Jorgen Christensen Dalsgaard (112 results)

Soft cover. Condition: Fair.

Hardcover. Condition: Fine. First Edition. Tall octavo: 416 p. with numerous textual figures. Original glossy boards; issued without a dust jacket. A fine copy.

Condition: New.

Condition: As New. Unread book in perfect condition.

Condition: New.

rilegato. Condition: Ottimo (Fine). Book.

Condition: New.

Condition: New. A comprehensive overview of the current state of knowledge in stellar astrophysical fluid dynamics. Editor(s): Thompson, Michael J.; Christensen-Dalsgaard, Jorgen. Num Pages: 432 pages, 115 b/w illus. 3 tables. BIC Classification: PGM; PHDF; PHVB. Category: (P) Professional & Vocational. Dimension: 247 x 174 x 22. Weight in Grams: 690. . 2008. 1st Edition. paperback. . . . . …

Condition: As New. Unread book in perfect condition.

Condition: New. A comprehensive overview of the current state of knowledge in stellar astrophysical fluid dynamics. Editor(s): Thompson, Michael J.; Christensen-Dalsgaard, Jorgen. Num Pages: 432 pages, 115 b/w illus. 3 tables. BIC Classification: PGM; PHDF; PHVB. Category: (P) Professional & Vocational. Dimension: 247 x 174 x 22. Weight in Grams: 690. . 2008. 1st Edition. paperback. . . . . Books ship from the US and Ireland. …

Condition: New. pp. 432.

Condition: New. pp. 632.

Paperback. Condition: Brand New. reprint edition. 628 pages. 10.00x7.01x1.43 inches. In Stock.

Condition: Sehr gut. Gebunden. Sehr gut erhalten. Hardcover. Very good condition. Sprache: Englisch Gewicht in Gramm: 1.

Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - Helio- and asteroseismology study the interior of the Sun and other stars, by means of observations of oscillations on their surfaces. The last 10 years in the study of the solar interior, to a has witnessed a very rapid evolution point where we can now contemplate investigating the physical state of matter, or the details of rotation and other large-scale motion, in the Sun. The stellar studies are in some respects at the point of the solar studies 10 years ago, but appear poised to take off. Thus the time was deemed ripe for lAO Symposium No 123, to assess the present status of this work, and plan for its future development. Apart from the seismic data, few observations are available to provide information about stellar interiors. Detailed studies, by spectral analysis, can be made of stellar surface properties, including atmospheric temperature and chemical composition. However, the stellar radiative spectrum is almost entirely fixed by the mass, luminosity, radius and surface rotation of the star, and contains essentially no other information about the interior. An important test of stellar evolution theory is provided by observations of stel lar clusters, whose members can reasonably be assumed to have the same age and chemical composition. The location of such stars in a HR diagram, where luminosity is plotted against the effective temperature, can roughly be understood in terms of stellar evolution calculations.…

Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - In all phases of the life of a star, hydrodynamical processes play a major role. This volume gives a comprehensive overview of the state of knowledge in stellar astrophysical fluid dynamics, and its publication marked the 60th birthday of Douglas Gough, Professor of Theoretical Physics at the University of Cambridge and leading contributor to stellar astrophysical fluid dynamics. Topics include properties of pulsating stars, helioseismology, convection and mixing in stellar interiors, dynamics of stellar rotation, planet formation and the generation of stellar and planetary magnetic fields. Each chapter is written by leading experts in the field, and the book provides an overview that is central to any attempt to understand the properties of stars and their evolution. With extensive references to the technical literature, this is a valuable text for researchers and graduate students in stellar astrophysics.…

Couverture souple. Condition: bon. R260269786: 1987. In-8. Broché. Très bon état, Couv. convenable, Dos satisfaisant, Intérieur frais. 604 pages augmentées de quelques figures en noir et blanc dans texte. . . . Classification Dewey : 420-Langue anglaise. Anglo-saxon.

Condition: New.

Condition: New.

Condition: New.

Condition: New.

Condition: New.

Condition: As New. Unread book in perfect condition.

Condition: New.

Condition: New. A comprehensive overview of the current state of knowledge in stellar astrophysical fluid dynamics. Editor(s): Thompson, Michael J.; Christensen-Dalsgaard, Jorgen. Num Pages: 430 pages, 115 b/w illus. 3 tables. BIC Classification: PGM; PHDF; PHVB. Category: (P) Professional & Vocational. Dimension: 247 x 174 x 24. Weight in Grams: 1012. . 2003. Illustrated. hardcover. . . . . …

Taschenbuch. Condition: Neu. SCORe '96: Solar Convection and Oscillations and their Relationship | F. P. Pijpers (u. a.) | Taschenbuch | Astrophysics and Space Science Library | vii | Englisch | 2012 | Springer | EAN 9789401061728 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu. …

Condition: New. The existence of strongly convecting layers in the Sun and stars provides us with a natural laboratory for the study of dynamical processes in intensely turbulent, magnetized, rotating, radiating fluids. This work contains papers which present developments in each of these fields. Editor(s): Pijpers, F.P.; Christensen-Dalsgaard, J.; Rosenthal, C.S. Series: Astrophysics and Space Science Library. Num Pages: 322 pages, biography. BIC Classification: PGS. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 235 x 155 x 19. Weight in Grams: 636. . 1998. Hardback. . . . . …

Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - This volume contains the reviews and poster papers presented at the workshop Solar Convection and Oscillations and their Relationship: SCORe '96, held in Arhus, Denmark, May 27 - 31, 1996. The aim of this workshop was to bring together experts in the fields of convection and helioseismology, and to stimulate collaborations and joint research. The participation to this workshop was purposely kept limited in order to provide optimal conditions for informal discussions. In autumn of 199,5 the long-awaited GONG network of solar telescopes became fully operational and the first data already show significant improvement over existing datasets on solar oscillations. Furthermore, in December of 1995 the satellite SOHO was launched which, together with GONG, provides a major step forward in both the quantity and the quality of available solar oscillation data. It is with this in mind that we decided to organize the workshop to prepare for the optimal use of this wealth of data, with which to deepen our understanding of solar structure and specifically, of one of the longest-standing problems in solar and stellar modelling: the treatment of convection.…

Buch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - This volume contains the reviews and poster papers presented at the workshop Solar Convection and Oscillations and their Relationship: SCORe '96, held in Arhus, Denmark, May 27 - 31, 1996. The aim of this workshop was to bring together experts in the fields of convection and helioseismology, and to stimulate collaborations and joint research. The participation to this workshop was purposely kept limited in order to provide optimal conditions for informal discussions. In autumn of 199,5 the long-awaited GONG network of solar telescopes became fully operational and the first data already show significant improvement over existing datasets on solar oscillations. Furthermore, in December of 1995 the satellite SOHO was launched which, together with GONG, provides a major step forward in both the quantity and the quality of available solar oscillation data. It is with this in mind that we decided to organize the workshop to prepare for the optimal use of this wealth of data, with which to deepen our understanding of solar structure and specifically, of one of the longest-standing problems in solar and stellar modelling: the treatment of convection.…

Kartoniert / Broschiert. Condition: New.