Journal articles
Long-term Variations of Venus’s 365 nm Albedo Observed by Venus Express , Akatsuki , MESSENGER , and the Hubble Space Telescope
Yeon Lee
1, 2
Kandis-Lea Jessup
3
Santiago Perez-Hoyos
4
Dmitrij Titov
5
Sébastien Lebonnois
6
Javier Peralta
7
Takeshi Horinouchi
8
Takeshi Imamura
1
Sanjay Limaye
9
Emmanuel Marcq
10
Masahiro Takagi
11
Atsushi Yamazaki
7, 12
Manabu Yamada
13
Shigeto Watanabe
14
Shin-Ya Murakami
7
Kazunori Ogohara
15
William Mcclintock
16
Gregory Holsclaw
16
Anthony Roman
17
Yeon Joo Lee 1, 2
Mail :
Author
Kandis-Lea Jessup 3
Mail :
Author
Santiago Perez-Hoyos 4
Author
Dmitrij V. Titov 5
Author
Sébastien Lebonnois 6
Mail :
Author IdHAL : sebastien-lebonnois ORCID : https://orcid.org/0000-0002-2390-8164
Javier Peralta 7
Mail :
Author
Takeshi Horinouchi 8
Author
Takeshi Imamura 1
Author
Sanjay Limaye 9
Author
Emmanuel Marcq 10
Mail :
Author IdHAL : emmanuel-marcq ORCID : https://orcid.org/0000-0002-1924-641X
Masahiro Takagi 11
Author
Atsushi Yamazaki 7, 12
Mail :
Author
Manabu Yamada 13
Author
Shigeto Watanabe 14
Author
Shin-Ya Murakami 7
Author
Kazunori Ogohara 15
Author
1
Graduate School of Frontier Sciences [Kashiwa] (5–1–5 Kashiwanoha, 277–8563 Kashiwa, Chiba - Japan)
- The University of Tokyo (7 Chome-3-1 Hongo, Bunkyo, Tokyo 113-8654, Japon - Japan)
2
ZAA - Zentrum für Astronomie und Astrophysik [Berlin] (Hardenbergstraße 36, D-10623 Berlin - Germany)
- TUB - Technische Universität Berlin (Straße des 17. Juni 135 10623 Berlin - Germany)
3
SwRI - Southwest Research Institute [Boulder] (1050 Walnut St, Suite 300,
Boulder, CO 80302 - United States)
4
Departamento de Fisica Aplicada [Bilbao] (Spain)
- UPV/EHU - Universidad del Pais Vasco / Euskal Herriko Unibertsitatea [Espagne] (Barrio Sarriena s/n, 48940 Leioa, Bizkaia Campus d'Álava : Vice-Rectorado, San Antonio 41, 01005 Vitoria ; campus de Biscaye et services centraux : Apdo 1397, 48080 Bilbao ; campus de Guipúzcoa : Vice-Rectorado, Fuenterrabia 13-1° , 20006 San Sebastián - Spain)
5
ESTEC - European Space Research and Technology Centre (Keplerlaan 1, 2201 Noordwijk - Netherlands)
- ESA - European Space Agency (France)
6
LMD - Laboratoire de Météorologie Dynamique (UMR 8539) (LMD ENS 24 Rue Lhomond 75231 Paris Cedex 05 - France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- X - École polytechnique (École polytechnique, 91128 Palaiseau Cedex - France)
- ENPC - École des Ponts ParisTech (École des Ponts ParisTech 6-8 avenue Blaise-Pascal Cité Descartes 77455 Champs-sur-Marne Marne-la-Vallée cedex 2 - France)
- SU - Sorbonne Université (21 rue de l’École de médecine - 75006 Paris - France)
- CNRS - Centre National de la Recherche Scientifique : UMR8539 (France)
- Département des Géosciences - ENS Paris (24 rue Lhomond, 75005 Paris, France - France)
- ENS Paris - École normale supérieure - Paris (45, Rue d'Ulm - 75230 Paris cedex 05 - France)
7
ISAS - Institute of Space and Astronautical Science (Sagamihara City, Kanagawa Prefecture 252-5210 - Japan)
8
Faculty of Environmental Earth Science [Sapporo] (Hokkaido University , N10W5 Sapporo , Hokkaido 060-0810 - Japan)
- Hokkaido University [Sapporo, Japan] (5 Chome Kita 8 Jōnishi, Kita Ward, Sapporo, Hokkaido Prefecture 060-0808, Japon - Japan)
9
SSEC - Space Science and Engineering Center [Madison] (1225 W. Dayton Street, Madison, WI 53706 - United States)
- University of Wisconsin-Madison (Madison, WI 53706 - United States)
10
IMPEC - LATMOS (France)
- LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales (11 boulevard d'Alembert
Quartier des Garennes
78280 - Guyancourt - France)
- INSU - CNRS - Institut national des sciences de l'Univers : UMR8190 (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR8190 (France)
- UVSQ - Université de Versailles Saint-Quentin-en-Yvelines : UMR8190 (55 avenue de Paris - 78035 Versailles cedex - France)
