Zobrazeno 1 - 10
of 54
pro vyhledávání: '"Melissa G, Trainer"'
Autor:
Daniel Y. Lo, Sushil K. Atreya, Michael H. Wong, Melissa G. Trainer, Heather B. Franz, Timothy H. McConnochie, Daniel Viúdez-Moreiras, Paul R. Mahaffy, Charles A. Malespin
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 3, p 65 (2024)
We explore and evaluate various processes that could drive the variations in the volume mixing ratio (VMR) of atmospheric O _2 observed by the quadrupole mass spectrometer (QMS) of the Sample Analysis at Mars (SAM) instrument suite on the Mars Scienc
Externí odkaz:
https://doaj.org/article/43609b8ea99f4dee84757175889c13eb
Autor:
Matthew W. Mullin, Barry Coyle, Paul R. Stysley, Melissa G. Trainer, Michael J. Hersh, Bryan L. James, Erich A. Frese, Guru Ramu, Kristen A. Washington, Joe Thomes, Eric I. Lyness, Juan Landers, Akif Ersahin, Peter D. Mule, Daniel G. Bae, Peter W. Barfknecht, Kevin A. Smith, Marc J. Matyseck, Timothy A. Petry, Amandeep Kaur, William J. Halaburda, Jackie I. Bartel, Keith A. Kienzle, Alejandro Rodriguez Perez, Jean-Marie Lauenstein, Richard F. Chuska
Publikováno v:
Solid State Lasers XXXII: Technology and Devices.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::782850ab04456c1a0697c6c05371f685
https://doi.org/10.1117/12.2650805
https://doi.org/10.1117/12.2650805
Autor:
Xiang Li, Friso van Amerom, Jacob D. Graham, Andrej Grubisic, Matthew B. Francom, Peter W. Barfknecht, William B. Brinckerhoff, Melissa G. Trainer, Marco E. Castillo
Publikováno v:
2023 IEEE Aerospace Conference.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::46bfe885cfc67454f3a9eddfc0a011f6
https://doi.org/10.1109/aero55745.2023.10115534
https://doi.org/10.1109/aero55745.2023.10115534
Autor:
Valentin Moulay, Caroline Freissinet, Malak Rizk-Bigourd, Arnaud Buch, Mayline Ancelin, Elise Couturier, Caroline Breton, Melissa G. Trainer, Cyril Szopa
Publikováno v:
Astrobiology.
Titan is a key planetary body for astrobiology, with the presence of a subsurface ocean and a dense atmosphere, in which complex chemistry is known to occur. Approximately 1-Titan-year after the Cassini-Huygens mission arrived in the saturnian system
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f118ecfed645ee4a8c1b1485242b0215
https://pubmed.ncbi.nlm.nih.gov/36577024
https://pubmed.ncbi.nlm.nih.gov/36577024
Autor:
Guillaume Avice, Rita Parai, Seth Jacobson, Jabrane Labidi, Melissa G. Trainer, Mihail P. Petkov
Publikováno v:
Space Science Reviews. 218
The composition the atmosphere of Venus results from the integration of many processes entering into play over the entire geological history of the planet. Determining the elemental abundances and isotopic ratios of noble gases (He, Ne, Ar, Kr, Xe) a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::932b56d899df5bdd5e6aabee02b70c6c
https://doi.org/10.1007/s11214-022-00929-9
https://doi.org/10.1007/s11214-022-00929-9
Autor:
D. B. Coyle, Matthew W. Mullin, Paul R. Stysley, Michael J. Hersh, Bryan L. James, Melissa G. Trainer
Publikováno v:
UV and Higher Energy Photonics: From Materials to Applications 2022.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4e201610eae3a2f4e0e27d705e3d8ad8
https://doi.org/10.1117/12.2644728
https://doi.org/10.1117/12.2644728
Autor:
Koyena Das, Thomas Gautier, Joseph Serigano, Cyril Szopa, Sarah M. Hörst, Maélie Coutelier, Sandrine Vinatier, Melissa G. Trainer
In Titan, the two major gases - dinitrogen (N2) and methane (CH4) are ionized and/or photolyzed at high altitudes by the sunlight and the energetic particles from Saturn's magnetosphere, resulting in rich atmospheric chemistry and a wide variety of c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0dcb5ed984a86f34ff46fd271a18d0e5
https://doi.org/10.5194/epsc2022-710
https://doi.org/10.5194/epsc2022-710
Autor:
David Boulesteix, Arnaud Buch, Amy J. Williams, Yuanyuan He, Caroline Freissinet, Melissa G. Trainer, Jennifer C. Stern, Cyril Szopa
Publikováno v:
SSRN Electronic Journal.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b6073f77d47f26df4c184d4356f835d3
https://doi.org/10.2139/ssrn.4223563
https://doi.org/10.2139/ssrn.4223563
Autor:
Simon Stähler, E. R. Stofan, Kevin P. Hand, C. D. Neish, William B. Brinckerhoff, Colin Wilson, Ralph D. Lorenz, Scot Rafkin, R. A. Yingst, Tetsuya Tokano, Kris Zacny, Jani Radebaugh, Christopher P. McKay, Patrick N. Peplowski, Alexander Hayes, Erich Karkoschka, Juan M. Lora, Jorge I. Nunez, Jason W. Barnes, Claire E. Newman, Melissa G. Trainer, Alice Le Gall, A. M. Parsons, Caroline Freissinet, Mark P. Panning, Lynnae C. Quick, David J. Lawrence, Carolyn M. Ernst, Cyril Szopa, Thomas P. Wagner, Jeffrey R. Johnson, Hiroaki Shiraishi, R. S. Miller, Kristin S. Sotzen, Sarah M. Hörst, Shannon MacKenzie, Elizabeth P. Turtle, Morgan L. Cable, Scott L. Murchie, Jason M. Soderblom, Angela Stickle
Publikováno v:
The Planetary Science Journal
The Planetary Science Journal, IOP Science, 2021, 2 (August), 130 (18pp). ⟨10.3847/psj/abfdcf⟩
The Planetary Science Journal, IOP Science, 2021, 2 (August), 130 (18pp). ⟨10.3847/psj/abfdcf⟩
NASA’s Dragonfly mission will send a rotorcraft lander to the surface of Titan in the mid-2030s. Dragonfly's science themes include investigation of Titan’s prebiotic chemistry, habitability, and potential chemical biosignatures from both water-b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::afe76082134333680768a54591a851bf
https://hal-insu.archives-ouvertes.fr/insu-03298915/file/Barnes_2021_Planet._Sci._J._2_130.pdf
https://hal-insu.archives-ouvertes.fr/insu-03298915/file/Barnes_2021_Planet._Sci._J._2_130.pdf
Autor:
Andrew Mastandrea, Jason W. Barnes, Elizabeth P. Turtle, Ralph D. Lorenz, Christopher P. McKay, Gary W. Hunter, Robert Osiander, Hiroshi Imanaka, Darby B. Makel, Melissa G. Trainer
Publikováno v:
Planetary and Space Science. 174:1-7
We summarize the observations and context for molecular hydrogen (H2) in Titan's atmosphere where it is the third most abundant gas. Hydrogen escapes to space but is replenished by methane photochemistry. An open question is whether there are sources
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::81ddaf0d2d2eaa40324c74cf423aaa02
https://doi.org/10.1016/j.pss.2019.05.010
https://doi.org/10.1016/j.pss.2019.05.010