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Broschiert. Zustand: Gut. 363 Seiten Das hier angebotene Buch stammt aus einer teilaufgelösten wissenschaftlichen Bibliothek und trägt die entsprechenden Kennzeichnungen (Rückenschild, Instituts-Stempel.). Schnitt und Einband sind etwas staubschmutzig; Einbandkanten sind leicht bestossen; der Buchzustand ist ansonsten ordentlich und dem Alter entsprechend gut. Sprache: Englisch Gewicht in Gramm: 530.…

Softcover. 183 Seiten. 8°. Originalbroschur. Gutes Ex. Mit Reihenverzeichnis. -- Bitte Portokosten außerhalb EU erfragen! / Please ask for postage costs outside EU! / S ' il vous plait demander des frais de port en dehors de l ' UE! // Bitte beachten Sie auch unsere Fotos! / Please also note our photos! / Veuillez noter nos photos -- Wenn es draußen stürmt, können Sie es sich mit einem guten Buch gemütlich machen und ein warmes Getränk dazu genießen. Bei uns finden Sie die passende Lektüre! -- Wir kaufen Ihre werthaltigen Bücher! K21699-203249.…

Softcover. Zustand: Gut. Ex-library with stamp and library-signature. GOOD condition, some traces of use. C-02441 3540085327 Sprache: Englisch Gewicht in Gramm: 550.

Zustand: New. In English.

Zustand: New. In English.

Broschiert. Zustand: Gut. 329 Seiten; Das hier angebotene Buch stammt aus einer teilaufgelösten Bibliothek und kann die entsprechenden Kennzeichnungen aufweisen (Rückenschild, Instituts-Stempel.); der Buchzustand ist ansonsten ordentlich und dem Alter entsprechend gut. In ENGLISCHER Sprache. Sprache: Englisch Gewicht in Gramm: 570. …

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Starting in 1995 numerical modeling of the Earth's dynamo has ourished with remarkable success. Direct numerical simulation of convection-driven MHD- ow in a rotating spherical shell show magnetic elds that resemble the geomagnetic eld in many respects: they are dominated by the axial dipole of approximately the right strength, they show spatial power spectra similar to that of Earth, and the magnetic eld morphology and the temporal var- tion of the eld resembles that of the geomagnetic eld (Christensen and Wicht 2007). Some models show stochastic dipole reversals whose details agree with what has been inferred from paleomagnetic data (Glatzmaier and Roberts 1995; Kutzner and Christensen 2002; Wicht 2005). While these models represent direct numerical simulations of the fundamental MHD equations without parameterized induction effects, they do not match actual pla- tary conditions in a number of respects. Speci cally, they rotate too slowly, are much less turbulent, and use a viscosity and thermal diffusivity that is far too large in comparison to magnetic diffusivity. Because of these discrepancies, the success of geodynamo models may seem surprising. In order to better understand the extent to which the models are applicable to planetary dynamos, scaling laws that relate basic properties of the dynamo to the fundamental control parameters play an important role. In recent years rst attempts have been made to derive such scaling laws from a set of numerical simulations that span the accessible parameter space (Christensen and Tilgner 2004; Christensen and Aubert 2006).…

Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Starting in 1995 numerical modeling of the Earth's dynamo has ourished with remarkable success. Direct numerical simulation of convection-driven MHD- ow in a rotating spherical shell show magnetic elds that resemble the geomagnetic eld in many respects: they are dominated by the axial dipole of approximately the right strength, they show spatial power spectra similar to that of Earth, and the magnetic eld morphology and the temporal var- tion of the eld resembles that of the geomagnetic eld (Christensen and Wicht 2007). Some models show stochastic dipole reversals whose details agree with what has been inferred from paleomagnetic data (Glatzmaier and Roberts 1995; Kutzner and Christensen 2002; Wicht 2005). While these models represent direct numerical simulations of the fundamental MHD equations without parameterized induction effects, they do not match actual pla- tary conditions in a number of respects. Speci cally, they rotate too slowly, are much less turbulent, and use a viscosity and thermal diffusivity that is far too large in comparison to magnetic diffusivity. Because of these discrepancies, the success of geodynamo models may seem surprising. In order to better understand the extent to which the models are applicable to planetary dynamos, scaling laws that relate basic properties of the dynamo to the fundamental control parameters play an important role. In recent years rst attempts have been made to derive such scaling laws from a set of numerical simulations that span the accessible parameter space (Christensen and Tilgner 2004; Christensen and Aubert 2006).…

