Zobrazeno 1 - 7
of 7
pro vyhledávání: '"E. I. Schaefer"'
Publikováno v:
Icarus. 317:621-648
The origin or origins of recurring slope lineae (RSL) on Mars are enigmatic. These seasonally dark, linear features correlate with temperatures appropriate for liquid water or brine. They also progress slowly downslope and fade (disappear) when inact
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1d5851f09ff1d2be794fcd55223cb42f
https://doi.org/10.1016/j.icarus.2018.07.014
https://doi.org/10.1016/j.icarus.2018.07.014
Autor:
Christopher W. Hamilton, Ali M. Bramson, E. I. Schaefer, S. P. Beard, M. M. Sori, Catherine D. Neish
Publikováno v:
Journal of Geophysical Research: Solid Earth. 126
Can fractal analysis enable us to classify a lava flow to a morphologic type (e.g., ‘a‘ā vs. pāhoehoe) solely by examining the geometry of the flow’s margin? If so, these classifications would prov...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ed9d9c7553ee6f27fa61b9c5d3758a10
https://doi.org/10.1029/2020jb020949
https://doi.org/10.1029/2020jb020949
Autor:
Alfred S. McEwen, Leslie K. Tamppari, Matthew Chojnacki, Sarah S. Sutton, E. I. Schaefer, Colin M. Dundas
Publikováno v:
Journal of Geophysical Research: Planets. 126
Following the planet-encircling dust event (PEDE) of Mars Year (MY) 34, MRO/HiRISE has seen many more candidate RSL than in typical Mars years. They were imaged at more than 285 unique locations fr...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::173d63b5f7b2e46f596981a4b472a635
https://doi.org/10.1029/2020je006575
https://doi.org/10.1029/2020je006575
Autor:
R. C. Elphic, Joshua L. Bandfield, Jennifer L. Heldmann, Lynn M. Carter, S. E. Kobs Nawotniak, Catherine D. Neish, J. R. Skok, D. S. S. Lim, Scott S. Hughes, William Brent Garry, Christopher W. Hamilton, E. I. Schaefer, Gordon R. Osinski
Publikováno v:
Icarus. 281:73-89
Lunar impact melt deposits have unique physical properties. They have among the highest observed radar returns at S-Band (12.6 cm wavelength), implying that they are rough at the decimeter scale. However, they are also observed in high-resolution opt
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d48b8151fb03554825a6a151b07bb765
https://doi.org/10.1016/j.icarus.2016.08.008
https://doi.org/10.1016/j.icarus.2016.08.008
Autor:
E. I. Schaefer, Jon D. Pelletier
Publikováno v:
Computers & Geosciences. 145:104554
In many geomorphic applications, it is necessary to reduce a polygon to a set of axial lines. For example, consider a fluvial channel network. On the one hand, this network has a polygonal footprint with reaches of finite width organized into a branc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cc6c583b80147d5cd1bd77ca3263184c
https://doi.org/10.1016/j.cageo.2020.104554
https://doi.org/10.1016/j.cageo.2020.104554
Autor:
E. I. Schaefer, Shane Byrne, Sarah Mattson, Marion Massé, Alfred S. McEwen, Lujendra Ojha, Colin M. Dundas, James J. Wray
Publikováno v:
Icarus. 231:365-376
Recurring Slope Lineae (RSL) are active features on Mars that might require flowing water. Most examples observed through 2011 formed on steep, equator-facing slopes in the southern mid-latitudes. They form and grow during warm seasons and fade and o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3a7ff26dad95558862ac7c61422deff8
https://doi.org/10.1016/j.icarus.2013.12.021
https://doi.org/10.1016/j.icarus.2013.12.021
Publikováno v:
Geophysical Research Letters. 38
[1] A fresh, 1.85 km diameter impact crater in the midlatitudes of Mars (38°N) named Vaduz exhibits distinctive crater‐related geological subunits (facies) extending up to ∼15 radii from the rim crest and perched >10 m above the adjacent plains.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b89c5bc6cfc25a83c48b9dfbc8e4dee3
https://doi.org/10.1029/2010gl046605
https://doi.org/10.1029/2010gl046605