Zobrazeno 1 - 10
of 24
pro vyhledávání: '"J A, Rodríguez Manfredi"'
Autor:
A. Vicente‐Retortillo, G. M. Martínez, M. T. Lemmon, R. Hueso, J. R. Johnson, R. Sullivan, C. E. Newman, E. Sebastián, D. Toledo, V. Apéstigue, I. Arruego, A. Munguira, A. Sánchez‐Lavega, N. Murdoch, M. Gillier, A. Stott, L. Mora‐Sotomayor, T. Bertrand, L. K. Tamppari, M. de la Torre Juárez, J.‐A. Rodríguez‐Manfredi
Publikováno v:
Journal of Geophysical Research: Planets. 128
We identify temporal variations in surface albedo at Jezero crater using first-of-their-kind high-cadence in-situ measurements of reflected shortwave radiation during the first 350 sols of the Mars 2020 mission. Simultaneous Mars Environmental Dynami
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::392d4ea6cb19caabb71b798620b1acb8
https://doi.org/10.1029/2022je007672
https://doi.org/10.1029/2022je007672
Autor:
A. Munguira, R. Hueso, A. Sánchez‐Lavega, M. de la Torre‐Juarez, G. M. Martínez, C. E. Newman, E. Sebastian, A. Lepinette, A. Vicente‐Retortillo, B. Chide, M. T. Lemmon, T. Bertrand, R. D. Lorenz, D. Banfield, J. Gómez‐Elvira, J. Martín‐Soler, S. Navarro, J. Pla‐García, J. A. Rodríguez‐Manfredi, J. Romeral, M. D. Smith, J. Torres
Publikováno v:
Journal of Geophysical Research: Planets. 128
The Mars Environmental Dynamics Analyzer instrument on Mars 2020 has five Atmospheric Temperature Sensors at two altitudes (0.84 and 1.45 m) plus a Thermal InfraRed Sensor that measures temperatures on the surface and at ∼40 m. We analyze the measu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cd2fc8906253d7bac9ec5ad2b514f7eb
https://doi.org/10.1029/2022je007559
https://doi.org/10.1029/2022je007559
Autor:
D. Viúdez‐Moreiras, M. de la Torre, J. Gómez‐Elvira, R. D. Lorenz, V. Apéstigue, S. Guzewich, M. Mischna, R. Sullivan, K. Herkenhoff, D. Toledo, M. Lemmon, M. Smith, C. E. Newman, A. Sánchez‐Lavega, J. A. Rodríguez‐Manfredi, M. Richardson, R. Hueso, A. M. Harri, L. Tamppari, I. Arruego, J. Bell
Publikováno v:
Journal of Geophysical Research: Planets. 127
Wind speeds measured by the Mars 2020 Perseverance rover in Jezero crater were fitted as a Weibull distribution. InSight wind data acquired in Elysium Planitia were also used to contextualize observations. Jezero winds were found to be much calmer on
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d606e357016e06f5ebcca3260fdc3d5
https://doi.org/10.1029/2022je007523
https://doi.org/10.1029/2022je007523
Autor:
D. Viúdez‐Moreiras, M. Lemmon, C. E. Newman, S. Guzewich, M. Mischna, J. Gómez‐Elvira, K. Herkenhoff, A. Sánchez‐Lavega, M. de la Torre, J. A. Rodríguez‐Manfredi, R. D. Lorenz, J. Pla‐García, R. Hueso, M. Richardson, L. Tamppari, M. Smith, V. Apéstigue, D. Toledo, J. Bell
Publikováno v:
Journal of Geophysical Research: Planets. 127
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b6dd7ff5a25c1a708ef11f1430434a7e
https://doi.org/10.1029/2022je007522
https://doi.org/10.1029/2022je007522
Autor:
A. Sánchez‐Lavega, T. del Rio‐Gaztelurrutia, R. Hueso, M. de la Torre Juárez, G. M. Martínez, A.‐M. Harri, M. Genzer, M. Hieta, J. Polkko, J. A. Rodríguez‐Manfredi, M. T. Lemmon, J. Pla‐García, D. Toledo, A. Vicente‐Retortillo, D. Viúdez‐Moreiras, A. Munguira, L. K. Tamppari, C. Newman, J. Gómez‐Elvira, S. Guzewich, T. Bertrand, V. Apéstigue, I. Arruego, M. Wolff, D. Banfield, I. Jaakonaho, T. Mäkinen
Mars rover Perseverance landed on 18 February 2021 on Jezero crater. It carries a weather station that has measured, among other quantities, surface atmospheric pressure. This study covers the first 460 sols or Martian days, a period that comprises a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20e8e5dc07e2ec0b5ff4934d0e29f6d1
