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Long-term Variations of Venus’s 365 nm Albedo Observed by Venus Express, Akatsuki, MESSENGER, and the Hubble Space Telescope
DOI: 10.3847/1538-3881/ab3120 Bibcode: 2019AJ....158..126L

Marcq, Emmanuel; Imamura, Takeshi; Titov, Dmitrij V. +16 more

An unknown absorber near the cloud-top level of Venus generates a broad absorption feature from the ultraviolet (UV) to visible, peaking around 360 nm, and therefore plays a critical role in the solar energy absorption. We present a quantitative study of the variability of the cloud albedo at 365 nm and its impact on Venus’s solar heating rates ba…

2019 The Astronomical Journal
VenusExpress eHST 36
Scattering Properties of the Venusian Clouds Observed by the UV Imager on board Akatsuki
DOI: 10.3847/1538-3881/aa78a5 Bibcode: 2017AJ....154...44L

Yamada, M.; Imamura, T.; Murakami, S. +6 more

We analyze the albedo of Venus obtained from the UV Imager on board Akatsuki. A relative global mean albedo over phase angle is used in this study, and we confirm the glory feature at 283 and 365 nm in the data acquired in 2016 May. We successfully simulate the observation using a radiative transfer model. Our results show that cloud aerosols of {…

2017 The Astronomical Journal
VenusExpress 27
High-resolution Satellite Imaging of the 2004 Transit of Venus and Asymmetries in the Cytherean Atmosphere
DOI: 10.1088/0004-6256/141/4/112 Bibcode: 2011AJ....141..112P

Schneider, Glenn; Pasachoff, Jay M.; Widemann, Thomas

This paper presents the only space-borne optical-imaging observations of the 2004 June 8 transit of Venus, the first such transit visible from Earth since AD 1882. The high-resolution, high-cadence satellite images we arranged from NASA's Transition Region and Coronal Explorer (TRACE) reveal the onset of visibility of Venus's atmosphere and give f…

2011 The Astronomical Journal
VenusExpress 26