Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Hoor AlMazmi"'
Autor:
Michael S. Chaffin, Christopher M. Fowler, Justin Deighan, Sonal Jain, Greg Holsclaw, Andréa Hughes, Robin Ramstad, Yaxue Dong, Dave Brain, Hoor AlMazmi, Krishnaprasad Chirakkil, John Correira, Scott England, J. Scott Evans, Matt Fillingim, Rob Lillis, Fatma Lootah, Susarla Raghuram, Jim McFadden, Jasper Halekas, Jared Espley, Nick Schneider, Majd Mayyasi, Christina O. Lee, Shannon Curry, Hessa AlMatroushi
Publikováno v:
Geophysical Research Letters, Vol 49, Iss 17, Pp n/a-n/a (2022)
Abstract Proton aurora at Mars are thought to form indirectly, as a result of solar wind proton charge exchange with planetary coronal hydrogen upstream of the bow shock. This charge exchange produces beamed energetic neutral atoms that bypass the in
Externí odkaz:
https://doaj.org/article/743a0c865bd44c1b9285ab3263056d5c
Autor:
Matthew Fillingim, Robert Lillis, Anna Mittelholz, Hessa AlMatroushi, Hoor AlMazmi, Michael Chaffin, Peter Chi, Krishnaprasad Chirakkil, John Corriera, Justin Deighan, Scott England, Scott Evans, Heidi Haviland, Greg Holsclaw, Sonal Jain, Catherine Johnson, Steven Joy, Benoit Langlais, Fatma Lootah, Susarla Raghuram
The Emirates Mars Ultraviolet Spectrometer (EMUS) onboard the Emirates Mars Mission spacecraft, which observes ultraviolet emission between approximately 100 and 170 nm, has observed multiple instances of nightside aurora at Mars. Variations in the a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5294224ee218215d527b6caa8dc21d5f
https://doi.org/10.5194/egusphere-egu23-2149
https://doi.org/10.5194/egusphere-egu23-2149
Autor:
Michael Chaffin, Justin Deighan, Sonal Jain, Greg Holsclaw, Raghuram Susarla, Hoor AlMazmi, Krishnaprasad Chirakkil, John Correira, Scott England, Frank Eparvier, J. Scott Evans, Matt Fillingim, Rob Lillis, Fatma Lootah, Ed Thiemann, Shannon Curry, Hessa AlMatroushi
The surface of the planet Mars exhibits a record of dessiccation and oxidation, the legacy of significant water escape to space as hydrogen and oxygen. This H escape can be constrained using ultraviolet observations of the planet's upper atmosphere,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f834f579ec992b1c0668fcc83e251d16
https://doi.org/10.5194/egusphere-egu23-9200
https://doi.org/10.5194/egusphere-egu23-9200
Autor:
Sonal K. Jain, Justin Deighan, Mike Chaffin, Greg Holsclaw, Rob Lillis, Matt Fillingim, J. Scott Evans, John Correira, Hessa AlMatroushi, Fatma Lootah, Scott England, Hoor AlMazmi, Ed Thiemann, Phil Chamberlin, Frank Eparvier
We present the first continuous observations of the extreme and far ultraviolet (EUV and FUV) dayglow emissions measured by Emirates Mars Ultraviolet Spectrometer (EMUS) onboard the Emirates Mars Mission. We found excellent agreement between the prev
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d26f693a287ac54749106e00cd2cc089
https://hdl.handle.net/10919/114852
https://hdl.handle.net/10919/114852
Autor:
Michael S. Chaffin, Justin Deighan, Sonal Jain, Greg Holsclaw, Hoor AlMazmi, Krishnaprasad Chirakkil, John Correira, Scott England, J. Scott Evans, Matt Fillingim, Rob Lillis, Fatma Lootah, Susarla Raghuram, Frank Eparvier, Ed Thiemann, Shannon Curry, Hessa AlMatroushi
Publikováno v:
Geophysical Research Letters. 49
Water is lost from the Mars upper atmosphere to space as hydrogen and oxygen, both of which can be observed in scattered ultraviolet sunlight at 102.6 nm. We present Emirates Mars Mission Emirates Mars Ultraviolet Spectrometer (EMM/EMUS) insertion or
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7c553464f889d35b4249c667c244a29c
https://doi.org/10.1029/2022gl099851
https://doi.org/10.1029/2022gl099851
Autor:
Michael Chaffin, Hoor Almazmi, Krishnaprasad Chirakkil, John Correira, Justin Deighan, Scott England, J. Scott Evans, Matthew Fillingim, Greg Holsclaw, Sonal Jain, Rob Lillis, Fatma Lootah, Susarla Raghuram, Hessa Al Matroushi
The Emirates Mars Ultraviolet Spectrometer (EMUS) instrument is one of three science instruments on board the “Hope Probe” of the Emirates Mars Mission (EMM). EMM arrived at Mars on February 9 2021, in order to explore the global dynamics of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::91303f7a8301a212d5b9818d68303270
https://doi.org/10.5194/egusphere-egu22-10731
https://doi.org/10.5194/egusphere-egu22-10731
Autor:
Hessa Almatroushi, Hoor AlMazmi, Noora AlMheiri, Mariam AlShamsi, Eman AlTunaiji, Khalid Badri, Robert J. Lillis, Fatma Lootah, Maryam Yousuf, Sarah Amiri, David A. Brain, Michael Chaffin, Justin Deighan, Christopher S. Edwards, Francois Forget, Michael D. Smith, Michael J. Wolff, Philip R. Christensen, Scott England, Matthew Fillingim, Gregory M. Holsclaw, Sonal Jain, Andrew R. Jones, Mikki Osterloo, Bruce M. Jakosky, Janet G. Luhmann, Roland M. B. Young
Publikováno v:
Space Science Reviews. 217
The Emirates Mars Mission (EMM) – Hope Probe – was developed to understand Mars atmospheric circulation, dynamics, and processes through characterization of the Mars atmosphere layers and its interconnections enabled by a unique high-altitude (19
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::08a4abee562437ae6f3dacc935fda6cc
https://doi.org/10.1007/s11214-021-00851-6
https://doi.org/10.1007/s11214-021-00851-6