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    Hurricane Superintensity

    Source: Journal of the Atmospheric Sciences:;2003:;Volume( 060 ):;issue: 019::page 2349
    Author:
    Persing, John
    ,
    Montgomery, Michael T.
    DOI: 10.1175/1520-0469(2003)060<2349:HS>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: High spatial and temporal resolution simulations using the Rotunno and Emanuel axisymmetric, cloud-resolving, hurricane model are found to greatly exceed Emanuel?s energetically based upper bound for maximum potential intensity (E-MPI). Using a control simulation similar to that of Rotunno and Emanuel with a sea surface temperature (SST) of 26.13°C, the E-MPI is exceeded after 15 simulation days, after the warming of the eye is able to extend down to the ocean surface. At still higher resolution, the modeled storm greatly exceeds E-MPI more quickly, during initial spinup, and the resulting intensity for the standard numerical and microphysical parameters is found to converge with, respectively, radial and vertical grid spacing of 3.75 km and 312.5 m with maximum tangential winds (Vmax) of ≈90 m s?1. This is notably greater than the energetically based upper bound of Vmax = 55 m s?1. This ?superintensity? occurs only in the presence of an enhancement of low-level eye entropy. The high-entropy air is entrained into the eyewall primarily by a breakdown of an azimuthal vortex sheet at the inner edge of the eyewall. Among the many underlying assumptions of E-MPI, only the violation of the related assumptions that the eyewall is neutral to moist ascent and that no entropy is fluxed from the eye to the eyewall can explain the degree of superintensity observed; other assumptions may be individually violated but their impacts on the intensity estimates are much smaller. The impact of the entrainment of heat from the eye to the eyewall on E-MPI theory is estimated through an ad hoc increase in the effective SST as a way of accounting for a second source of heat. This procedure produces a close estimate of the modeled intensity, but the problem is not closed since the degree of eyewall heating is not known a priori. Published observations and recent three-dimensional, cloud-resolving modeling studies are reviewed that appear to present various aspects of the observed entropy structure and the eye?eyewall interaction of the superintensity mechanism.
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      Hurricane Superintensity

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    http://yetl.yabesh.ir/yetl1/handle/yetl/4159884
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    contributor authorPersing, John
    contributor authorMontgomery, Michael T.
    date accessioned2017-06-09T14:38:20Z
    date available2017-06-09T14:38:20Z
    date copyright2003/10/01
    date issued2003
    identifier issn0022-4928
    identifier otherams-23334.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4159884
    description abstractHigh spatial and temporal resolution simulations using the Rotunno and Emanuel axisymmetric, cloud-resolving, hurricane model are found to greatly exceed Emanuel?s energetically based upper bound for maximum potential intensity (E-MPI). Using a control simulation similar to that of Rotunno and Emanuel with a sea surface temperature (SST) of 26.13°C, the E-MPI is exceeded after 15 simulation days, after the warming of the eye is able to extend down to the ocean surface. At still higher resolution, the modeled storm greatly exceeds E-MPI more quickly, during initial spinup, and the resulting intensity for the standard numerical and microphysical parameters is found to converge with, respectively, radial and vertical grid spacing of 3.75 km and 312.5 m with maximum tangential winds (Vmax) of ≈90 m s?1. This is notably greater than the energetically based upper bound of Vmax = 55 m s?1. This ?superintensity? occurs only in the presence of an enhancement of low-level eye entropy. The high-entropy air is entrained into the eyewall primarily by a breakdown of an azimuthal vortex sheet at the inner edge of the eyewall. Among the many underlying assumptions of E-MPI, only the violation of the related assumptions that the eyewall is neutral to moist ascent and that no entropy is fluxed from the eye to the eyewall can explain the degree of superintensity observed; other assumptions may be individually violated but their impacts on the intensity estimates are much smaller. The impact of the entrainment of heat from the eye to the eyewall on E-MPI theory is estimated through an ad hoc increase in the effective SST as a way of accounting for a second source of heat. This procedure produces a close estimate of the modeled intensity, but the problem is not closed since the degree of eyewall heating is not known a priori. Published observations and recent three-dimensional, cloud-resolving modeling studies are reviewed that appear to present various aspects of the observed entropy structure and the eye?eyewall interaction of the superintensity mechanism.
    publisherAmerican Meteorological Society
    titleHurricane Superintensity
    typeJournal Paper
    journal volume60
    journal issue19
    journal titleJournal of the Atmospheric Sciences
    identifier doi10.1175/1520-0469(2003)060<2349:HS>2.0.CO;2
    journal fristpage2349
    journal lastpage2371
    treeJournal of the Atmospheric Sciences:;2003:;Volume( 060 ):;issue: 019
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
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