By De-Zheng Sun, Frank Bryan

Published by means of the yankee Geophysical Union as a part of the Geophysical Monograph Series.

Climate Dynamics: Why Does weather Vary? offers the key weather phenomena in the weather process to underscore the efficiency of dynamics in giving upward push to weather switch and variability. those phenomena contain deep convection over the Indo-Pacific hot pool and its planetary-scale association: the Madden-Julian Oscillation, the monsoons, the El Nino-Southern Oscillation, the Pacific Decadal Oscillation, and the low-frequency variability of extratropical circulations. the amount additionally has a bankruptcy concentrating on the dialogue of the factors of the hot melting of Arctic sea ice and a bankruptcy dedicated to the dialogue of the motives of modern alterations within the frequency and depth of tropical cyclones. On each one subject, the elemental fabric of weather dynamics is roofed to assist the certainty of the vanguard study, making the amount obtainable to a vast spectrum of readers.

The quantity highlights include

  • Diabatic and nonlinear points of the El Nino-Southern Oscillation
  • Causes of sea ice melting within the Arctic
  • Impact of world warming on tropical cyclone activity
  • Origins of the Pacific Decadal Oscillation
  • Causes of weather variability of Asian monsoons

The quantity may be of specific curiosity to graduate scholars and younger researchers in atmospheric and oceanic sciences and similar disciplines akin to geology and geography. The ebook may also be an excellent learn should you have a extra common curiosity within the Earth's weather and why it varies.


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Additional resources for Climate Dynamics: Why Does Climate Vary?

Sample text

The same analysis approach is applied to the daily NCEP/ NCAR reanalysis data. Here the negative OLR is used to represent the convection and a total of 25 strong northward propagation cases are selected. The following BSISO features derived from the model are confirmed by the observational data. (1) A new convection is initiated over the western equatorial Indian Ocean, which then moves to the eastern equatorial Indian Ocean along the equator. (2) After moving to the eastern equatorial Indian Ocean around 908E, the convection begins to move northward toward the northern Bay of Bengal.

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Iga, T. Nasuno, and M. Satoh (2005), A global cloud-resolving simulation: Preliminary results from an aqua planet experiment, Geophys. Res. 1029/2005GL022459. Tripoli, G. , and W. R. Cotton (1989), Numerical study of an observed orogenic mesoscale convective system. Part 1: Simulated genesis and comparison with observations, Mon. , 117, 273 – 304. Tung, W. , and M. Yanai (2002a), Convective momentum transport observed during the TOGA COARE IOP. Part I: General features, J. Atmos. , 59, 1857 – 1871.

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