Surface temperature dependence of tropical cyclone‐permitting simulations in a spherical model with uniform thermal forcing
Tropical cyclone (TC)‐permitting general circulation model simulations are performed with spherical geometry and uniform thermal forcing, including uniform sea surface temperature (SST) and insolation. The dependence of the TC number and TC intensity on SST is examined in a series of simulations wit...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Merlis, Timothy M [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2016 |
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| Rechteinformationen: |
Nutzungsrecht: © 2016. American Geophysical Union. All Rights Reserved. |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Geophysical research letters - Washington, DC : Union, 1974, 43(2016), 6, Seite 2859-2865 |
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| Übergeordnetes Werk: |
volume:43 ; year:2016 ; number:6 ; pages:2859-2865 |
| Links: |
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| DOI / URN: |
10.1002/2016GL067730 |
|---|
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OLC1972638025 |
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| 520 | |a Tropical cyclone (TC)‐permitting general circulation model simulations are performed with spherical geometry and uniform thermal forcing, including uniform sea surface temperature (SST) and insolation. The dependence of the TC number and TC intensity on SST is examined in a series of simulations with varied SST. The results are compared to corresponding simulations with doubly periodic f ‐plane geometry, rotating radiative convective equilibrium. The turbulent equilibria in simulations with spherical geometry have an inhomogenous distribution of TCs with the density of TCs increasing from low to high latitudes. The preferred region of TC genesis is the subtropics, but genesis shifts poleward and becomes less frequent with increasing SST. Both rotating radiative convective equilibrium and spherical geometry simulations have decreasing TC number and increasing TC intensity as SST is increased. SST dependence of TCs assessed with uniform SST GCM simulations Spherical geometry allows TC poleward drift Results are broadly similar to rotating radiative convective equilibrium | ||
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| 650 | 4 | |a climate | |
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| 650 | 4 | |a Temperature | |
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| 650 | 4 | |a Dependence | |
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| 700 | 1 | |a Held, Isaac M |4 oth | |
| 700 | 1 | |a Zhao, Ming |4 oth | |
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10.1002/2016GL067730 doi PQ20160430 (DE-627)OLC1972638025 (DE-599)GBVOLC1972638025 (PRQ)p950-9c63e2e20aacb2d029854c5384fbe7d7185d1090b7f5de1980d03ed7b34e23650 (KEY)0026932820160000043000602859surfacetemperaturedependenceoftropicalcyclonepermi DE-627 ger DE-627 rakwb eng 550 DNB 38.70 bkl Merlis, Timothy M verfasserin aut Surface temperature dependence of tropical cyclone‐permitting simulations in a spherical model with uniform thermal forcing 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Tropical cyclone (TC)‐permitting general circulation model simulations are performed with spherical geometry and uniform thermal forcing, including uniform sea surface temperature (SST) and insolation. The dependence of the TC number and TC intensity on SST is examined in a series of simulations with varied SST. The results are compared to corresponding simulations with doubly periodic f ‐plane geometry, rotating radiative convective equilibrium. The turbulent equilibria in simulations with spherical geometry have an inhomogenous distribution of TCs with the density of TCs increasing from low to high latitudes. The preferred region of TC genesis is the subtropics, but genesis shifts poleward and becomes less frequent with increasing SST. Both rotating radiative convective equilibrium and spherical geometry simulations have decreasing TC number and increasing TC intensity as SST is increased. SST dependence of TCs assessed with uniform SST GCM simulations Spherical geometry allows TC poleward drift Results are broadly similar to rotating radiative convective equilibrium Nutzungsrecht: © 2016. American Geophysical Union. All Rights Reserved. climate tropical cyclones Temperature Cyclones Dependence Geometry Equilibrium Zhou, Wenyu oth Held, Isaac M oth Zhao, Ming oth Enthalten in Geophysical research letters Washington, DC : Union, 1974 43(2016), 6, Seite 2859-2865 (DE-627)129095109 (DE-600)7403-2 (DE-576)01443122X 0094-8276 nnns volume:43 year:2016 number:6 pages:2859-2865 http://dx.doi.org/10.1002/2016GL067730 Volltext http://onlinelibrary.wiley.com/doi/10.1002/2016GL067730/abstract http://search.proquest.com/docview/1782348384 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_47 GBV_ILN_62 GBV_ILN_154 GBV_ILN_601 GBV_ILN_2279 38.70 AVZ AR 43 2016 6 2859-2865 |
