Alluvial Fan Morphology, distribution and formation on Titan-Reference-Cited by-同舟云学术

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Alluvial Fan Morphology, distribution and formation on Titan

Published:2016-05 Issue: Volume:270 Page:238-247
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Birch S.P.D.,Hayes A.G.,Howard A.D.,Moore J.M.,Radebaugh J.

Funder

NASA Cassini Data Analysis Program

NASA Earth and Space Science Fellowship Program

Cassini-Huygens mission

ESA

ASI

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference72 articles.

1. Near-infrared spectral mapping of Titan’s mountains and channels;Barnes;J. Geophys. Res. Planets,2007

2. Spectroscopy, morphometry, and photoclinometry of Titan’s dunefields from Cassini/VIMS;Barnes;Icarus,2008

3. Organic sedimentary deposits in Titan’s dry lakebeds: Probable evaporite;Barnes;Icarus,2011

4. Alluvial fan processes and forms;Blair,1994

5. Processes and Forms of Alluvial Fans;Blair,2009

Cited by 41 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Methane storm characteristics and evolution in simulations of Titan’s hydroclimate;Icarus;2025-01

2. Moisture transport and the methane cycle of Titan’s lower atmosphere;Icarus;2024-11

3. Detailed chemical composition analysis of the Soi crater region on Titan;Icarus;2024-10

4. The history and processes of Titan's equator from the geospatial-topology of spectrally distinct units;Icarus;2024-07

5. Signatures of wave erosion in Titan’s coasts;Science Advances;2024-06-21

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