Geophysik II / Geophysics II

1. Front Matter

   Pages II-VIII

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2. Dynamic Meteorology

   • A. Eliassen, E. Kleinschmidt Jr.

   Pages 1-154

3. Strahlung in der unteren Atmosphäre

   • Fritz Möller

   Pages 155-253

4. Vision through the Atmosphere

   • W. E. K. Middleton

   Pages 254-287

5. Polarization of Skylight

   • Zdeněk Sekera

   Pages 288-328

6. Diffusion des radiations par les gouttes d’eau en suspension dans l’atmosphère

   • J. Bricard

   Pages 329-369

7. Ozon in der Erdatmosphäre

   • H. K. Paetzold, E. Regener

   Pages 370-426

8. Geophysical Aspects of Meteors

   • A. C. B. Lovell

   Pages 427-454

9. Sound Propagation in Air

   • Everett F. Cox

   Pages 455-478

10. The Physics of Clouds

    • F. H. Ludlam, B. J. Mason

    Pages 479-540

11. Atmosphärische Elektrizität

    • R. Mühleisen

    Pages 541-607

12. Oceanography

    • H. U. Sverdrup

    Pages 608-670

13. Oberflächen-Wellen des Meeres

    • Hans Ulrich Roll

    Pages 671-733

14. Gezeitenkräfte

    • Julius Bartels

    Pages 734-774

15. Tides of the Solid Earth

    • Rudolf Tomaschek

    Pages 775-845

16. Flutwellen und Gezeiten des Wassers

    • A. Defant

    Pages 846-927

17. Atmosphärische Gezeiten

    • W. Kertz

    Pages 928-981

18. Physical Volcanology

    • S. Sakuma, T. Nagata

    Pages 982-1011

19. Back Matter

    Pages 1012-1046

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45 downwards because (j on the average increases with height; but this conclusion does not follow from (18.3) when the dependency of Kc upon ~o is taken into consideration. s 2 ERTELl and PRIESTLEY and SWINBANK have shown that the upward eddy­ flux of sensible heat must be larger than indicated by (18.3), because this formula does not account for the fact that rising eddies are systematically warmer than sinking eddies because of the effect of buoyancy. The reader is referred to the reviews by SUTTON [22], [23] and PRIESTLEY and SHEP­ PARD [15) for further details concerning eddy-flux of heat and turbulent diffusion. 19. RICHARDSON'S criterion. The right-hand side of (15.10) represents the rate of production of eddy energy. The last term represents energy loss by dissipation; in order that the eddy energy shall be maintained, it is therefore necessary that P div V" - (! V" v" . grad. v > O.

• Wellen
• atmosphere
• density
• diffraction
• diffusion
• dynamics
• electricity
• energy
• geophysics
• gravitation
• heat
• hydrodynamics
• physics
• radiation
• wave

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