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10.1002/2016GL067730 doi PQ20160430 (DE-627)OLC1972638025 (DE-599)GBVOLC1972638025 (PRQ)p950-9c63e2e20aacb2d029854c5384fbe7d7185d1090b7f5de1980d03ed7b34e23650 (KEY)0026932820160000043000602859surfacetemperaturedependenceoftropicalcyclonepermi DE-627 ger DE-627 rakwb eng 550 DNB 38.70 bkl Merlis, Timothy M verfasserin aut Surface temperature dependence of tropical cyclone‐permitting simulations in a spherical model with uniform thermal forcing 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Tropical cyclone (TC)‐permitting general circulation model simulations are performed with spherical geometry and uniform thermal forcing, including uniform sea surface temperature (SST) and insolation. The dependence of the TC number and TC intensity on SST is examined in a series of simulations with varied SST. The results are compared to corresponding simulations with doubly periodic f ‐plane geometry, rotating radiative convective equilibrium. The turbulent equilibria in simulations with spherical geometry have an inhomogenous distribution of TCs with the density of TCs increasing from low to high latitudes. The preferred region of TC genesis is the subtropics, but genesis shifts poleward and becomes less frequent with increasing SST. Both rotating radiative convective equilibrium and spherical geometry simulations have decreasing TC number and increasing TC intensity as SST is increased. SST dependence of TCs assessed with uniform SST GCM simulations Spherical geometry allows TC poleward drift Results are broadly similar to rotating radiative convective equilibrium Nutzungsrecht: © 2016. American Geophysical Union. All Rights Reserved. climate tropical cyclones Temperature Cyclones Dependence Geometry Equilibrium Zhou, Wenyu oth Held, Isaac M oth Zhao, Ming oth Enthalten in Geophysical research letters Washington, DC : Union, 1974 43(2016), 6, Seite 2859-2865 (DE-627)129095109 (DE-600)7403-2 (DE-576)01443122X 0094-8276 nnns volume:43 year:2016 number:6 pages:2859-2865 http://dx.doi.org/10.1002/2016GL067730 Volltext http://onlinelibrary.wiley.com/doi/10.1002/2016GL067730/abstract http://search.proquest.com/docview/1782348384 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_47 GBV_ILN_62 GBV_ILN_154 GBV_ILN_601 GBV_ILN_2279 38.70 AVZ AR 43 2016 6 2859-2865 |
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10.1002/2016GL067730 doi PQ20160430 (DE-627)OLC1972638025 (DE-599)GBVOLC1972638025 (PRQ)p950-9c63e2e20aacb2d029854c5384fbe7d7185d1090b7f5de1980d03ed7b34e23650 (KEY)0026932820160000043000602859surfacetemperaturedependenceoftropicalcyclonepermi DE-627 ger DE-627 rakwb eng 550 DNB 38.70 bkl Merlis, Timothy M verfasserin aut Surface temperature dependence of tropical cyclone‐permitting simulations in a spherical model with uniform thermal forcing 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Tropical cyclone (TC)‐permitting general circulation model simulations are performed with spherical geometry and uniform thermal forcing, including uniform sea surface temperature (SST) and insolation. The dependence of the TC number and TC intensity on SST is examined in a series of simulations with varied SST. The results are compared to corresponding simulations with doubly periodic f ‐plane geometry, rotating radiative convective equilibrium. The turbulent equilibria in simulations with spherical geometry have an inhomogenous distribution of TCs with the density of TCs increasing from low to high latitudes. The preferred region of TC genesis is the subtropics, but genesis shifts poleward and becomes less frequent with increasing SST. Both rotating radiative convective equilibrium and spherical geometry simulations have decreasing TC number and increasing TC intensity as SST is increased. SST dependence of TCs assessed with uniform SST GCM simulations Spherical geometry allows TC poleward drift Results are broadly similar to rotating radiative convective equilibrium Nutzungsrecht: © 2016. American Geophysical Union. All Rights Reserved. climate tropical cyclones Temperature Cyclones Dependence Geometry Equilibrium Zhou, Wenyu oth Held, Isaac M oth Zhao, Ming oth Enthalten in Geophysical research letters Washington, DC : Union, 1974 43(2016), 6, Seite 2859-2865 (DE-627)129095109 (DE-600)7403-2 (DE-576)01443122X 0094-8276 nnns volume:43 year:2016 number:6 pages:2859-2865 http://dx.doi.org/10.1002/2016GL067730 Volltext http://onlinelibrary.wiley.com/doi/10.1002/2016GL067730/abstract http://search.proquest.com/docview/1782348384 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_47 GBV_ILN_62 GBV_ILN_154 GBV_ILN_601 GBV_ILN_2279 38.70 AVZ AR 43 2016 6 2859-2865 |