https://hdl.handle.net/20.500.12666/840
https://hdl.handle.net/20.500.12666/840
Autor:
G. M. Martínez, E. Sebastián, A. Vicente‐Retortillo, M. D. Smith, J. R. Johnson, E. Fischer, H. Savijärvi, D. Toledo, R. Hueso, L. Mora‐Sotomayor, H. Gillespie, A. Munguira, A. Sánchez‐Lavega, M. T. Lemmon, F. Gómez, J. Polkko, L. Mandon, V. Apéstigue, I. Arruego, M. Ramos, P. Conrad, C. E. Newman, M. de la Torre‐Juarez, F. Jordan, L. K. Tamppari, T. H. McConnochie, A.‐M. Harri, M. Genzer, M. Hieta, M.‐P. Zorzano, M. Siegler, O. Prieto, A. Molina, J. A. Rodríguez‐Manfredi
Data Availability Statement All Mars 2020 MEDA data necessary to reproduce each figure shown in this manuscript are available via the Planetary Data System (PDS) Atmospheres node (Rodriguez-Manfredi & de la Torre Juarez, 2021). An exception to this a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dd7f2f9654bad5e8764d263654daa563
https://doi.org/10.1002/essoar.10512234.1
https://doi.org/10.1002/essoar.10512234.1
Autor:
R. Hueso, C. E. Newman, T. del Río‐Gaztelurrutia, A. Munguira, A. Sánchez‐Lavega, D. Toledo, V. Apéstigue, I. Arruego, A. Vicente‐Retortillo, G. Martínez, M. Lemmon, R. Lorenz, M. Richardson, D. Viudez‐Moreiras, M. de la Torre‐Juarez, J. A. Rodríguez‐Manfredi, L. K. Tamppari, N. Murdoch, S. Navarro‐López, J. Gómez‐Elvira, M. Baker, J. Pla‐García, A. M. Harri, M. Hieta, M. Genzer, J. Polkko, I. Jaakonaho, T. Makinen, A. Stott, D. Mimoun, B. Chide, E. Sebastian, D. Banfield, A. Lepinette‐Malvite
We characterize vortex and dust devils (DDs) at Jezero from pressure and winds obtained with the Mars Environmental Dynamics Analyzer (MEDA) instrument on Mars 2020 over 415 Martian days (sols) (Ls = 6°–213°). Vortices are abundant (4.9 per sol w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e077cc691a5077bbd1c999c469e3e552
https://doi.org/10.1002/essoar.10512158.1
https://doi.org/10.1002/essoar.10512158.1
Autor:
S. Zurita‐Zurita, M. de la Torre Juárez, C. E. Newman, D. Viúdez‐Moreiras, H. T. Kahanpää, A.‐M. Harri, M. T. Lemmon, J. Pla‐García, J. A. Rodríguez‐Manfredi
Funding Information: The authors would like to thank the MCAM and Rover Environmental Monitoring Station Teams. Comments and suggestions by the M. Battalio and M. Mischna were very useful and are gratefully acknowledged. The authors also thank suppor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7005e345bf4085e3b7accf0809583a52
https://aaltodoc.aalto.fi/handle/123456789/116787
https://aaltodoc.aalto.fi/handle/123456789/116787
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
S, Maurice, B, Chide, N, Murdoch, R D, Lorenz, D, Mimoun, R C, Wiens, A, Stott, X, Jacob, T, Bertrand, F, Montmessin, N L, Lanza, C, Alvarez-Llamas, S M, Angel, M, Aung, J, Balaram, O, Beyssac, A, Cousin, G, Delory, O, Forni, T, Fouchet, O, Gasnault, H, Grip, M, Hecht, J, Hoffman, J, Laserna, J, Lasue, J, Maki, J, McClean, P-Y, Meslin, S, Le Mouélic, A, Munguira, C E, Newman, J A, Rodríguez Manfredi, J, Moros, A, Ollila, P, Pilleri, S, Schröder, M, de la Torre Juárez, T, Tzanetos, K M, Stack, K, Farley, K, Williford, P, Willis
Publikováno v:
Nature. 605(7911)
Before the Perseverance rover landing, the acoustic environment of Mars was unknown. Models predicted that: (1) atmospheric turbulence changes at centimetre scales or smaller at the point where molecular viscosity converts kinetic energy into heat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::d06fb38362884923e9cc4b6ab11468b5
https://pubmed.ncbi.nlm.nih.gov/35864234
https://pubmed.ncbi.nlm.nih.gov/35864234