Zobrazeno 1 - 10
of 13
pro vyhledávání: '"Vilmos Steinmann"'
Publikováno v:
Remote Sensing, Vol 16, Iss 19, p 3649 (2024)
Identifying surface sites with significant astrobiological potential on Mars requires a comprehensive understanding of past geological processes and conditions there, including the shallow subsurface region. Numerical modelling could distinguish betw
Externí odkaz:
https://doaj.org/article/81d22754eba84d2baaaa3336ab14de9f
Autor:
Vilmos Steinmann, Ákos Kereszturi
Publikováno v:
Aerospace, Vol 11, Iss 9, p 784 (2024)
A model-based surface fluvial erosion and deposition approach was adapted to Martian conditions to forecast the potential locations for shallow subsurface sampling by the Rosalind Franklin ExoMars rover at Oxia Planum. While remote and on-site images
Externí odkaz:
https://doaj.org/article/f08a74bd0f4544b3b39c39f391cf7370
Publikováno v:
Hungarian Geographical Bulletin, Vol 69, Iss 4, Pp 333-348 (2020)
This work analysis an 81 km long 1.85 km wide fluvial valley on Mars (at 2°55’ South and 111°53’ East) for the first time, located near to the so-called Palos carter and Tinto Vallis, called Tinto-B hereafter. The length of the valley is approx
Externí odkaz:
https://doaj.org/article/84751069beeb4e6fbf66b005103ff579
Autor:
Vilmos Steinmann, Ákos Kereszturi
There are many hydrological models for normal terrestrial environments based on precipitation related erosion, but few of them work well in arid and hyper-arid conditions. These extreme arid regions can be good Mars analogue sites to test and model t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6c1f89a6317f35c0a8175aafc86f1f29
https://doi.org/10.5194/egusphere-egu23-5987
https://doi.org/10.5194/egusphere-egu23-5987
Autor:
Vilmos Steinmann, Ákos Kereszturi
Introduction: Simulating the fluvial activity produced landscape changes on the Earth is difficult and even harder on another planet, like Mars. There are several erosion models (eg. USLE, RUSLE), which can be well used in terrestrial environments, b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ac855cedac43608ef9b859d23e500302
https://doi.org/10.5194/egusphere-egu22-7857
https://doi.org/10.5194/egusphere-egu22-7857
Autor:
Rickbir Bahia, Vilmos Steinmann
Introduction: Mars’ surface is carved by an array of dendritic valley networks, which are evidence for ancient water cycles and surface run-off on Mars. The majority of these networks appear to have formed during the Late Noachian – Early Hesperi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b9816de1ad12bf01ee7c3cec7d0aa6b0
https://doi.org/10.5194/egusphere-egu22-1282
https://doi.org/10.5194/egusphere-egu22-1282
Autor:
Vilmos Steinmann, Ákos Kereszturi
Most of the Martian fluvial valleys formed in the early period (around the Noachian-Hesperian boundary or before), but the formation durations are not well determined, however it would be important to understand as it is related to the climatic histo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dee7e2edf735ced9c3f41fa7b5c52d3e
https://doi.org/10.5194/epsc2021-212
https://doi.org/10.5194/epsc2021-212
Autor:
Vilmos Steinmann, Ákos Kereszturi
Publikováno v:
Icarus. 322:54-68
Several characteristics of very small impact craters of lunar surface have recently been improved by high resolution datasets. Lunar impact craters with diameter below 100 m and especially below 10 m were surveyed and compared at mare and terra surfa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ff2da0852b2252297976561b12bfb8c9
https://doi.org/10.1016/j.icarus.2018.12.039
https://doi.org/10.1016/j.icarus.2018.12.039
Autor:
Vilmos Steinmann, Ákos Kereszturi
The erosion on Mars is poorly understood, especially the fluvial erosion, which modified obviously the surface of the Red Planet. There are several erosion models for the terrestrial environment. These models are without climbing completeness: USLE,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::55fa3b7212cf04bbcef8b83b75b0e3bd
https://doi.org/10.5194/epsc2020-227
https://doi.org/10.5194/epsc2020-227
Surface erosion happened intensively of Mars in the Noachian, partly from precipitation and/or ice melting. However the exact method of erosion is poorly understood, despite various models are used for the Earth successfully. In this work we present
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::96ecbb14ffc76629deb9dd7fba4c6351
https://doi.org/10.5194/egusphere-egu2020-204
https://doi.org/10.5194/egusphere-egu2020-204