- SU - Sorbonne Université : UMR8190 (21 rue de l’École de médecine - 75006 Paris - France)
11
Kyoto Sangyo University (Motoyama, Kamigamo, Kita-ku Kyoto-City 603-8555 Japan - Japan)
12
Department of Earth and Planetary Science [Tokyo] (Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 - Japan)
- The University of Tokyo (7 Chome-3-1 Hongo, Bunkyo, Tokyo 113-8654, Japon - Japan)
13
PERC - Planetary Exploration Research Center [Chiba] (2-17-1 Tsudanuma, Narashino, 275-0016 Chiba, Japan - Japan)
- CIT - Chiba Institute of Technology (2-17-1 Tsudanuma Narashino-shi Chiba 275-0016 Japan - Japan)
14
Hokkaido Information University (Hokkaido 069-0832, Japon - Japan)
15
University of Shiga Prefecture (2500, Hassaka-cho, Hikone-City, Shiga 522-8533 Japan - Japan)
16
LASP - Laboratory for Atmospheric and Space Physics [Boulder] (1234 Innovation Drive, Boulder, CO 80303-7814 - United States)
- University of Colorado [Boulder] (Boulder, Colorado 80309 - United States)
17
STSci - Space Telescope Science Institute (3700 San Martin Drive, Baltimore, MD 21218, USA - United States)
Abstract : 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 based on an analysis of Venus Express and Akatsuki UV images and Hubble Space Telescope and MESSENGER UV spectral data; in this analysis, the calibration correction factor of the UV images of Venus Express (Venus Monitoring Camera) is updated relative to the Hubble and MESSENGER albedo measurements. Our results indicate that the 365 nm albedo varied by a factor of 2 from 2006 to 2017 over the entire planet, producing a 25%-40% change in the low-latitude solar heating rate according to our radiative transfer calculations. Thus, the cloud-top level atmosphere should have experienced considerable solar heating variations over this period. Our global circulation model calculations show that this variable solar heating rate may explain the observed variations of zonal wind from 2006 to 2017. Overlaps in the timescale of the long-term UV albedo and the solar activity variations make it plausible that solar extreme UV intensity and cosmic-ray variations influenced the observed albedo trends. The albedo variations might also be linked with temporal variations of the upper cloud SO 2 gas abundance, which affects the H2SO4-H2O aerosol formation.
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Journal articles
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https://hal-insu.archives-ouvertes.fr/insu-02283341
Contributor : Catherine Cardon <>
Submitted on : Tuesday, September 10, 2019 - 4:54:38 PM
Last modification on : Tuesday, June 16, 2020 - 3:44:02 PM
Document(s) archivé(s) le : Saturday, February 8, 2020 - 12:08:23 AM
Contributor : Catherine Cardon <>
Submitted on : Tuesday, September 10, 2019 - 4:54:38 PM
Last modification on : Tuesday, June 16, 2020 - 3:44:02 PM
Document(s) archivé(s) le : Saturday, February 8, 2020 - 12:08:23 AM
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Lee_2019_AJ_158_126.pdf
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Identifiers
- HAL Id : insu-02283341, version 1
- DOI : 10.3847/1538-3881/ab3120
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INSU | LATMOS | X-LMD | UVSQ | CNRS | X | ENPC | LMD | X-DEP-MECA | ENS-PARIS | SORBONNE-UNIVERSITE | SU-SCIENCES | PSL | ENPC-LMD | UNIV-PARIS-SACLAY | PARISTECH
Citation
Yeon Lee, Kandis-Lea Jessup, Santiago Perez-Hoyos, Dmitrij Titov, Sébastien Lebonnois, et al.. Long-term Variations of Venus’s 365 nm Albedo Observed by Venus Express , Akatsuki , MESSENGER , and the Hubble Space Telescope. Astronomical Journal, American Astronomical Society, 2019, 158 (3), pp.126. ⟨10.3847/1538-3881/ab3120⟩. ⟨insu-02283341⟩
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