Journal article icon

Journal article

Vertical distribution of aerosols and hazes over Jupiter's great red spot and its surroundings in 2016 from HST/WFC3 imaging

Abstract:
In this work, we have analyzed images provided by the Hubble Space Telescope's Wide Field Camera 3 (HST/WFC3) in December 2016, with a spectral coverage from the ultraviolet to the near infrared. We have obtained the spectral reflectivity of the GRS and its surroundings, with particular emphasis on selected, dynamically interesting regions. A spectral characterization of the GRS area is performed following two different procedures: (a) in terms of Altitude/Opacity and Color Indices (AOI and CI); (b) by means of automatic spectral classification. We used the NEMESIS radiative transfer suite to retrieve the main atmospheric parameters (e.g., particle vertical and size distributions, refractive indices) that are able to explain the observed spectral reflectivity. The optimal a priori model atmosphere used for the retrievals is obtained from a grid of about 12,000 different atmospheric models, and choosing the one that best fits South Tropical Zone (STrZ) spectra and its observed limb-darkening. We conclude that the spectral reflectivity of the GRS area is well reproduced with the following layout: (a) a stratospheric haze with its base near the 100 mbar level, with optical depths at 900 nm of the order of unity and particles with a size of 0.3 μm; (b) a more vertically extended tropospheric haze, with τ (900 nm) ∼10 down to 500 mbar and micron sized particles. Both haze layers show a stronger short wavelength absorption, and thus both act as chromophores. The altitude difference between clouds tops in the GRS and surrounding areas is ∼10 km.
Publication status:
Published
Peer review status:
Peer reviewed

Actions


Access Document


Publisher copy:
10.1029/2021je006996

Authors


More by this author
Role:
Author
ORCID:
0000-0002-9305-1901
More by this author
Role:
Author
ORCID:
0000-0001-7234-7634
More by this author
Role:
Author
ORCID:
0000-0003-3643-716X
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Oxford college:
St Anne's College
Role:
Author
ORCID:
0000-0002-6772-384X


Publisher:
American Geophysical Union
Journal:
Journal of Geophysical Research: Planets More from this journal
Volume:
126
Issue:
11
Article number:
e2021JE006996
Publication date:
2021-10-28
Acceptance date:
2021-10-13
DOI:
EISSN:
2169-9100
ISSN:
2169-9097


Language:
English
Keywords:
Pubs id:
1206267
Local pid:
pubs:1206267
Deposit date:
2021-11-23

Terms of use



Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP