词条 | Elivagar Flumina |
释义 |
The Elivagar Flumina is named after the Élivágar, a group of poisonous ice rivers in Norse mythology.[6] References1. ^{{cite web|url=https://www.researchgate.net/figure/262986396_fig1_Fig-1-Cassini-RADAR-image-of-Menrva-and-Elivagar-Flumina-taken-during-the-T3-fly-by|title=Fig. 1. Cassini RADAR image of Menrva and Elivagar Flumina taken during the T3 fly-by, showing the channels near Menrva and the catchment basin (highlighted in blue).|publisher=Researchgate|access-date=18 June 2016}} {{Titan}}{{crater-stub}}2. ^1 {{cite journal|title=Geomorphologic mapping of the Menrva region of Titan using Cassini RADAR data|year=2011|first=David|last=Williams|first2=Jani|last2=Radebaugh|first3=Rosaly|last3=Lopes|first4=Ellen|last4=Stofan|bibcode=2011Icar..212..744W|doi=10.1016/j.icarus.2011.01.014}} 3. ^{{cite web|url=http://www.lpi.usra.edu/meetings/lpsc2013/pdf/2641.pdf|title=ALLUVIAL FANS ON TITAN REVEAL MATERIALS, PROCESSES AND REGIONAL CONDITIONS|access-date=18 June 2016|year=2013}} 4. ^Ingo Müller-Wodarg; Caitlin A. Griffith; Emmanuel Lellouch, 2014. Titan: Interior, Surface, Atmosphere, and Space Environment. Cambridge University Press. p. 69. {{ISBN|978-0-521-19992-6}}. 5. ^Williams, David A., et al. "Geomorphologic mapping of the Menrva region of Titan using Cassini RADAR data." Icarus212.2 (2011): 744-750. 6. ^Robert Brown; Jean Pierre Lebreton; Hunter Waite, 2009. Titan from Cassini-Huygens. Springer Science & Business Media. p. 508. {{ISBN|978-1-4020-9215-2}}. 1 : Surface features of Titan (moon) |
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