Zobrazeno 1 - 10
of 150
pro vyhledávání: '"Yin, QZ"'
Autor:
Jenniskens, P, Utas, J, Yin, QZ, Matson, RD, Fries, M, Howell, JA, Free, D, Albers, J, Devillepoix, H, Bland, P, Miller, A, Verish, R, Garvie, LAJ, Zolensky, ME, Ziegler, K, Sanborn, ME, Verosub, KL, Rowland, DJ, Ostrowski, DR, Bryson, K, Laubenstein, M, Zhou, Q, Li, QL, Li, XH, Liu, Y, Tang, GQ, Welten, K, Caffee, MW, Meier, MMM, Plant, AA, Maden, C, Busemann, H, Granvik, M
Publikováno v:
Meteoritics and Planetary Science, vol 54, iss 4
Jenniskens, P; Utas, J; Yin, QZ; Matson, RD; Fries, M; Howell, JA; et al.(2019). The Creston, California, meteorite fall and the origin of L chondrites. Meteoritics and Planetary Science. doi: 10.1111/maps.13235. UC Davis: Retrieved from: http://www.escholarship.org/uc/item/1tj2s85x
Jenniskens, P; Utas, J; Yin, QZ; Matson, RD; Fries, M; Howell, JA; et al.(2019). The Creston, California, meteorite fall and the origin of L chondrites. Meteoritics and Planetary Science. doi: 10.1111/maps.13235. UC Davis: Retrieved from: http://www.escholarship.org/uc/item/1tj2s85x
It has been proposed that all L chondrites resulted from an ongoing collisional cascade of fragments that originated from the formation of the ~500Ma old asteroid family Gefion, located near the 5:2 mean-motion resonance with Jupiter in the middle Ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::0938f17118952881cceda62fdad6f09a
https://escholarship.org/uc/item/1tj2s85x
https://escholarship.org/uc/item/1tj2s85x
Publikováno v:
Shi, X; Yin, QZ; Gao, H; Chang, YC; Jackson, WM; Wiens, RC; et al.(2017). Branching Ratios in Vacuum Ultraviolet Photodissociation of CO and N2: Implications for Oxygen and Nitrogen Isotopic Compositions of the Solar Nebula. Astrophysical Journal, 850(1). doi: 10.3847/1538-4357/aa8ee7. UC Davis: Retrieved from: http://www.escholarship.org/uc/item/62s4b93z
© 2017. The American Astronomical Society. All rights reserved.. NASA's Genesis mission reveals that the rare isotope15N is approximately seven times more enriched than the rare isotopes17O and18O in the terrestrial planets relative to the Sun. Here
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::55f4a1082ce801226d68a74cbdb70d83
http://www.escholarship.org/uc/item/62s4b93z
http://www.escholarship.org/uc/item/62s4b93z
Publikováno v:
Lu, Z; Chang, YC; Yin, QZ; Ng, CY; & Jackson, WM. (2014). Evidence for direct molecular oxygen production in CO2photodissociation. Science, 346(6205), 61-64. doi: 10.1126/science.1257156. UC Davis: Retrieved from: http://www.escholarship.org/uc/item/3pq1x57q
Photodissociation of carbon dioxide (CO2) has long been assumed to proceed exclusively to carbon monoxide (CO) and oxygen atom (O) primary products. However, recent theoretical calculations suggested that an exit channel to produce C + O2should also
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::a6c2310d83980daa429e2adb3e5efb59
http://www.escholarship.org/uc/item/3pq1x57q
http://www.escholarship.org/uc/item/3pq1x57q
Publikováno v:
Gao, H; Song, Y; Chang, YC; Shi, X; Yin, QZ; Wiens, RC; et al.(2013). Branching ratio measurements for vacuum ultraviolet photodissociation of12C16O. Journal of Physical Chemistry A, 117(29), 6185-6195. doi: 10.1021/jp400412n. UC Davis: Retrieved from: http://www.escholarship.org/uc/item/3dd7z08n
The branching ratios for the spin-forbidden photodissociation channels of12C16O in the vacuum ultraviolet (VUV) photon energy region from 102 500 (12.709 eV) to 106 300 cm-1(13.180 eV) have been investigated using the VUV laser time-slice velocity-ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::07340744c09a8440c5f67c6766a5f89d
http://www.escholarship.org/uc/item/3dd7z08n
http://www.escholarship.org/uc/item/3dd7z08n
Publikováno v:
Modeling the interglacials of the last one million years.
Publikováno v:
Astronomical theory and orbital forcing.
Autor:
BERGER A. CLAUSSEN M., YIN QZ.
Publikováno v:
Factor Separation Method and Paleoclimates.
Publikováno v:
Modelling the Past and Future Interglacials in Response to Astronomical and Greenhouse Gas Forcing.
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