Re-analysis of the 267 GHz ALMA observations of Venus
I. A. G. Snellen; L. Guzman-Ramirez; M. R. Hogerheijde; A. P. S. Hygate; F. F. S. van der Tak · 2020 · Astronomy & Astrophysics
WASTE classifies this as Negative / Null Result Report · AI classification, approximate
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Abstract (excerpt)
Context. ALMA observations of Venus at 267 GHz that show the apparent presence of phosphine (PH 3 ) in its atmosphere have been presented in the literature. Phosphine currently has no evident production routes on the planet’s surface or in…
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Metadata source: Crossref · DOI 10.1051/0004-6361/202039717