Sk thompson (37 resultados)

Brossura. Condición: buono. Volume integro, fresco all'interno, copertina flessibile solo normali segni di usura, foto su richiesta.

First Edition. Near fine copy in the original title-printed stiff card wrappers. Slightest suggestion only of creasing and dust-dulling to the spine bands and panel edges. Remains particularly and uncommonly well-preserved; tight, bright, clean and strong. ; 265 pages; An unread copy with unopened pages; publisher's ads to the rear. 1 Kg.…

First Edition. Near fine copy in the original title-printed stiff card wrappers. Slightest suggestion only of creasing and dust-dulling to the spine bands and panel edges. Remains particularly and uncommonly well-preserved; tight, bright, clean and strong. ; 265 pages; An unread copy with unopened pages; publisher's ads to the rear. 1 Kg.…

Relié. In-8 (15,3 x 23 cm), reliure demi-peau, dos à 5 nerfs, pièce de titre, couverture conservée, 265 pages ; très bon état général. Livraison a domicile (La Poste) ou en Mondial Relay sur simple demande. Bibliothèque Historique.

Paperback. Condición: Very good. First Edition. Paperback. First Edition. 19pp; A bit of loosening, else very good. The Kansan Thompson, a Civil War veteran, was cashiered after court-martial in San Antonio for drunkeness on duty. This document presents the record and Thompson's application for reinstatement, with the endorsement of Kansas's Senators and Congressmen. He presents affidavits from Allen Factor and Carolina July, "Private Seminole Negro Indian scouts," who swear that Thompson wasn't drunk; his horse was merely "very unruly.".…

225x140mm, 265pages, Bel exemplaire. Envoi groupé : les frais de port sont calculés sur le poids total de la commande ; chaque livre supplémentaire coûte donc beaucoup moins cher à expédier. Commandez plusieurs livres et économisez sur le port ! / Combined shipping: postage is charged on the total weight of your order, so each additional book ships at a reduced rate. Order several books from us and save on postage ! / Envois Europe : Droits et taxes inclus - aucun frais à la livraison / Shipments to Europe: Duties and taxes included - no delivery charges.…

Condición: As New. Unread book in perfect condition.

Condición: New.

Condición: New.

Condición: New.

Taschenbuch. Condición: 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. Condición: 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).…

Condición: New. pp. 436.

Condición: 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).…

Condición: New. pp. vi + 430 2009th edition Reprinted from SPACE SCIENCE REVIEWS, 144/1-4, 2009.

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

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

Condición: As New. Unread book in perfect condition.

Hardcover. Condición: Like New. LIKE NEW. SHIPS FROM MULTIPLE LOCATIONS. book.

Condición: As New. Unread book in perfect condition.

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

Gebunden. Condición: New. This book discusses adaptive sampling designs which are used in surveys where data collection requires modification as a result of observations made during the process. The strategies detailed in the book offer solutions to the long-standing problem of esti.

Couverture souple. Condición: bon. R300261363: 1938. in-8. Broché. Etat d'usage, Couv. défraîchie, Dos à nerfs, Intérieur acceptable. Paris, Payot, 1938, in 8, broché, 265 pp. . . . Classification Dewey : 355.343-Services secrets, espionage.

rilegato copertina rigida. Condición: Good. Payot, 1938. Collana Bibliotheque Historique. Traduit de l'anglais par Adrien F. Vochelle, avec trois documents, 265 pp. copertina rigida Buono (Good) piccole fioriture su sguardie, ottima leggibilità e condizione delle pagine interne.

Single Issue Magazine. Estado de la sobrecubierta: No Dust Jacket As Issued. First Edition. A particularly interesting vintage issue containing a broad assortment of content, perhaps most notably the ten-page illustrated article "Traits of My Plantation Negroes" by plantation owner Howard Snyder. For those unfamiliar with the nature of life on plantations, this article will most likely raise your eyebrows several notches. Other content includes: A Hedonist (story); The God in the Garden (Japanese appreciation of nature's beauty; Forbidden Fruit (story); Making Towns Fit to Live In; C in Alt (story); The License of the Youngsters; White Dreams (story); The High Cost of Politics; Traps and Guns and Other Things; The Crystal Heart (part III); Jack London - Man and Husband (part IV); A Showman in Brazil (part I); The Ukraine and the Balance of Power (fascinating reading in light of current events); The Tide of Affairs; Investment and Banking. [32], 321-480, [38 ads] p. Includes a wonderful assortment of illustrated ads, several of which are in glorious color, most notably the full-page "Just Say Hires" root beer ad illustrated by Maxfield Parrish. Clean, tight and unmarked with light wear. A quality example of this special issue. Flacks (4th Edn) p. 127.; Color Ad; 8vo Very Good No dust jacket as issued. Illustrated by Parrish, Maxfield (ilustrador). …

Condición: new. Questo è un articolo print on demand.

Taschenbuch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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). 432 pp. Englisch.…

Buch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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). 436 pp. Englisch.…

Gebunden. Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Steven K. Thompson, PhD, is Shrum Chair in Science and Professor of Statistics at the Simon Fraser University. During his career, he has served on the faculties of the Pennsylvania State University, the University of Auckland, and the University of Alaska. .…