Sprache: Englisch
Verlag: Cambridge University Press, 1996
ISBN 10: 0521563070 ISBN 13: 9780521563079
Anbieter: Anybook.com, Lincoln, Vereinigtes Königreich
EUR 34,58
Anzahl: 1 verfügbar
In den WarenkorbZustand: Good. Volume 6. This is an ex-library book and may have the usual library/used-book markings inside.This book has hardback covers. Clean from markings. In good all round condition. No dust jacket. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,1100grams, ISBN:9780521563079.
Sprache: Englisch
Verlag: Cambridge University Press, 1996
ISBN 10: 0521563070 ISBN 13: 9780521563079
Anbieter: Ria Christie Collections, Uxbridge, Vereinigtes Königreich
EUR 118,59
Anzahl: Mehr als 20 verfügbar
In den WarenkorbZustand: New. In.
Sprache: Englisch
Verlag: Cambridge University Press, 1996
ISBN 10: 0521563070 ISBN 13: 9780521563079
Anbieter: Kennys Bookstore, Olney, MD, USA
EUR 173,28
Anzahl: Mehr als 20 verfügbar
In den WarenkorbZustand: New. A 1996 review of how the interior of the Sun can be studied using the powerful techniques of helioseismology and neutrino astronomy. Editor(s): Cortes, T.Roca; Sanchez, Francisco. Num Pages: 424 pages, 30 b/w illus. 1 map 7 tables. BIC Classification: PGS; PHVB. Category: (P) Professional & Vocational. Dimension: 247 x 174 x 24. Weight in Grams: 95. . 1996. 1st Edition. hardcover. . . . . Books ship from the US and Ireland.
Sprache: Englisch
Verlag: Cambridge University Press, 1996
ISBN 10: 0521563070 ISBN 13: 9780521563079
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - The complex internal structure of the Sun can now be studied in detail through helioseismology and neutrino astronomy. The VI Canary Islands Winter School of Astrophysics was dedicated to examining these powerful new techniques. Based on this meeting, seven specially written chapters by world experts renowned for their teaching skills are presented in this timely volume. With a clear and pedagogical style we are shown how the internal composition (density, He abundance, etc.) and dynamical structure (rotation, subsurface velocity fields, etc.) of the Sun can be deduced through helioseismology; and how the central temperature can be inferred from measurements of the flux of solar neutrinos. This volume provides an excellent introduction for graduate students and an up-to-date overview for researchers working on the Sun, neutrino astronomy and helio- and asteroseismology.