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10.1002/2016GL067730 doi PQ20160430 (DE-627)OLC1972638025 (DE-599)GBVOLC1972638025 (PRQ)p950-9c63e2e20aacb2d029854c5384fbe7d7185d1090b7f5de1980d03ed7b34e23650 (KEY)0026932820160000043000602859surfacetemperaturedependenceoftropicalcyclonepermi DE-627 ger DE-627 rakwb eng 550 DNB 38.70 bkl Merlis, Timothy M verfasserin aut Surface temperature dependence of tropical cyclone‐permitting simulations in a spherical model with uniform thermal forcing 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Tropical cyclone (TC)‐permitting general circulation model simulations are performed with spherical geometry and uniform thermal forcing, including uniform sea surface temperature (SST) and insolation. The dependence of the TC number and TC intensity on SST is examined in a series of simulations with varied SST. The results are compared to corresponding simulations with doubly periodic f ‐plane geometry, rotating radiative convective equilibrium. The turbulent equilibria in simulations with spherical geometry have an inhomogenous distribution of TCs with the density of TCs increasing from low to high latitudes. The preferred region of TC genesis is the subtropics, but genesis shifts poleward and becomes less frequent with increasing SST. Both rotating radiative convective equilibrium and spherical geometry simulations have decreasing TC number and increasing TC intensity as SST is increased. SST dependence of TCs assessed with uniform SST GCM simulations Spherical geometry allows TC poleward drift Results are broadly similar to rotating radiative convective equilibrium Nutzungsrecht: © 2016. American Geophysical Union. All Rights Reserved. climate tropical cyclones Temperature Cyclones Dependence Geometry Equilibrium Zhou, Wenyu oth Held, Isaac M oth Zhao, Ming oth Enthalten in Geophysical research letters Washington, DC : Union, 1974 43(2016), 6, Seite 2859-2865 (DE-627)129095109 (DE-600)7403-2 (DE-576)01443122X 0094-8276 nnns volume:43 year:2016 number:6 pages:2859-2865 http://dx.doi.org/10.1002/2016GL067730 Volltext http://onlinelibrary.wiley.com/doi/10.1002/2016GL067730/abstract http://search.proquest.com/docview/1782348384 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_47 GBV_ILN_62 GBV_ILN_154 GBV_ILN_601 GBV_ILN_2279 38.70 AVZ AR 43 2016 6 2859-2865 |
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10.1002/2016GL067730 doi PQ20160430 (DE-627)OLC1972638025 (DE-599)GBVOLC1972638025 (PRQ)p950-9c63e2e20aacb2d029854c5384fbe7d7185d1090b7f5de1980d03ed7b34e23650 (KEY)0026932820160000043000602859surfacetemperaturedependenceoftropicalcyclonepermi DE-627 ger DE-627 rakwb eng 550 DNB 38.70 bkl Merlis, Timothy M verfasserin aut Surface temperature dependence of tropical cyclone‐permitting simulations in a spherical model with uniform thermal forcing 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Tropical cyclone (TC)‐permitting general circulation model simulations are performed with spherical geometry and uniform thermal forcing, including uniform sea surface temperature (SST) and insolation. The dependence of the TC number and TC intensity on SST is examined in a series of simulations with varied SST. The results are compared to corresponding simulations with doubly periodic f ‐plane geometry, rotating radiative convective equilibrium. The turbulent equilibria in simulations with spherical geometry have an inhomogenous distribution of TCs with the density of TCs increasing from low to high latitudes. The preferred region of TC genesis is the subtropics, but genesis shifts poleward and becomes less frequent with increasing SST. Both rotating radiative convective equilibrium and spherical geometry simulations have decreasing TC number and increasing TC intensity as SST is increased. SST dependence of TCs assessed with uniform SST GCM simulations Spherical geometry allows TC poleward drift Results are broadly similar to rotating radiative convective equilibrium Nutzungsrecht: © 2016. American Geophysical Union. All Rights Reserved. climate tropical cyclones Temperature Cyclones Dependence Geometry Equilibrium Zhou, Wenyu oth Held, Isaac M oth Zhao, Ming oth Enthalten in Geophysical research letters Washington, DC : Union, 1974 43(2016), 6, Seite 2859-2865 (DE-627)129095109 (DE-600)7403-2 (DE-576)01443122X 0094-8276 nnns volume:43 year:2016 number:6 pages:2859-2865 http://dx.doi.org/10.1002/2016GL067730 Volltext http://onlinelibrary.wiley.com/doi/10.1002/2016GL067730/abstract http://search.proquest.com/docview/1782348384 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_47 GBV_ILN_62 GBV_ILN_154 GBV_ILN_601 GBV_ILN_2279 38.70 AVZ AR 43 2016 6 2859-2865 |
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550 DNB 38.70 bkl Surface temperature dependence of tropical cyclone‐permitting simulations in a spherical model with uniform thermal forcing climate tropical cyclones Temperature Cyclones Dependence Geometry Equilibrium |
