File:Example of apparently detected PH3 spectrum on Venus after baseline-fitting with residual offset above and 5 ppb model of PH3 superimposed.png
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editDescriptionExample of apparently detected PH3 spectrum on Venus after baseline-fitting with residual offset above and 5 ppb model of PH3 superimposed.png |
English: "Figure (f5) shows the same spectrum (in red) after removal of the 4th-order polynomial plotted in Figure (f4). The overlaid curve (in black) is a model profile for 5 ppb of PH 3, scaled from our radiative transfer model, and with a spectral baseline subtracted in the same way as for the data, and the upper (grey) histogram shows the residual after subtraction of this model line."
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Date | |
Source | https://arxiv.org/abs/2011.08176 |
Author | Authors of the study: Jane S. Greaves, Anita M. S. Richards, William Bains, Paul B. Rimmer, David L. Clements, Sara Seager, Janusz J. Petkowski, Clara Sousa-Silva, Sukrit Ranjan, Helen J. Fraser |
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current | 22:50, 27 December 2020 | 7,351 × 5,046 (240 KB) | Prototyperspective (talk | contribs) | Uploaded a work by Authors of the study: Jane S. Greaves, Anita M. S. Richards, William Bains, Paul B. Rimmer, David L. Clements, Sara Seager, Janusz J. Petkowski, Clara Sousa-Silva, Sukrit Ranjan, Helen J. Fraser from https://arxiv.org/abs/2011.08176 with UploadWizard |
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Horizontal resolution | 37.8 dpc |
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Vertical resolution | 37.8 dpc |