Zobrazeno 1 - 10
of 22
pro vyhledávání: '"James F. J. Bryson"'
Autor:
Elias N. Mansbach, Jay Shah, Wyn Williams, Clara Maurel, James F. J. Bryson, Benjamin P. Weiss
Publikováno v:
Geochemistry, Geophysics, Geosystems, Vol 23, Iss 11, Pp n/a-n/a (2022)
Abstract Paleomagnetic studies of meteorites provide unique constraints on the evolution of magnetic fields in the early solar system. These studies rely on the identification of magnetic minerals that can retain stable magnetizations over ≳4.5 bil
Externí odkaz:
https://doaj.org/article/7b985affd42e4f60acf36d614a1638cf
Autor:
Claire I. O. Nichols, James F. J. Bryson, Roberts Blukis, Julia Herrero‐Albillos, Florian Kronast, Rudolf Rüffer, Aleksandr I. Chumakov, Richard J. Harrison
Publikováno v:
Geochemistry, Geophysics, Geosystems, Vol 21, Iss 2, Pp n/a-n/a (2020)
Abstract Iron and stony‐iron meteorites form the Widmanstätten pattern during slow cooling. This pattern is composed of several microstructures whose length‐scale, composition and magnetic properties are dependent upon cooling rate. Here we focu
Externí odkaz:
https://doaj.org/article/db27a17e0fca49ab8dcdf55a89be8de0
Autor:
James F. J. Bryson
Publikováno v:
International Journal of Philosophy and Theology. 81:136-154
This article situates Roger Scruton in the tradition of Christian Platonism. It begins by revisiting Scruton’s reluctance to pursue theological speculation as it has been traditionally practised in...
Autor:
James F. J. Bryson, Francis Nimmo, B. Getzin, Benjamin P. Weiss, Andreas Scholl, J. N. H. Abrahams
Publikováno v:
other univ website
The textures and accretion ages of chondrites have been used to argue that their parent asteroids never differentiated. Without a core, undifferentiated planetesimals could not have generated magnetic fields through dynamo activity, so chondrites are
Autor:
James F. J. Bryson, Florian Kronast, Julia Herrero-Albillos, Claire I. O. Nichols, Richard J. Harrison, Roger R. Fu, Benjamin P. Weiss, John A. Tarduno, Rory D. Cottrell
Several paleomagnetic studies have been conducted on five main group pallasites: Brenham, Marjalahti, Springwater, Imilac and Esquel. These pallasites have distinct cooling histories, meaning that ...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ba6a6682cdadd6d78c4cec72b84a2376
https://doi.org/10.1002/essoar.10506802.1
https://doi.org/10.1002/essoar.10506802.1
Autor:
Carol A. Raymond, Linda T. Elkins-Tanton, Benjamin P. Weiss, Jay Shah, Rajesh V. Chopdekar, Clara Maurel, James F. J. Bryson
Publikováno v:
Geophysical Research Letters, vol 48, iss 6
Geophysical Research Letters
Geophysical Research Letters, American Geophysical Union, 2021, 48 (6), ⟨10.1029/2020GL091917⟩
Geophysical Research Letters, 2021, 48 (6), ⟨10.1029/2020GL091917⟩
Geophysical Research Letters
Geophysical Research Letters, American Geophysical Union, 2021, 48 (6), ⟨10.1029/2020GL091917⟩
Geophysical Research Letters, 2021, 48 (6), ⟨10.1029/2020GL091917⟩
The existence of numerous iron meteorite groups indicates that some planetesimals underwent melting that led to metal-silicate segregation, sometimes producing metallic cores. Meteorite paleomagnetic records suggest that crystallization of these core
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::19f9d9aff4c81604760a9c21c4152851
https://escholarship.org/uc/item/79j4x6ch
https://escholarship.org/uc/item/79j4x6ch
Carbonaceous chondrites experienced varying degrees of aqueous alteration on their parent asteroids, which influenced their mineralogies, textures, and bulk chemical and isotopic compositions. Although this alteration was a crucial event in the histo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cebd91a555ea7af1dbd1063ef5bf91e0
https://www.repository.cam.ac.uk/handle/1810/329257
https://www.repository.cam.ac.uk/handle/1810/329257
Autor:
Claire I. O. Nichols, James F. J. Bryson, Roger R. Fu, Benjamin P. Weiss, Richard J. Harrison, John A. Tarduno, Rory D. Cottrell, Florian Kronast, Julia Herrero-Albillos
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Funder: FP7 Ideas: European Research Council (FP7 Ideas); Id: http://dx.doi.org/10.13039/100011199; Grant(s): 320750, 312284
Funder: NASA Solar Systems Workings program
Funder: The Geological Society
Funder: Mineralogical Society of Gr
Funder: NASA Solar Systems Workings program
Funder: The Geological Society
Funder: Mineralogical Society of Gr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::485e3d7371255d122cd50d8a477c14f7
https://www.repository.cam.ac.uk/handle/1810/325832
https://www.repository.cam.ac.uk/handle/1810/325832
Autor:
Richard J. Harrison, James F. J. Bryson, Claire I. O. Nichols, Florian Kronast, Rudolf Rüffer, Roberts Blukis, Julia Herrero-Albillos, Aleksandr I. Chumakov
Publikováno v:
Zaguán: Repositorio Digital de la Universidad de Zaragoza
Universidad de Zaragoza
Geochemistry Geophysics Geosystems (G3)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Zaguán. Repositorio Digital de la Universidad de Zaragoza
Universidad de Zaragoza
Geochemistry Geophysics Geosystems (G3)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Zaguán. Repositorio Digital de la Universidad de Zaragoza
Iron and stony‐iron meteorites form the Widmanstätten pattern during slow cooling. This pattern is composed of several microstructures whose length‐scale, composition and magnetic properties are dependent upon cooling rate. Here we focus on the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3761082ae152fbf7e5bbc2675f971f46
https://ora.ox.ac.uk/objects/uuid:4c93add9-5051-4d7e-a84d-62a11738adbb
https://ora.ox.ac.uk/objects/uuid:4c93add9-5051-4d7e-a84d-62a11738adbb
Autor:
R. J. Lyons, James F. J. Bryson, Matthew R. Ball, Benjamin P. Weiss, Rajesh V. Chopdekar, Andreas Scholl, Clara Maurel, William F. Bottke, Fred J. Ciesla
Publikováno v:
Science advances, vol 6, iss 30
Science Advances
Science Advances
A broad spectrum of fully differentiated, partially melted, and possibly unmelted objects populated the early solar system.
Modern meteorite classification schemes assume that no single planetary body could be source of both unmelted (chondritic
Modern meteorite classification schemes assume that no single planetary body could be source of both unmelted (chondritic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9d5af6bd55e0c22af80ab5cd4b8a44ff
https://escholarship.org/uc/item/4b00b540
https://escholarship.org/uc/item/4b00b540