PERHAPS A GIFT VOUCHER FOR MUM?: MOTHER'S DAY

Close Notification

Your cart does not contain any items

$184.95

Hardback

Not in-store but you can order this
How long will it take?

QTY:

English
Cambridge University Press
12 November 2020
Recent observational results from space- and ground-based telescopes have demonstrated that a unified approach to the relationships between solar and stellar magnetism is necessary to advance our understanding of magnetic fields. The Proceedings of IAU Symposium 354 present recent results and discussions of emerging topics, including: magnetic field diagnostics using high-resolution observation; initial data from ALMA, Chinese Radio Spectroheliograph and other instruments; the detection of stellar magnetospheres; and the detailed mapping of magnetic fields on the surface of stars using new unique instrumentation. These observations stimulate comparisons of solar and stellar results, and improve our understanding of how surface magnetic structures and their evolution are related to the generation of magnetic fields by dynamos in solar and stellar interiors. This volume benefits graduate students and researchers interested in the recent advances and key problems of solar and stellar magnetic fields, and their impacts on planetary atmospheres.

Edited by:   , , ,
Imprint:   Cambridge University Press
Country of Publication:   United Kingdom
Dimensions:   Height: 254mm,  Width: 182mm,  Spine: 23mm
Weight:   970g
ISBN:   9781108482493
ISBN 10:   110848249X
Series:   Proceedings of the International Astronomical Union Symposia and Colloquia
Pages:   512
Publication Date:  
Audience:   Professional and scholarly ,  Undergraduate
Format:   Hardback
Publisher's Status:   Active
Part I. Total Solar Eclipse of 2019; Part II. New Observational Diagnostics of Solar, Stellar and Interstellar Magnetic Fields; Part III. Progress in Understanding the Solar/Stellar Interior Dynamics and Dynamos; Part IV. Stellar Rotation and Magnetism; Part V. Role of Magnetic Fields in Solar and Stellar Variability; Part VI. Star-Planet Relations; Part VII. Formation, Structure and Dynamics of Solar and Stellar Coronae and Winds; Part VIII. Mechanisms of Flaring and CME Activity on the Sun and Stars; Part IX. Surface Magnetic Fields of the Sun and Stars; Part X. Observations of Solar Eclipses and Exoplanetary Transits.

See Also