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注意:仅列出部分参考文献,下载原文获取全部文献信息。Only extraordinary volcanism can explain the presence of parts per billion phosphine on Venus
William Bains et al.
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Low levels of sulphur dioxide contamination of Venusian phosphine spectra
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Phosphine gas in the cloud decks of Venus
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Phosphine on Venus Cannot Be Explained by Conventional Processes
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Volcanically extruded phosphides as an abiotic source of Venusian phosphine
N. Truong et al.
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Reply to: No evidence of phosphine in the atmosphere of Venus from independent analyses
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No evidence of phosphine in the atmosphere of Venus from independent analyses
G. L. Villanueva et al.
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Claimed Detection of PH3 in the Clouds of Venus Is Consistent with Mesospheric SO2
Andrew P. Lincowski et al.
ASTROPHYSICAL JOURNAL LETTERS (2021)
Complications in the ALMA Detection of Phosphine at Venus
Alex B. Akins et al.
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The statistical reliability of 267-GHz JCMT observations of Venus: no significant evidence for phosphine absorption
M. A. Thompson
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Phosphine as a Biosignature Gas in Exoplanet Atmospheres
Clara Sousa-Silva et al.
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A stringent upper limit of the PH3 abundance at the cloud top of Venus
T. Encrenaz et al.
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Re-analysis of the 267 GHz ALMA observations of Venus: No statistically significant detection of phosphine
I. A. G. Snellen et al.
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Phosphine in Venus' atmosphere: Detection attempts and upper limits above the cloud top assessed from the SOIR/VEx spectra
L. Trompet et al.
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Planetary Spectrum Generator: An accurate online radiative transfer suite for atmospheres, comets, small bodies and exoplanets
G. L. Villanueva et al.
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The upGREAT Dual Frequency Heterodyne Arrays for SOFIA
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Transmission spectrum of Venus as a transiting exoplanet
D. Ehrenreich et al.
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High-resolution wide-band fast Fourier transform spectrometers
B. Klein et al.
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Upper limits for undetected trace species in the stratosphere of Titan
Conor A. Nixon et al.
FARADAY DISCUSSIONS (2010)
Structure of the Venusian atmosphere from surface up to 100 km
L. V. Zasova et al.
COSMIC RESEARCH (2006)