Some Problems in Geophysics
Some Problems in Geophysics
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In our eReader you can find the full English version of the book. Read Some Problems in Geophysics Online - link to read the book on full screen. Our eReader also allows you to upload and read Pdf, Txt, ePub and fb2 books. In the Mini eReder on the page below you can quickly view all pages of the book - Read Book Some Problems in Geophysics
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Report of the Krakatoa Committee of the Royal Society of London (1888). +5 107 14-1 Lecture l4 Turbulence Spectra and Vortex Formation Alexandre Joel Chorin Introduction . It is well knovm that the energy spectnim E(k, t) of a turbulent flow has, for large wave number k, a universal form, i. E. A form common to a variety of flows whose larger scale features have little in common. This fact is often explained by the universal equilibrium hypothesis, well summarized in Batchelor : The range of wa...ve numbers k which contain most of the energy ("the energy containing eddies") can be regarded as a ""? 1/2 definite group, with characteristic velocity u = (u ) ' and Characteristic length 2 » k^^, where u is the velocity vector, the bar under u denotes a vector, the bar above (u ) denotes an appropriate average, and k is a typical wave number in the group. The characteristic time of these eddies is l/n, and the time scale of their decay is u/|3H|; these times are experimentally found to be comparable, and thus this range of k's has no feature resembling an equilibrium.
What to read after Some Problems in Geophysics?
You can find similar books in the "Read Also" column, or choose other free books by J J Stoker to read onlineMoreLess
To quickly assess the difficulty of the text, read a short excerpt:
Report of the Krakatoa Committee of the Royal Society of London (1888). +5 107 14-1 Lecture l4 Turbulence Spectra and Vortex Formation Alexandre Joel Chorin Introduction . It is well knovm that the energy spectnim E(k, t) of a turbulent flow has, for large wave number k, a universal form, i. E. A form common to a variety of flows whose larger scale features have little in common. This fact is often explained by the universal equilibrium hypothesis, well summarized in Batchelor : The range of wa...ve numbers k which contain most of the energy ("the energy containing eddies") can be regarded as a ""? 1/2 definite group, with characteristic velocity u = (u ) ' and Characteristic length 2 » k^^, where u is the velocity vector, the bar under u denotes a vector, the bar above (u ) denotes an appropriate average, and k is a typical wave number in the group. The characteristic time of these eddies is l/n, and the time scale of their decay is u/|3H|; these times are experimentally found to be comparable, and thus this range of k's has no feature resembling an equilibrium.
What to read after Some Problems in Geophysics?
You can find similar books in the "Read Also" column, or choose other free books by J J Stoker to read onlineMoreLess
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