New determination of the HCN profile in the stratosphere of Neptune from millimeter-wave spectroscopy
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201323300/pdf
Reference48 articles.
1. The Heinrich Hertz Telescope and the Submillimeter Telescope Observatory
2. The Abundances of Methane and Ortho/Para Hydrogen on Uranus and Neptune: Implications of New Laboratory 4-0 H2 Quadrupole Line Parameters
3. Hydrocarbons in Neptune's stratosphere from Voyager infrared observations
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1. Collisional excitation of HNC by He found to be stronger than for structural isomer HCN in experiments at the low temperatures of interstellar space;Nature Chemistry;2022-05-05
2. Collisional excitation of HNC by He found to be stronger than for structural isomer HCN in experiments at the low temperatures of interstellar space;NAT CHEM;2022
3. Uranus’s and Neptune’s Stratospheric Water Abundance and Vertical Profile from Herschel-HIFI*;The Planetary Science Journal;2022-04-01
4. Atmospheric chemistry on Uranus and Neptune;Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences;2020-11-09
5. A Belt-like Distribution of Gaseous Hydrogen Cyanide on Neptune’s Equatorial Stratosphere Detected by ALMA;The Astrophysical Journal;2020-10-23
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