the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
On the quasi-steady vorticity balance in the mature stage of hurricane Irma (2017)
Michiel L. J. Baatsen
Aarnout J. van Delden
Abstract. Tropical cyclone (TC) intensification is a process depending on many factors related to the thermodynamical state and environmental influences. It remains a challenge to accurately model TC intensity due to the role of unsteady features like deep convective bursts, boundary layer dynamics and eddy processes. The impermeability theorem for potential vorticity substance, PVS, on isentropic surfaces provides a way to analyze the absolute vorticity structure and tendency in TCs. We will examine this theorem in a numerical simulation of hurricane Irma (2017) near lifetime-peak intensity. Hurricane Irma was a very intense hurricane that persisted as a category five hurricane on the Saffir-Simpson intensity scale for three consecutive days, the longest for any Atlantic hurricane since satellite observations. During this period the intensity of Irma was remarkably constant. According to the impermeability theorem, the radially outward vorticity flux due to divergence above the atmospheric boundary layer must be compensated by an equally strong radially inward vorticity flux due to the effect of diabatic heating in the presence of vertical wind shear. The model results agree with this theorem and we find a strong anticorrelation between the advective and diabatic components of the radial vorticity flux. The impact of parametrized turbulence on the vorticity balance is found to be weak and does not explain the residual flux that would otherwise close the vorticity balance.
- Preprint
(3285 KB) - Metadata XML
- BibTeX
- EndNote
Jasper de Jong et al.
Status: open (until 06 Oct 2023)
-
RC1: 'Comment on egusphere-2023-1259', Anonymous Referee #1, 21 Aug 2023
reply
Please see the attached file.
-
RC2: 'Comment on egusphere-2023-1259', Anonymous Referee #1, 21 Aug 2023
reply
I appologize no reference in my specific comment#2. I revised the comment as follows:
L49-50: Did the authors quantitatively confirm the radiative cooling for the warm core extension? Previous studies indicated that adiabatic processes associated with subsidence in the eye can be a major contribution to the development of the warming in the eye (e.g., Stern and Zhang, 2013; Ohno and Satoh, 2015).
Reference
Ohno, T., and M. Satoh, 2015: On the warm core of a tropical cyclone formed near the tropopause. J. Atmos. Sci., 72, 551–571, doi:10.1175/JAS-D-14-0078.1.
Stern, D. P., and F. Zhang, 2013: Howdoes the eyewarm? Part I:Apotential temperature budget analysis of an idealized tropical cyclone. J. Atmos. Sci., 70, 73–90, doi:10.1175/JAS-D-11-0329.1.
Citation: https://doi.org/10.5194/egusphere-2023-1259-RC2 -
RC3: 'Comment on egusphere-2023-1259', Anonymous Referee #2, 28 Sep 2023
reply
Please see attachment
-
RC4: 'Comment on egusphere-2023-1259', Anonymous Referee #3, 28 Sep 2023
reply
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-1259/egusphere-2023-1259-RC4-supplement.pdf
Jasper de Jong et al.
Jasper de Jong et al.
Viewed
HTML | XML | Total | BibTeX | EndNote | |
---|---|---|---|---|---|
208 | 59 | 17 | 284 | 3 | 3 |
- HTML: 208
- PDF: 59
- XML: 17
- Total: 284
- BibTeX: 3
- EndNote: 3
Viewed (geographical distribution)
Country | # | Views | % |
---|
Total: | 0 |
HTML: | 0 |
PDF: | 0 |
XML: | 0 |
- 1