Zobrazeno 1 - 10
of 13
pro vyhledávání: '"Phil J. Sutton"'
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
We perform simulations of the M⊕ self-gravitating exoring thought to orbit the large exoplanet J1407b. We use a mass of MJ1407b=20MJ (which is close to the revised upper limit) and a semi-major axis of a=5AU, equating to an orbital period of ∼11y
Externí odkaz:
https://doaj.org/article/7c056a1bd9614dcfa931d1123ba68531
Autor:
M James Salinger, James Renwick, Erik Behrens, A Brett Mullan, Howard J Diamond, Pascal Sirguey, Robert O Smith, Michael C T Trought, Lisa Alexander V, Nicolas J Cullen, B Blair Fitzharris, Christopher D Hepburn, Amber K Parker, Phil J Sutton
Publikováno v:
Environmental Research Letters, Vol 14, Iss 4, p 044023 (2019)
During austral summer (DJF) 2017/18, the New Zealand region experienced an unprecedented coupled ocean-atmosphere heatwave, covering an area of 4 million km ^2 . Regional average air temperature anomalies over land were +2.2 °C, and sea surface temp
Externí odkaz:
https://doaj.org/article/6c7b5c2c9120425494b7bda244cbd94f
Autor:
James A. Renwick, Phil J. Sutton, Mads S. Thomsen, Allan Siano, Michael C. T. Trought, Howard J. Diamond, Claire Scofield, Amber Parker, Edmar Teixeira, B. B. Fitzharris, Huub Kerckhoffs, Robert O. Smith, M. James Salinger, Nicholas Herold, Paul Johnstone, Erik Behrens, A. Brett Mullan, Paul M. South, Denise Fernandez
Publikováno v:
Climatic Change. 162:485-506
During austral summers (DJF) 1934/35, 2017/18 and 2018/19, the New Zealand (NZ) region (approximately 4 million km2) experienced the most intense coupled ocean-atmosphere heatwaves on record. Average air temperature anomalies over land were + 1.7 to
Autor:
Graham J. Rickard, Phil J. Sutton, Jonny Williams, Erik Behrens, Michael Williams, Olaf Morgenstern
Publikováno v:
Journal of Advances in Modeling Earth Systems, Vol 12, Iss 7, Pp n/a-n/a (2020)
This paper describes the development of New Zealand's Earth System Model (NZESM) and evaluates its performance against its parent model (United Kingdom Earth System Model, UKESM) and observations. The main difference between the two earth system mode
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::92d5325051eac19337f39c26909c3df4
https://doi.org/10.1002/essoar.10501460.1
https://doi.org/10.1002/essoar.10501460.1
Publikováno v:
International Journal of Astrobiology. 18:323-328
High-density regions within the spiral arms are expected to have profound effects on passing stars. Understanding of the potential effects on the Earth and our Solar System is dependent on a robust model of arm passage dynamics. Using a novel combina
Autor:
Christopher P. Wirth, Kathryn V. Lester, Elisa V. Quintana, Samuel N. Quinn, Alex Hughes, Roland Vanderspek, Juliette C. Becker, Elise Furlan, Eric L. N. Jensen, Elisabeth Matthews, Courtney D. Dressing, Keivan G. Stassun, Shaun Atherton, Phil J. Sutton, Steven Giacalone, A. Fukui, Ian J. M. Crossfield, J. Villasenor, Enric Palle, Richard P. Schwarz, Felipe Murgas, George Zhou, Crystal L. Gnilka, Norio Narita, Andrew Vanderburg, George R. Ricker, Dax L. Feliz, Adrian M. Price-Whelan, Erica J. Gonzales, Jeffrey C. Smith, Karen Collins, Luke G. Bouma, Jon M. Jenkins, Megan Bedell, Joshua N. Winn, Trevor J. David, Nicholas J. Scott, Joseph E. Rodriguez, Tianjun Gan, Daniel J. Stevens, René Tronsgaard, Allyson Bieryla, Christina Hedges, Tara Fetherolf, Michael Vezie, Sara Seager, John F. Kielkopf, David W. Latham, Lars A. Buchhave, Michael B. Lund, Steve B. Howell, Robert J. Siverd
Publikováno v:
The Astronomical Journal. 162:305
Autor:
Phil J. Sutton
With the use of numerical models, we investigate whether Mean Motion Resonances (MMR) with nearby moons to the J1407b ring system were the cause of the observed 0.0267AU wide gap located at 0.4AU. Only one location of a moon at 0.63AU (corresponding
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8d8bb289e63e07ea9096102e3778161
http://arxiv.org/abs/1902.09285
http://arxiv.org/abs/1902.09285
Autor:
Phil J. Sutton
Saturns F-ring is a unique, narrow ring that lies (radially) close to the tidally disruptive Roche limit of water ice for Saturn. Significant work has been done that shows it to be one of the most dynamic places in the Solar System. Aggregates that a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e447ea3fb9a29a592700fa251078eff3
Autor:
Feo V. Kusmartsev, Phil J. Sutton
Saturns rings are known to show remarkable real time variability in their structure. Many of which can be associated to interactions with nearby moons and moonlets. Possibly the most interesting and dynamic place in the rings, probably in the whole S
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::69a5c043bba0b68490b7b329536fbed5
http://arxiv.org/abs/1609.01086
http://arxiv.org/abs/1609.01086
Autor:
Feo V. Kusmartsev, Phil J. Sutton
Saturn's rings, reminiscent of an early Solar system present a unique opportunity to investigate experimentally some mechanisms thought to be responsible for planet and planetesimal formation in protoplanetary discs. Here, we extended the comparison
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f815777b0bcf1212dbea371f0a4131f