectance spectroscopy are needed to constrain the age of lava flows with high emissivit…

2020 The Planetary Science Journal
VenusExpress 20