Zobrazeno 1 - 10
of 53
pro vyhledávání: '"T. J. BRADLEY"'
Autor:
D. A. Sallman, M. M. Al Malki, A. S. Asch, E. S. Wang, J. G. Jurcic, T. J. Bradley, I. W. Flinn, D. A. Pollyea, S. N. Kambhampati, T. N. Tanaka, J. F. Zeidner, G. Garcia-Manero, D. Jeyakumar, L. Gu, A. Tan, M. Chao, C. O’Hear, I. Lal, P. Vyas, N. Daver
Publikováno v:
HemaSphere, Vol 6, Pp 67-68 (2022)
Externí odkaz:
https://doaj.org/article/f11a8ee031f8479881eff9499ea7ccf4
Publikováno v:
Journal of Geophysical Research: Space Physics. 127
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5958817e6c14bb75018c9bbed7de1d4d
https://doi.org/10.1029/2021ja030198
https://doi.org/10.1029/2021ja030198
Autor:
N. R. Staniland, Elias Roussos, G. Provan, Stanley W. H. Cowley, G. J. Hunt, Hao Cao, Chihiro Tao, T. J. Bradley, Michele K. Dougherty, Emma J. Bunce
Publikováno v:
Journal of Geophysical Research: Space Physics. 126
During Cassini's Grand Finale proximal orbits, the spacecraft traversed the nightside magnetotail to ∼21 Saturn radii. Clear signatures of Saturn's equatorial current sheet are observed in the magnetic field data. An axisymmetric model of the ring
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0e73921dc8ac609297274eb4533f0bdd
https://doi.org/10.1029/2020ja028605
https://doi.org/10.1029/2020ja028605
Autor:
G. Provan, G. J. Hunt, Stanley W. H. Cowley, Emma J. Bunce, T. J. Bradley, Nicholas Achilleos
Publikováno v:
Journal of Geophysical Research: Space Physics. 125
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::39b3239b6a98ec86ddbd6158a321b2d3
https://doi.org/10.1029/2020ja028247
https://doi.org/10.1029/2020ja028247
Autor:
G. J. Hunt, Hao Cao, G. Provan, Stanley W. H. Cowley, Michele K. Dougherty, T. J. Bradley, Emma J. Bunce
Publikováno v:
Journal of Geophysical Research: Space Physics. 124:379-404
Work at the University of Leicester was supported by STFC grant ST/N000749/1. Work at Imperial College was supported by STFC grant ST/N000692/1. EJB was supported by a Royal Society Wolfson Research Merit Award. MKD was supported by Royal Society Res
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::334ccaed5f144754a1b93657256dd14e
https://doi.org/10.1029/2018ja026121
https://doi.org/10.1029/2018ja026121
Autor:
Elias Roussos, Emma J. Bunce, Chihiro Tao, Stan W. H. Cowley, G. J. Hunt, Gabrielle Provan, T. J. Bradley, Michele K. Dougherty, N. R. Staniland
The presence of a substantial azimuthal current sheet in Saturn’s magnetosphere was identified in Voyager and Pioneer magnetometer data. Data from these spacecraft showed depressions in the strength of the field below that expected for the internal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ec4519df9edd5472a031303e2e8b1bd9
https://doi.org/10.5194/egusphere-egu2020-11306
https://doi.org/10.5194/egusphere-egu2020-11306
Autor:
Stanley W. H. Cowley, A. W. Smith, G. Provan, Emma J. Bunce, T. J. Bradley, Caitriona M. Jackman
Publikováno v:
Journal of Geophysical Research: Space Physics. 123:9476-9507
We conduct a statistical analysis of 2,094 reconnection events in Saturn's near-equatorial magnetotail previously identified in Cassini magnetometer data from intervals during 2006 and 2009/2010. These consist of tailward propagating plasmoids and pl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::327415c95c6fdbc0d15eb6b91edcd586
https://doi.org/10.1029/2018ja025932
https://doi.org/10.1029/2018ja025932
Autor:
Stanley W. H. Cowley, T. J. Bradley, Michele K. Dougherty, Emma J. Bunce, G. Provan, G. J. Hunt
Publikováno v:
Journal of Geophysical Research: Space Physics. 123:3859-3899
We determine properties of Saturn's planetary period oscillations from Cassini magnetic measurements over the ~2‐year interval from September 2015 to end of mission in September 2017, spanning Saturn northern summer solstice in May 2017. Phases of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d7773f25793342bf79240e985bf8f8c6
https://doi.org/10.1029/2018ja025237
https://doi.org/10.1029/2018ja025237
Autor:
Stanley W. H. Cowley, Michele K. Dougherty, G. J. Hunt, G. Provan, Emma J. Bunce, T. J. Bradley, Hao Cao
We analyze periapsis pass magnetic field data from the final 23 orbits of the Cassini spacecraft at Saturn, uniquely encompassing auroral, subauroral, ring region, and intra-ring field lines, to determine the planetary period oscillations (PPOs) and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::078ff0db350006f80fd57f1a8e082e8c
https://resolver.caltech.edu/CaltechAUTHORS:20200206-081459766
https://resolver.caltech.edu/CaltechAUTHORS:20200206-081459766
Autor:
Wayne Pryor, Alexander Bader, G. Provan, T. J. Bradley, Chihiro Tao, Joe Kinrade, Zhonghua Yao, G. J. Hunt, Emma J. Bunce, Sarah V. Badman, Licia C Ray, Stanley W. H. Cowley
Saturn's main aurorae are thought to be generated by plasma flow shears associated with a gradient in angular plasma velocity in the outer magnetosphere. Dungey cycle convection across the polar cap, in combination with rotational flow, may maximize
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7c66d5c35bae9054f2ce91cd70498f18
https://doi.org/10.1029/2019GL084620
https://doi.org/10.1029/2019GL084620