Zobrazeno 1 - 10
of 169
pro vyhledávání: '"E Moores"'
Autor:
M. T. Lemmon, A. Vicente‐Retortillo, S. D. Guzewich, M. de la Torre Juárez, A. C. Innanen, C. L. Campbell, J. N. Maki, M. C. Malin, J. E. Moores
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 23, Pp n/a-n/a (2024)
Abstract Water and carbon dioxide each form mesospheric clouds on Mars. At such altitudes (40–100 km), clouds may remain sunlit for part of the night. We describe a previously unreported, visually spectacular season of iridescent, noctilucent cloud
Externí odkaz:
https://doaj.org/article/41c0a8ae925b45a6844fdc6d3fc716e1
Five Mars Years of Cloud Observations at Gale Crater: Opacities, Variability, and Ice Crystal Habits
Autor:
Conor W. Hayes, Jacob L. Kloos, Alex C. Innanen, Charissa L. Campbell, Haley M. Sapers, John E. Moores
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 2, p 51 (2024)
We update the record of cloud opacity observations conducted by the Mars Science Laboratory (MSL) Curiosity rover to cover the first five Mars Years (MYs) of the mission ( L _s = 160° of MY 31 to L _s = 160° of MY 36). Over the three MY period that
Externí odkaz:
https://doaj.org/article/8d09a9550528439685a1ad0d2547f849
Autor:
Alex C. Innanen, Brittney A. Cooper, Conor W. Hayes, Charissa L. Campbell, Jacob L. Kloos, Scott D. Guzewich, John E. Moores
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 3, p 72 (2024)
We examine 3 yr of phase-function observations of water-ice clouds taken during the Aphelion Cloud Belt season by the Mars Science Laboratory (MSL). We derive lower-bound single-scattering phase functions for Mars years (MYs) 34, 35, and 36, over a r
Externí odkaz:
https://doaj.org/article/e0d645bdcd6b4cfbb582565cdcb0c39d
Publikováno v:
Astrobiology. 23:280-290
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4befa0d8ac4cbd3b8f9e667471108aba
https://doi.org/10.1089/ast.2021.0184
https://doi.org/10.1089/ast.2021.0184
Publikováno v:
Advances in Space Research.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::97f47c52e5583973c5a0f94346784e63
https://doi.org/10.1016/j.asr.2023.04.004
https://doi.org/10.1016/j.asr.2023.04.004
Autor:
Nancy Borkowski, Amy Yarbrough Landry, S. Robert Hernandez, Leon E. Moores, Jeff M. Szychowski
Publikováno v:
Journal of Healthcare Management. 66:433-448
EXECUTIVE SUMMARY Little work has been done comparing the performance of hospitals with physician CEOs versus nonphysician CEOs, despite the ease of identifying this characteristic and extant leadership theories suggesting a relationship between tech
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::da80378aee5ed3fe408a1aba40c5981a
https://doi.org/10.1097/jhm-d-20-00157
https://doi.org/10.1097/jhm-d-20-00157
Publikováno v:
Astrobiology. 21:394-404
Ultraviolet (UV) irradiation on the surface of Mars is an important factor that affects the survivability of microorganisms on Mars. The possibility of martian brines made from Fe2(SO4)3, MnSO4, and MgSO4 salts providing a habitable niche on Mars via
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ca54dedf56f3480a5b3dbb112e4c859c
https://doi.org/10.1089/ast.2020.2285
https://doi.org/10.1089/ast.2020.2285
Autor:
John E. Moores, Gretchen Benedix, Shiv Meka, Daniel Marrable, Kevin Chai, Charissa L. Campbell, Christina L. Smith, Andrew L. Rohl
Publikováno v:
Acta Astronautica. 181:1-13
Currently, Martian water–ice cloud properties, such as wind direction and angular wind velocity, are determined through manual analysis of atmospheric movies taken by the Mars Science Laboratory (MSL, Curiosity). These atmospheric movies, known as
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::01afc75c67e8b5560585c2a17551ea39
https://doi.org/10.1016/j.actaastro.2020.12.041
https://doi.org/10.1016/j.actaastro.2020.12.041
Lava planets have non-global, condensible atmospheres similar to icy bodies within the solar system. Because they depend on interior dynamics, studying the atmospheres of lava planets can lead to understanding unique geological processes driven by th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7c2397605dec2a232dfa972a92dec7ef
https://ora.ox.ac.uk/objects/uuid:39ac6ac5-2d20-4f4d-bf05-38469fccbb9d
https://ora.ox.ac.uk/objects/uuid:39ac6ac5-2d20-4f4d-bf05-38469fccbb9d
