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Condizione: good. A copy that has been read, remains in good condition. All pages are intact, and the cover is intact. The spine and cover show signs of wear. Pages can include notes and highlighting and show signs of wear, and the copy can include "From the library of" labels or previous owner inscriptions. 100% GUARANTEE! Shipped with delivery confirmation, if you're not satisfied with purchase please return item! Ships via media mail.…

Condizione: New. In English.

Softcover. Condizione: Gut. Ehem. Bibliotheksexemplar mit Signatur und Stempel. GUTER Zustand, ein paar Gebrauchsspuren. Ex-library with stamp and library-signature. GOOD condition, some traces of use. C-01576 3540574212 Sprache: Englisch Gewicht in Gramm: 550.

paperback. Condizione: New. In shrink wrap. Looks like an interesting title.

Condizione: New.

Condizione: New.

Condizione: As New. Unread book in perfect condition.

Condizione: As New. Unread book in perfect condition.

Condizione: As New. Unread book in perfect condition.

Condizione: New. In English.

Condizione: New.

Condizione: New. pp. 64.

Taschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - Vertical temperature profiles of the Venus atmosphere up to 80 km height were calculated in a time dependent model. A steady state of the atmospheric profiles was reached by numerical intergration from an arbitrary initial distribution of temperature by assuming some atmospheric parameters as surface pressure, planetary albedo etc. The time-rate-of-change of temperature was determined by the vertical divergence of the following fluxes: solar insolation, net infrared radiation of the atmosphere and the ground surface, and sensible heat. The radiation calculation was based on the absorption bands of carbon dioxide and water vapor from the near to the far infrared region of the spectrum. Absorption by clouds was taken into account in parameterized form. Atmospheric profiles were calculated as a function of water vapor content, height and absorptivity of the cloud layer, surface pressure, eddy diffusion coefficient, planetaryalbedo, latitude, and time of day. It appeared, that the lower layers of a pure carbon dioxide atmosphere are convective with an adiabatic lapse rate of temperature. The lapse rate of a carbon dioxide atmosphere with some additional water va por and thus strong absorption of solar energy is practically adiabatic due to the downward transport of sensible heat. Comparison with direct measurements indicates that the atmosphere below the c10ud level 4 is likely to contain water vapor. A mixing ratio of 10- is sufficient to explain the observed temperature profile.…

Paperback. Condizione: Brand New. spiral-bound edition. 64 pages. German language. 10.99x8.27x0.15 inches. In Stock.

Paperback. Condizione: Very Good. Dust Jacket may NOT BE INCLUDED.CDs may be missing. SHIPS FROM MULTIPLE LOCATIONS. book.

Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. The theory of Dirichlet forms has witnessed recently somevery important developments both in theoretical foundationsand in applications (stochasticprocesses, quantum fieldtheory, composite materials.). It was therefore felttimely to have on this subje. …

Taschenbuch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Vertical temperature profiles of the Venus atmosphere up to 80 km height were calculated in a time dependent model. A steady state of the atmospheric profiles was reached by numerical intergration from an arbitrary initial distribution of temperature by assuming some atmospheric parameters as surface pressure, planetary albedo etc. The time-rate-of-change of temperature was determined by the vertical divergence of the following fluxes: solar insolation, net infrared radiation of the atmosphere and the ground surface, and sensible heat. The radiation calculation was based on the absorption bands of carbon dioxide and water vapor from the near to the far infrared region of the spectrum. Absorption by clouds was taken into account in parameterized form. Atmospheric profiles were calculated as a function of water vapor content, height and absorptivity of the cloud layer, surface pressure, eddy diffusion coefficient, planetaryalbedo, latitude, and time of day. It appeared, that the lower layers of a pure carbon dioxide atmosphere are convective with an adiabatic lapse rate of temperature. The lapse rate of a carbon dioxide atmosphere with some additional water va por and thus strong absorption of solar energy is practically adiabatic due to the downward transport of sensible heat. Comparison with direct measurements indicates that the atmosphere below the c10ud level 4 is likely to contain water vapor. A mixing ratio of 10- is sufficient to explain the observed temperature profile. 64 pp. Deutsch.…

Condizione: New. Print on Demand pp. 64 12:B&W 8.5 x 11 in or 280 x 216 mm Perfect Bound on White w/Gloss Lam.

Condizione: New. PRINT ON DEMAND pp. 64.

Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. und Problemstellung.- Fakten und Voraussetzungen.- 2.1 Elemente der Umlaufbahn, Rotation und Dimension des Planeten Venus.- 2.2 Zusammensetzung der Atmosphaere.- 2.3 Wolken.- 2.4 Temperatur und Druck an der Oberflaeche.- 2.5 Voraussetzungen.- Theorie.- 3.1 St.…

Taschenbuch. Condizione: Neu. This item is printed on demand - Print on Demand Titel. Neuware -und Problemstellung.- Fakten und Voraussetzungen.- 2.1 Elemente der Umlaufbahn, Rotation und Dimension des Planeten Venus.- 2.2 Zusammensetzung der Atmosphäre.- 2.3 Wolken.- 2.4 Temperatur und Druck an der Oberfläche.- 2.5 Voraussetzungen.- Theorie.- 3.1 Strahlungsströme.- 3.2 Wärmetransport.- Absorptionsfunktionen.- 4.1 Absorptionsspektren von Kohlendioxid und Wasserdampf.- 4.2 Absorptionsmodelle.- 4.3 Auswertung der Absorptionsdaten.- 4.4 Berechnung der Absorptionsfunktionen.- 4.5 Temperatur- und Druckkorrektur.- 4.6 Absorption von Gasgemischen.- 4.7 Interpolations - und Extrapolationsverfahren.- Modell und Methode.- 5.1 Modell.- 5.2 Anfangsbedingungen.- 5.3 Randbedingungen.- 5.4 Rechenmethode.- Fehlerbetrachtung.- Ergebnisse.- 7.1 Wasserdampfgehalt.- 7.2 Wolken.- 7.3 Bodendruck, Diffusionskoeffizient, Albedo, Randbedingungen.- 7.4 Meridionale und tageszeitliche Temperaturunterschiede.- Vergleich mit anderen Ergebnissen.- Allgemeine Zirkulation der Venusatmosphäre.- Zusammenfassung.- Summary.- Symbole und Abkürzungen.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 64 pp. Deutsch.…

Taschenbuch. Condizione: Neu. Temperaturberechnung der Venusatmosphäre bis 80 km Höhe aufgrund Solarer und Thermischer Strahlungsströme Sowie Konvektiver und Turbulenter Wärmetransporte | E. Roeckner | Taschenbuch | 58 S. | Deutsch | Springer | EAN 9783540057765 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu Print on Demand. …