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  1. NTU Theses and Dissertations Repository
  2. 理學院
  3. 天文物理研究所
請用此 Handle URI 來引用此文件: http://tdr.lib.ntu.edu.tw/jspui/handle/123456789/35851
完整後設資料紀錄
DC 欄位值語言
dc.contributor.advisor李太楓(Typhoon Lee)
dc.contributor.authorShang-Min Tsaien
dc.contributor.author蔡尚旻zh_TW
dc.date.accessioned2021-06-13T07:47:33Z-
dc.date.available2011-08-22
dc.date.copyright2011-08-22
dc.date.issued2011
dc.date.submitted2011-08-20
dc.identifier.citation[Adrian E. Gill] Atmosphere-Ocean Dynamics, Volume 30 (Academic Press, 1982))
[Burrows et al. 2008] Burrows, A., Budaj, J.,and Hubeny, I. 2008, ApJ, 678, 1436
[Chapman and Lindzen 1970] S. Chapman and R.S. Lindzen (1970). Atmospheric
Tides, D. Reidel Press, Dordrecht, Holland, 200 pp.
[Dobbs-Dixon (2010)] Ian Dobbs-Dixon et al. 2010 ApJ, 710, 139
[Fels and Lindzen(1974)] S. Fels and R.S. Lindzen, Geophys. Fl. Dyn., 6, 149-191
[Fritts] Fritts, D. C., Gravity wave saturation in the middle atmosphere: A review
of theory and observations, Rev. Geophys., 22(3), 275308
[Knutson et al. 2009] Heather A. Knutson et al. 2009 ApJ, 690, 822
[Lindzen (1970a)] R.S. Lindzen , Internal gravity waves in atmospheres with realistic
dissipation and temperature. I. Mathematical development and propagation of
waves into the thermosphere. Geophys. Fluid Dynamics 1 (1970a), pp. 303355.
[Lindzen (1971)] R.S. Lindzen and D. Blake . Internal gravity waves in atmospheres
with realistic dissipation and temperature: Part II. Thermal tides excited below
the mesopause. Geophys. Fl. Dyn., 2, 31-61.
[Lindzen (1981)] Turbulence and stress due to gravity wave and tidal breakdown.
J. Geophys. Res., 86, 9707-9714.
[Rossow & Williams, 1979] Rossow, W.B., and G.P. Williams, 1979: Large-scale
motion in the Venus stratosphere. J. Atmos Sci., 36, 377-389
[Showman & Polvani, 2011)] Showman, A.P., & Polvani, L.M. 2011, preprint(arXiv:1103.3101v1)
[Thrastarson & Cho 2010] Thrastarson and James Y-K. Cho 2010 ApJ, 716, 144
[Watkin & Cho(2010)] Chris Watkins and J. Y-K. Cho 2010 ApJ, 714, 904
[Zhu 2006] Zhu, Xun Planetary and Space Science, Volume 54, Issue 8, p. 761-773
dc.identifier.urihttp://tdr.lib.ntu.edu.tw/jspui/handle/123456789/35851-
dc.description.abstract迄今已發現的系外行星中,大多數是暴露在強烈的恆星輻射下的巨大氣體行星,而且有可能已被母恆星潮汐鎖定。這些系外行星的3D大氣模擬,和部分觀測結果顯示其赤道區域的大氣有超自轉風的現象,即赤道區域的環流移動的比行星自轉還要快。此現象在太陽系內幾個自轉緩慢的行星,例如金星和泰坦(土衛六)上被觀察到。人們嘗試提出不同的物理機制來解釋赤道區域的超自轉風。我們採用首先由 Fels 和 Lindzen(1974)所提的假設,在金星上的赤道超自轉風的來源是熱潮汐引起的垂直動量傳送。熱潮汐是恆星加熱大氣所驅動的大氣中溫度,密度,壓力,和風速的週期性振盪,熱潮汐的垂直結構基本上就是週期對應於母恆星的大尺度內部重力波。在行星大氣中,在被加熱的區域(波的來源區)所產生的熱潮汐和重力波有往和母恆星視運動相反方向加速的效果,造成超自轉風。我們應用HD 209458b的參數進行線性分析,探討超自轉風的形成和維持。研究的結果指出,當被加熱的區域在環流的中心(垂直方向)附近時,熱潮汐可以解釋超自轉風的動量來源,並且在垂直方向上重新分布大氣中的水平動量。zh_TW
