Atmospheric Structure of Neptune in 1994, 1995, and 1996: HST Imaging at Multiple Wavelengths-Reference-Cited by-同舟云学术

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Atmospheric Structure of Neptune in 1994, 1995, and 1996: HST Imaging at Multiple Wavelengths

Published:1997-10 Issue:2 Volume:129 Page:466-481
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Hammel H.B.,Lockwood G.W.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference30 articles.

1. The Planet Uranus;Alexander,1965

2. Clouds and hazes in the atmosphere of Neptune;Baines,1995

3. Hubble Space Telescope observations of the 1990 equatorial disturbance on Saturn: Zonal winds and central meridian albedos;Barnet;Icarus,1992

4. R. F. Beebe, G. S. Orton, R. A. West, 1989, Time-variable nature of the jovian cloud properties and thermal structure: An observational perspective, Time-Variable Phenomena in the Jovian System, M. J. S. BeltonR. A. WestJ. Rahe, NASA-SP, 494

5. Wide Field and Planetary Camera 2 Instrument Handbook;Burrows,1995

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

5. EPIC simulations of Neptune’s dark spots using an active cloud microphysical model;Monthly Notices of the Royal Astronomical Society;2020-06-22

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