Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Michael S. Chaffin"'
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:
Alexey A. Novoselov, Dailto Silva, Jerusa Schneider, Ximena Celeste Abrevaya, Michael S. Chaffin, Paloma Serrano, Margareth Sugano Navarro, Maria Josiane Conti, Carlos Roberto de Souza Filho
Publikováno v:
Scientific Reports, Vol 7, Iss 1, Pp 1-11 (2017)
Abstract The environmental conditions on the Earth before 4 billion years ago are highly uncertain, largely because of the lack of a substantial rock record from this period. During this time interval, known as the Hadean, the young planet transforme
Externí odkaz:
https://doaj.org/article/389e8aa024af44deba1bc287f0007ec9
Publikováno v:
Journal of Geophysical Research: Planets. 128
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ad0ff000f01f07e5a68f9f8b5c7b8f08
https://doi.org/10.1029/2022je007576
https://doi.org/10.1029/2022je007576
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