Stenflo (125 résultats)

Heft. Etat : Gut. 482-490 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; der Buchzustand ist ansonsten ordentlich und dem Alter entsprechend gut. Einbandkanten sind leicht bestoßen.In ENGLISCHER Sprache. Sprache: Englisch Gewicht in Gramm: 20.…

Heft. Etat : Gut. 32 Seiten; Stempel auf Einband, Seiten alters-/papierbedingt angebräunt; ansonsten ordentlicher Erhaltungszustand; Sprache: Englisch Gewicht in Gramm: 80.

No Binding. Etat : Very Good. ORIGINAL 1970 PUBLICATION; no covers; light creasing of upper corners of several leaves; o/w in very good condition. Book.

Etat : Good. 1983. No Edition Remarks. 564 pages. Illustrated paper cover. Contains black and white diagrams. Clean pages and diagrams with light tanning and mild foxing throughout. Binding remains firm. Paper covers have mild edge-wear with slight rubbing to surfaces and curling to corners. Minor tanning to spine and covers.…

Etat : New.

Paperback or Softback. Etat : New. Solar Photosphere: Structure, Convection, and Magnetic Fields: Proceedings of the 138th Symposium of the International Astronomical Union Held in Kiev. Book.

Etat : New.

Etat : As New. Unread book in perfect condition.

Etat : As New. Unread book in perfect condition.

Etat : New.

No Binding. Etat : Very Good. ORIGINAL 1977 PUBLICATION; ex-observatory library; no covers; small chips along gutter where disbound, o/w in very good condition. Book.

Etat : New.

Etat : New. In English.

Etat : New. Proceedings of the 138th Symposium of the International Astronomical Union, held in Kiev, U.S.S.R., May 15-20, 1989 Editor(s): Stenflo, Jan. Series: International Astronomical Union Symposia (Closed). Num Pages: 560 pages, biography. BIC Classification: PGS; PHVB. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 235 x 155 x 30. Weight in Grams: 1015. . 1989. Softcover reprint of the original 1st ed. 1990. Paperback. . . . . …

Etat : New. In English.

Etat : As New. Unread book in perfect condition.

Etat : New. pp. 448.

Hardcover. Etat : UsedGood. Hardcover; proceedings of the 30th Nobel Symposium held April 2-4, 1975 at Kiruna Geophysical Institute, Kiruna, Sweden; surplus library copy with the usual stampings; reference number taped to spine; bar code taped to front cover; fading and shelf wear to exterior; corners bumped; in good condition with clean text, firm binding. No dust jacket. …

Etat : New. pp. 576.

Paperback. Etat : Brand New. reprint edition. 450 pages. 9.25x6.10x1.00 inches. In Stock.

Gr.8. 560 pp. Original hardcover with dustjackett. Good copy. Achtung: Gewichtsbedingt erfolgt der Versand per Päckchen (EUR 5,19 Inlandsporto). Bitte bestellen Sie nur, wenn Sie dieser Portoanpassung zustimmen können.

Etat : New. Proceedings of the 138th Symposium of the International Astronomical Union, held in Kiev, U.S.S.R., May 15-20, 1989 Editor(s): Stenflo, Jan. Series: International Astronomical Union Symposia (Closed). Num Pages: 560 pages, biography. BIC Classification: PGS; PHVB. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 235 x 155 x 30. Weight in Grams: 1015. . 1989. Softcover reprint of the original 1st ed. 1990. Paperback. . . . . Books ship from the US and Ireland. …

Paperback. Etat : Brand New. reprint edition. 572 pages. 9.25x6.10x1.30 inches. In Stock.

Taschenbuch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - Much progress has been made in recent years in understanding the complex physics of polarized radiation in the sun and stars. This physics includes vector radiative transfer and spectral line formation in the presence of magnetic fields, scattering theory and coherence effects, partial redistribution and turbulent magnetic fields, numerical techniques and Stokes inversion, as well as concepts for polarimetric imaging with a precision limited only by photon statistics. The present volume gives a comprehensive and up-to-date account of this rapidly evolving field of science.…

Taschenbuch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - Solar and stellar photospheres constitute the layers most accessible to observations, forming the interface between the interior and the outside of the stars. The solar atmosphere is a rich physics laboratory, in which the whole spectrum of radiative, dynamical, and magnetic processes that tranfer energy into space can be observed. As the fundamental processes take place on very small spatial scales, we need high resolution observations to explore them. On the other hand the small-scale processes act together to form global properties of the sun, which have their origins in the solar interior. The rapid advances in observational techniques and theoreticallllodelling over the past decade made it very timely to bring together scientists from east and west to the first lAU Symposium on this topic. The physics of the photosphere involves complicated interactions between magnetic fields, convection, waves, and radiation. During the past decade our understanding of these gener ally small-scale structures and processes has been dramatically advanced. New instrumen tations, on ground and in space, have given us new means to study the granular convection. Diagnostic methods in Stokes polarimetry have allowed us to go beyond the limitations of spatial resolution to explore the structure and dynamics of the subarcsec magnetic struc tures. Extensive numerical simulations of the interaction between convection and magnetic fields using powerful supercomputers are providing deepened physical insight. Granulation, magnetic fields, and dynamo processes are being explored in the photospheres of other stars, guided by our improved understanding of the solar photosphere.…

Hardcover. Etat : As New. Leichte Kratzer / Abnutzungen / Druckstellen. Novel instruments for high-precision imaging polarimetry have opened new possibilities, including for exploring effects in radiative scattering, atomic physics, spectral line formation, and radiative transfer. This volume gives a comprehensive and up-to-date account of this rapidly evolving and interdisciplinary field of science.…

Etat : New.

Hardcover. Etat : new. Hardcover. Traditionally, solar and stellar physics have been two separate branches of astronomy, which independently of each other have developed their own scientific goals and methods. During the last decade, however, we have witnessed a gradual convergence of these two areas: The solar physicists realize more and more that the sun has to be seen as a special case in a large family of stars of various properties. A more complete understanding of the sun can only be achieved by considering it in this broader context. The stellar physicists on the other hand have become aware that the detailed knowledge of the physical processes that the solar physicists have reached has a more general significance and can be applied to a variety of other astrophysical objects. Observational techniques developed in solar work can frequently be adapted for other stars as well. This unified approach to solar and stellar physics is often called the "solar-stellar connection". One main goal of this approach has been to understand the general nature and causes of stellar activity. The pioneering and visionary program to search for activity cycles on other stars started by Olin Wilson at the Mount Wilson Observatory 16 years ago has born fruit: in his sample of 91 stars, cyclic behaviour similar to that of the sun is found to be quite common, but many stars also show irregular activity fluctua.tions of large amplitude. The pioneering and visionary program to search for activity cycles on other stars started by Olin Wilson at the Mount Wilson Observatory 16 years ago has born fruit: in his sample of 91 stars, cyclic behaviour similar to that of the sun is found to be quite common, but many stars also show irregular activity fluctua.tions of large amplitude. Shipping may be from multiple locations in the US or from the UK, depending on stock availability.…

Taschenbuch. Etat : Neu. Solar Photosphere: Structure, Convection, and Magnetic Fields | Proceedings of the 138th Symposium of the International Astronomical Union Held in kiev,USSR, May 15-20, 1989 | Jan Olof Stenflo | Taschenbuch | xii | Englisch | 1989 | Springer Netherland | EAN 9780792305309 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.…

Etat : New.