dc.description.abstractThe large majority of exoplanets discovered thus far are gas planets exposed to strong stellar irradiation, and are likely to be tidally locked by their parent stars. Both 3D models and observations of the tidally locked gas giants have suggested the phenomena of equatorial superrotation in the atmosphere; i.e. the equatorial winds blow faster than self rotation of the planets. The phenomena have exhibited in several slow rotating planets such as Venus and Titan. Some mechanisms have been proposed to explain the equatorial superrotation. In our work, we adopt the theory first suggested by Fels and Lindzen (1974), that the equatorial superroatation on Venus resulted from the thermal tides pumping the momentum via vertical transport. Thermal tides are oscillations in temperature, density, pressure, and wind velocity driven by the stellar heating. The vertical structure of thermal tides is basically internal gravity waves with the pattern speed equal to the apparent motion of the parent star. Thermal tides or waves generated in the stellar heating region have the effect of acceleration to the direction opposite to the stellar motion, leading to the maintenance of superrotational winds. A linear analysis is applied to HD209458b to demonstrate the superrotation formation and maintenance. Our model suggests that when the stellar heating is absorbed near the center of the equatorial jet, the superrotation can be explained by thermal tides, which provide the momentum redistribution between different altitudes of the atmosphere.en
dc.description.provenanceMade available in DSpace on 2021-06-13T07:47:33Z (GMT). No. of bitstreams: 1
ntu-100-R97244007-1.pdf: 2062437 bytes, checksum: 77b39dc8a9c387663354a40978ef9a2a (MD5)
Previous issue date: 2011
en
dc.description.tableofcontents1 Introduction 1
2 Linear Model 3
2.1 Equations of Equivalent Gravity Waves . . . . . . . . . . . . . . . . . 3
2.1.1 Basic equations . . . . . . . . . . . . . . . . . . . . . . . . . . 3
2.1.2 Background Structure . . . . . . . . . . . . . . . . . . . . . . 5
2.1.3 Perturbation equations . . . . . . . . . . . . . . . . . . . . . . 9
2.1.4 Dispersion Relation and the Equivalent Depth . . . . . . . . . 11
2.1.5 Equivalent depth and latitudinal wave number in vertical shear
condition . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13
2.1.6 the WKB solutions . . . . . . . . . . . . . . . . . . . . . . . . 13
2.2 Numerical method . . . . . . . . . . . . . . . . . . . . . . . . . . . . 14
2.3 Reynolds stress . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15
2.4 Linear saturation process . . . . . . . . . . . . . . . . . . . . . . . . . 15
2.5 The interaction of waves and the zonal mean flow . . . . . . . . . . . 16
3 Numerical results 18
4 Summary 38
A Eliassen-Palm theorems 39
Bibliography 41
dc.language.isoen
dc.title熱木星上熱潮汐和赤道環流的交互作用zh_TW
dc.titleThe Interaction of Thermal Tides with the Equatorial Winds on Hot Jupitersen
dc.typeThesis
dc.date.schoolyear99-2
dc.description.degree碩士
dc.contributor.coadvisor辜品高(Pin-Gao Gu)
dc.contributor.oralexamcommittee梁茂昌(Mao-Chang Liang)
dc.subject.keyword系外行星,熱木星,大氣,赤道環流,熱潮汐,內部重力波,超自轉風,zh_TW
dc.subject.keywordexoplanet,hot Jupiter,atmospheres,thermal tides,waves,superrotation,en
dc.relation.page42
dc.rights.note有償授權
dc.date.accepted2011-08-20
dc.contributor.author-college理學院zh_TW
dc.contributor.author-dept天文物理研究所zh_TW
顯示於系所單位:天文物理研究所

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