Exploring Key Characteristics in Saturn's Infrared Auroral Emissions Using VLT‐CRIRES: Intensities, Ion Line‐of‐Sight Velocities, and Rotational Temperatures-Reference-Cited by-同舟云学术

Exploring Key Characteristics in Saturn's Infrared Auroral Emissions Using VLT‐CRIRES: Intensities, Ion Line‐of‐Sight Velocities, and Rotational Temperatures

Published:2019-07-03 Issue:13 Volume:46 Page:7137-7146
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Chowdhury M. N.¹^ORCID,Stallard T. S.¹^ORCID,Melin H.¹^ORCID,Johnson R. E.²^ORCID

Affiliation:

1. Department of Physics and Astronomy University of Leicester Leicester UK

2. Hotelli Korpikartano Inari Finland

Funder

Central Laser Facility, Science and Technology Facilities Council

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019GL083250

Reference43 articles.

1. Statistical Planetary Period Oscillation Signatures in Saturn's UV Auroral Intensity

2. Location of Saturn's northern infrared aurora determined from Cassini VIMS images

3. Auroral emissions of the giant planets

4. Origin of Saturn's aurora: Simultaneous observations by Cassini and the Hubble Space Telescope

5. Response of Jupiter's and Saturn's auroral activity to the solar wind

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