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Surface temperature dependence of tropical cyclone‐permitting simulations in a spherical model with uniform thermal forcing |
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Surface temperature dependence of tropical cyclone‐permitting simulations in a spherical model with uniform thermal forcing |
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Merlis, Timothy M |
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Geophysical research letters |
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10.1002/2016GL067730 |
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surface temperature dependence of tropical cyclone‐permitting simulations in a spherical model with uniform thermal forcing |
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Surface temperature dependence of tropical cyclone‐permitting simulations in a spherical model with uniform thermal forcing |
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Tropical cyclone (TC)‐permitting general circulation model simulations are performed with spherical geometry and uniform thermal forcing, including uniform sea surface temperature (SST) and insolation. The dependence of the TC number and TC intensity on SST is examined in a series of simulations with varied SST. The results are compared to corresponding simulations with doubly periodic f ‐plane geometry, rotating radiative convective equilibrium. The turbulent equilibria in simulations with spherical geometry have an inhomogenous distribution of TCs with the density of TCs increasing from low to high latitudes. The preferred region of TC genesis is the subtropics, but genesis shifts poleward and becomes less frequent with increasing SST. Both rotating radiative convective equilibrium and spherical geometry simulations have decreasing TC number and increasing TC intensity as SST is increased. SST dependence of TCs assessed with uniform SST GCM simulations Spherical geometry allows TC poleward drift Results are broadly similar to rotating radiative convective equilibrium |
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Tropical cyclone (TC)‐permitting general circulation model simulations are performed with spherical geometry and uniform thermal forcing, including uniform sea surface temperature (SST) and insolation. The dependence of the TC number and TC intensity on SST is examined in a series of simulations with varied SST. The results are compared to corresponding simulations with doubly periodic f ‐plane geometry, rotating radiative convective equilibrium. The turbulent equilibria in simulations with spherical geometry have an inhomogenous distribution of TCs with the density of TCs increasing from low to high latitudes. The preferred region of TC genesis is the subtropics, but genesis shifts poleward and becomes less frequent with increasing SST. Both rotating radiative convective equilibrium and spherical geometry simulations have decreasing TC number and increasing TC intensity as SST is increased. SST dependence of TCs assessed with uniform SST GCM simulations Spherical geometry allows TC poleward drift Results are broadly similar to rotating radiative convective equilibrium |
| abstract_unstemmed |
Tropical cyclone (TC)‐permitting general circulation model simulations are performed with spherical geometry and uniform thermal forcing, including uniform sea surface temperature (SST) and insolation. The dependence of the TC number and TC intensity on SST is examined in a series of simulations with varied SST. The results are compared to corresponding simulations with doubly periodic f ‐plane geometry, rotating radiative convective equilibrium. The turbulent equilibria in simulations with spherical geometry have an inhomogenous distribution of TCs with the density of TCs increasing from low to high latitudes. The preferred region of TC genesis is the subtropics, but genesis shifts poleward and becomes less frequent with increasing SST. Both rotating radiative convective equilibrium and spherical geometry simulations have decreasing TC number and increasing TC intensity as SST is increased. SST dependence of TCs assessed with uniform SST GCM simulations Spherical geometry allows TC poleward drift Results are broadly similar to rotating radiative convective equilibrium |
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Surface temperature dependence of tropical cyclone‐permitting simulations in a spherical model with uniform thermal forcing |
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http://dx.doi.org/10.1002/2016GL067730 http://onlinelibrary.wiley.com/doi/10.1002/2016GL067730/abstract http://search.proquest.com/docview/1782348384 |
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Zhou, Wenyu Held, Isaac M Zhao, Ming |
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