This work reviews possible signatures and potential detectability of present-day volcanically
emitted material in the atmosphere of Venus. We first discuss the expected composition of …

Abstract The Radio Occultation Science Experiment (ROSE) is part of the scientific payload
of the Mars Atmosphere Volatile EvolutioN (MAVEN) spacecraft. Here we motivate the …

The atmosphere of Venus remains mysterious, with many outstanding chemical connundra.
These include the unexpected presence of∼ 10 ppm O2 in the cloud layers, an unknown …

Venus is an exceptional natural experiment to test our understanding of atmospheric sulfur
chemistry. Previous modeling efforts have focused on understanding either the middle or …

We show that solar irradiances calculated across Venus' clouds support the potential for
Earth-like phototrophy and that treatment of Venus' aerosols containing neutralized sulfuric …

The search for life beyond Earth has focused on Mars and the icy moons Europa and
Enceladus, all of which are considered a safe haven for life due to evidence of current or …

We present distributions of the zonal-mean temperature and static stability in the Venusian
atmosphere obtained from Venus Express and Akatsuki radio occultation profiles …

Although Venus is a terrestrial planet similar to Earth, its atmospheric circulation is much
different and poorly characterized. Winds at the cloud top have been measured …

Power fluctuations are observed on radio signals propagating through the Venus
atmosphere. These scintillations, due to fluctuations in refractive index, are particularly …

From the discovery that Venus has an atmosphere during the 1761 transit by M. Lomonosov
to the current exploration of the planet by the Akatsuki orbiter, we continue to learn about the …