Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Mariah Baker"'
Autor:
Constantinos Charalambous, Matt Golombek, Tom Pike, Mark Lemmon, Aymeric Spiga, Claire Newman, Veronique Ansan, Mariah Baker, Maria Banks, Ralph Lorenz, Alexander Stott, Daniel Viudez-Moreiras
Aeolian activity, the movement of sand and dust by the wind, is common on Earth and has been observed on other planets [1]. Under the current climatic conditions on Mars, aeolian activity is the primary process of surface modification driven by winds
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f61838866e5c47ecc2f6fb7450e06b52
https://doi.org/10.5194/egusphere-egu23-9921
https://doi.org/10.5194/egusphere-egu23-9921
Autor:
Catherine M. Weitz, Catherine O’Connell‐Cooper, Lucy Thompson, Robert J. Sullivan, Mariah Baker, John A. Grant
Publikováno v:
Journal of Geophysical Research: Planets. 127
Autor:
Kathryn M. Stack, William E. Dietrich, Michael P. Lamb, Robert J. Sullivan, John R. Christian, Claire E. Newman, Catherine D. O’Connell‐Cooper, Jonathan W. Sneed, Mackenzie Day, Mariah Baker, Raymond E. Arvidson, Christopher M. Fedo, Sabrina Khan, Rebecca M. E. Williams, Kristen A. Bennett, Alexander B. Bryk, Shannon Cofield, Lauren A. Edgar, Valerie K. Fox, Abigail A. Fraeman, Christopher H. House, David M. Rubin, Vivian Z. Sun, Jason K. Van Beek
Publikováno v:
Journal of Geophysical Research: Planets. 127
Gale crater, the field site for NASA's Mars Science Laboratory Curiosity rover, contains a diverse and extensive record of aeolian deposition and erosion. This study focuses on a series of regularly spaced, curvilinear, and sometimes branching bedroc
The transition from sand ripples to megaripples encodes information about the physics of how both sand-sized (moved via saltation) and coarsegrained (moved via impact creep) particles interact unde...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2d81b86815dbc8a85a64b73d5fe5449f
https://doi.org/10.1002/essoar.10502483.1
https://doi.org/10.1002/essoar.10502483.1
Autor:
Mariah Baker, Beth Willman
Observational bias against finding Milky Way (MW) dwarf galaxies at low Galactic latitudes (b < 20 deg) and at low surface brightnesses (fainter than 29 mag arcsec^-2, in the V-band) currently limits our understanding of the faintest limits of the ga
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a4d1bebcb54ad2c6bdebd61c267cc78e
http://arxiv.org/abs/1507.00734
http://arxiv.org/abs/1507.00734
Autor:
Jay Strader, Annie Preston, Andrew P. Sturner, Tonima Tasnim Ananna, Ross Fadely, Tim Douglas, Erin Boettcher, Jacob Gilbert, Mariah Baker, Emily C. Cunningham, Beth Willman, Erica Hopkins
We present an extensive search for RR Lyrae stars in and around the ultra-faint Milky Way companions Segue 2 and Segue 3. The former (M_V = -2.5, Belokurov et al. 2009) appears to be an extremely faint dwarf galaxy companion of the Milky Way. The lat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::81f8768e77161185013afd3cb819d4aa
http://arxiv.org/abs/1308.2227
http://arxiv.org/abs/1308.2227
Autor:
Bernard Hallet, Ronald S. Sletten, Michael Malin, Nicolas Mangold, Robert J. Sullivan, Alberto G. Fairén, Germán Martínez, Mariah Baker, Juergen Schieber, Javier Martin‐Torres, Maria‐Paz Zorzano
Publikováno v:
Journal of Geophysical Reseacrh-Planets
On Mars, near the equator, much of the terrain in Gale Crater consists of bedrock outcrops separated by relatively smooth, uniform regolith surfaces. In scattered sites, however, distinct patterns—in the form and texture of the ground surface—con