DETECTION OF WIND PROFILE ON TITAN FROM ALMA OBSERVATIONS: LINE PROFILE RETRIEVALS OF HNC, HC3N, CH3CN, AND HCN
Titan, Saturn's largest natural satellite, is the only one with a substantial atmosphere in the Solar System. In situ observations of Titan's atmosphere using Huygens probe conrmed three dominated molecules: nitrogen, methane, and hydrogen; and uncovered its vertical thermal prole consi...
Saved in:
Main Author: | Badingah, Luluatul |
---|---|
Format: | Final Project |
Language: | Indonesia |
Subjects: | |
Online Access: | https://digilib.itb.ac.id/gdl/view/47896 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Institution: | Institut Teknologi Bandung |
Language: | Indonesia |
Similar Items
-
STUDY OF WIND SPEED VARIABILITY AND THE DISTRIBUTION OF ABUNDANCE OF MOLECULES ON TITAN FROM ALMA'S OBSERVATIONS
by: Badingah, Luluatul -
OVERVIEW OF NITRILE COMPOUNDS IN TITAN'S ATMOSPHERE: HCN (HYDROGEN CYANIDE), HC3N (CYANOACETYLENE), AND HC5N (CYANOBUTADIYNE)
by: Febrianti, Sindy -
SEARCH FOR PENTADIYNENITRILE COMPOUND (HC5N) IN THE ATMOSPHERE OF TITAN TROUGH OBSERVATION OF ALMA
by: Assyafa'at, Farhan -
STUDY OF TITANâS SEASONAL VARIATION IN HYDROGEN CYANIDE (HCN) EFFECTS USING ALMA DURING THE PERIOD 2012-2016
by: Az Zahra, Maulidiani -
Quantum dynamics study of H2+CN → HCN+H reaction in full dimensions
by: Zhu, W., et al.
Published: (2014)