Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Constantinou, Tereza"'
Autor:
Cesario, Lorenzo, Lichtenberg, Tim, Alei, Eleonora, Carrión-González, Óscar, Dannert, Felix A., Defrère, Denis, Ertel, Steve, Fortier, Andrea, Muñoz, A. García, Glauser, Adrian M., Hansen, Jonah T., Helled, Ravit, Huber, Philipp A., Ireland, Michael J., Kammerer, Jens, Laugier, Romain, Lillo-Box, Jorge, Menti, Franziska, Meyer, Michael R., Noack, Lena, Quanz, Sascha P., Quirrenbach, Andreas, Rugheimer, Sarah, van der Tak, Floris, Wang, Haiyang S., Anger, Marius, Balsalobre-Ruza, Olga, Bhattarai, Surendra, Braam, Marrick, Castro-González, Amadeo, Cockell, Charles S., Constantinou, Tereza, Cugno, Gabriele, Davoult, Jeanne, Güdel, Manuel, Hernitschek, Nina, Hinkley, Sasha, Itoh, Satoshi, Janson, Markus, Johansen, Anders, Jones, Hugh R. A., Kane, Stephen R., van Kempen, Tim A., Kislyakova, Kristina G., Korth, Judith, Kovacevic, Andjelka B., Kraus, Stefan, Kuiper, Rolf, Mathew, Joice, Matsuo, Taro, Miguel, Yamila, Min, Michiel, Navarro, Ramon, Ramirez, Ramses M., Rauer, Heike, Ricketti, Berke Vow, Romagnolo, Amedeo, Schlecker, Martin, Sneed, Evan L., Squicciarini, Vito, Stassun, Keivan G., Tamura, Motohide, Viudez-Moreiras, Daniel, Wordsworth, Robin D., Collaboration, the LIFE
The increased brightness temperature of young rocky protoplanets during their magma ocean epoch makes them potentially amenable to atmospheric characterization to distances from the solar system far greater than thermally equilibrated terrestrial exo
Externí odkaz:
http://arxiv.org/abs/2410.13457
Compared to the diversity seen in exoplanets, Venus is a veritable astrophysical twin of the Earth, however its global cloud layer truncates features in transmission spectroscopy, masking its non-Earth-like nature. Observational indicators that can d
Externí odkaz:
http://arxiv.org/abs/2108.05778
Autor:
Rimmer, Paul B., Jordan, Sean, Constantinou, Tereza, Woitke, Peter, Shorttle, Oliver, Paschodimas, Alessia, Hobbs, Richard
The depletion of SO$_2$ and H$_2$O in and above the clouds of Venus (45 -- 65 km) cannot be explained by known gas-phase chemistry and the observed composition of the atmosphere. We apply a full-atmosphere model of Venus to investigate three potentia
Externí odkaz:
http://arxiv.org/abs/2101.08582
Autor:
Kammerer, Jens, Sallum, Stephanie, Sanchez-Bermudez, Joel, Glauser, Adrian M., Quanz, Sascha P., Hansen, Jonah, Dannert, Felix, Ireland, Michael, Linz, Hendrik, Absil, Olivier, Alei, Eleonora, Angerhausen, Daniel, Birbacher, Thomas, Defrère, Denis, Fortier, Andrea, Huber, Philipp A., Kammerer, Jens, Laugier, Romain, Lichtenberg, Tim, Noack, Lena, Ranganathan, Mohanakrishna, Rugheimer, Sarah, Airapetian, Vladimir, Alibert, Yann, Amado, Pedro J., Anger, Marius, Anugu, Narsireddy, Aragon, Max, Armstrong, David J., Balbi, Amedeo, Balsalobre-Ruza, Olga, Banik, Deepayan, Beck, Mathias, Bhattarai, Surendra, Biren, Jonas, Bottoni, Jacopo, Braam, Marrick, Brandeker, Alexis, Buchhave, Lars A., Caballero, José A., Cabrera, Juan, Carone, Ludmila, Carrión-González, Óscar, Castro-González, Amadeo, Chan, Kenny, Coelho, Ligia F., Constantinou, Tereza, Cowan, Nicolas, Danchi, William, Dandumont, Colin, Davoult, Jeanne, Dawn, Arjun, de Vera, Jean-Pierre P., de Visser, Pieter J., Dorn, Caroline, Duque Lara, Juan A., Elowitz, Mark, Ertel, Steve, Fang, Yuedong, Felix, Simon, Fortney, Jonathan, Fridlund, Malcolm, García Muñoz, Antonio, Gillmann, Cedric, Golabek, Gregor, Grenfell, John Lee, Guidi, Greta, Guilera, Octavio, Hagelberg, Janis, Hansen, Janina, Haqq-Misra, Jacob, Hara, Nathan, Helled, Ravit, Herbst, Konstantin, Hernitschek, Nina, Hinkley, Sasha, Ito, Takahiro, Itoh, Satoshi, Ivanovski, Stavro, Janson, Markus, Johansen, Anders, Jones, Hugh, Kane, Stephen, Kitzmann, Daniel, Kovacevic, Andjelka B., Kraus, Stefan, Krause, Oliver, Kruijssen, J. M. Diederik, Kuiper, Rolf, Kuriakose, Alen, Labadie, Lucas, Lacour, Sylvestre, Lanza, Antonino F., Leedjärv, Laurits, Lendl, Monika, Leung, Michaela, Lillo-Box, Jorge, Loicq, Jérôme, Luque, Rafael, Mahadevan, Suvrath, Majumdar, Liton, Malbet, Fabien, Mallia, Franco, Mathew, Joice, Matsuo, Taro, Matthews, Elisabeth, Meadows, Victoria, Mennesson, Bertrand, Meyer, Michael R., Molaverdikhani, Karan, Mollière, Paul, Monnier, John, Navarro, Ramon, Nsamba, Benard, Oguri, Kenshiro, Oza, Apurva, Palle, Enric, Persson, Carina, Pitman, Joe, Plávalová, Eva, Pozuelos, Francisco J., Quirrenbach, Andreas, Ramirez, Ramses, Reiners, Ansgar, Ribas, Ignasi, Rice, Malena, Ricketti, Berke Vow, Roelfsema, Peter, Romagnolo, Amedeo, Ronco, María Paula, Schlecker, Martin, Schonhut-Stasik, Jessica, Schwieterman, Edward, Sefilian, Antranik A., Serabyn, Eugene, Shahi, Chinmay, Sharma, Siddhant, Silva, Laura, Singh, Swapnil, Sneed, Evan L., Spencer, Locke, Squicciarini, Vito, Staguhn, Johannes, Stapelfeldt, Karl, Stassun, Keivan, Tamura, Motohide, Taysum, Benjamin, van der Tak, Floris, van Kempen, Tim A., Vasisht, Gautam, Wang, Haiyang S., Wordsworth, Robin, Wyatt, Mark
Publikováno v:
Proceedings of SPIE; August 2024, Vol. 13095 Issue: 1 p130951D-130951D-21, 12964171p
Autor:
Rimmer, Paul B., Jordan, Sean, Constantinou, Tereza, Woitke, Peter, Shorttle, Oliver, Hobbs, Richard, Paschodimas, Alessia
The depletion of SO2 and H2O in and above the clouds of Venus (45–65 km) cannot be explained by known gas-phase chemistry and the observed composition of the atmosphere. We apply a full-atmosphere model of Venus to investigate three potential expla
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e64864054d32cddac4f1717d021564c6