Zustand: Sehr gut. Zustand: Sehr gut | Seiten: 436 | Sprache: Englisch | Produktart: Bücher | Starting in 1995 numerical modeling of the Earth¿s dynamo has ourished with remarkable success. Direct numerical simulation of convection-driven MHD- ow in a rotating spherical shell show magnetic elds that resemble the geomagnetic eld in many respects: they are dominated by the axial dipole of approximately the right strength, they show spatial power spectra similar to that of Earth, and the magnetic eld morphology and the temporal var- tion of the eld resembles that of the geomagnetic eld (Christensen and Wicht 2007). Some models show stochastic dipole reversals whose details agree with what has been inferred from paleomagnetic data (Glatzmaier and Roberts 1995; Kutzner and Christensen 2002; Wicht 2005). While these models represent direct numerical simulations of the fundamental MHD equations without parameterized induction effects, they do not match actual pla- tary conditions in a number of respects. Speci cally, they rotate too slowly, are much less turbulent, and use a viscosity and thermal diffusivity that is far too large in comparison to magnetic diffusivity. Because of these discrepancies, the success of geodynamo models may seem surprising. In order to better understand the extent to which the models are applicable to planetary dynamos, scaling laws that relate basic properties of the dynamo to the fundamental control parameters play an important role. In recent years rst attempts have been made to derive such scaling laws from a set of numerical simulations that span the accessible parameter space (Christensen and Tilgner 2004; Christensen and Aubert 2006).…

Paperback. Zustand: Brand New. 436 pages. 9.25x6.10x1.03 inches. In Stock.

Hardcover. Zustand: Brand New. 1st edition. 430 pages. 9.29x0.87x0.31 inches. In Stock.

Hardcover. Zustand: Gut bis sehr gut. 1. Auflage. "Unzerreissbares Bilderbuch" 8 Pappseiten , selten. Um 1940 erschienen. J. P. Werth (illustrator).

Zustand: gut. The Origin and Dynamics of Solar Magnetism (Space Sciences Series of ISSI, 32, Band 144) In englischer Sprache. pages.

Zustand: Sehr gut. Zustand: Sehr gut | Seiten: 370 | Sprache: Englisch | Produktart: Bücher | Keine Beschreibung verfügbar.

62 (2) Seiten auf kräftigem matten Kunstdruckpapier; durchgehend teils farbig, teils original-farblithographisch bebildert. - Farbig illustrierter Original-Halbleineneinband mit Deckeltitel, Rundum-Rotschnitt; gr.-4to.(ca. 32 x 24 cm). ~~~ 1. AUFLAGE, GROSSFORMATIGE GEBUNDENE ORIGINALAUSGABE. - Leinenrücken stärker-, Hinterdeckel leicht-, Vorderdeckel gering fleckig; Einbandkanten leicht berieben; ansonsten sehr gutes Exemplar. …

Broschur. Zustand: Gut. Ecken/Kanten berieben, hinterer Buchdeckel und Seiten vereinzelt mit Altersflecken! Rar! Geschichte von Kindern, die sich beim Beerensammeln in Tiere verwandeln. In deutscher Sprache. 20 pages. 20 x 26 cm.

Couverture souple. Zustand: bon. R260269622: 1983. In-8. Broché. Très bon état, Couv. convenable, Dos satisfaisant, Intérieur frais. 329 pages. . . . Classification Dewey : 420-Langue anglaise. Anglo-saxon.

Amsterdam, North-Holland [Elsevier Science Publishers], 1993. Thick 8vo (22.4 x 15.2 cm). xxxiv, 615 pp.; several photos, numerous text figures. Original printed cloth. = A rarely seen publication. The conference was attended by 46 physicists, and eight lecturers giving eight courses. Next to a course on Astrophysical fluid dynamics, they include Hydrodynamic turbulence, Generic instabilities and nonlinear dynamics, Magnetohydrodynamic turbulence, Dynamo theory, Thermal convection and penetration, Linear adiabatic stellar pulsation, and Instabilities and turbulence in rotating stars. Stamps on front free endpaper recto, half-title, and title; lightly cocked; small bump to lower edge, affecting a few leaves; otherwise a very good, clean copy.…