No evidence of phosphine in the atmosphere of Venus from independent analyses
G. L. Villanueva, M. Cordiner, P. G. J. Irwin, I. de Pater, B. Butler, M. Gurwell, S. N. Milam, C. A. Nixon, S. H. Luszcz-Cook, C. F. Wilson, V. Kofman, G. Liuzzi, S. Faggi, T. J. Fauchez, M. Lippi, R. Cosentino, A. E. Thelen, A. Moullet, P. Hartogh, E. M. Molter, S. Charnley, G. N. Arney, A. M. Mandell, N. Biver, A. C. Vandaele, K. R. de Kleer, R. Kopparapu
Topics & Concepts
James Clerk Maxwell TelescopeVenusAtmosphere of VenusAtmosphere (unit)Radiative transferPhysicsAstrobiologySpectral lineAstrophysicsRemote sensingAtmospheric radiative transfer codesAstronomySolar atmosphereEnvironmental scienceAtmospheric modelsOptical depthPhosphineGeostationary orbitSaturnSpectral signatureCloud coverEmission spectrumSpectral analysisAtmosphere of EarthTelescopePlanetary Science and ExplorationAstro and Planetary ScienceHistory and Developments in Astronomy