Evolution of Saturn’s north polar color and cloud structure between 2012 and 2017 inferred from Cassini VIMS and ISS observations-Reference-Cited by-同舟云学术

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Evolution of Saturn’s north polar color and cloud structure between 2012 and 2017 inferred from Cassini VIMS and ISS observations

Published:2021-07 Issue: Volume:362 Page:114409
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Sromovsky L.A.^ORCID,Baines K.H.,Fry P.M.

Funder

NASA

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference85 articles.

1. Saturn’s Atmospheric Helium Abundance from Cassini Composite Infrared Spectrometer Data;Achterberg;Plan. Sci. J.,2020

2. Thermal Emission From Saturn’s Polar Cyclones;Achterberg;Geophys. Res. Lett.,2018

3. Ancillary data services of NASA’s Navigation and Ancillary Information Facility;Acton;Planet. Space Sci.,1996

4. The de-striping of the VIMS-V images and the observations of HCN limb emission in the Titan atmosphere at 3μm;Adriani;Mem. Soc. Astron. Ital. Suppl.,2007

5. Modernization of the Integrated Software for Imagers and Spectrometers;Anderson,2004

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1. Relaxed magnetic structures in the Saturn's ring;Physics of Plasmas;2024-06-01

2. Saturn's Atmosphere in Northern Summer Revealed by JWST/MIRI;Journal of Geophysical Research: Planets;2023-09

3. Mid-Infrared Observations of the Giant Planets;Remote Sensing;2023-03-28

4. Giant Planet Atmospheres: Dynamics and Variability from UV to Near-IR Hubble and Adaptive Optics Imaging;Remote Sensing;2022-03-21

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