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MHD Waves in the Solar Atmosphere
Bernard Roberts
出版
Cambridge University Press
, 2019-07-18
主題
Mathematics / Applied
Science / Space Science / Astronomy
Science / Physics / Astrophysics
Science / Physics / Electromagnetism
Science / Earth Sciences / Meteorology & Climatology
Science / Physics / General
Science / Earth Sciences / Seismology & Volcanism
Science / Mechanics / Fluids
ISBN
1108427669
9781108427661
URL
http://books.google.com.hk/books?id=1jCdDwAAQBAJ&hl=&source=gbs_api
EBook
SAMPLE
註釋
This volume presents a full mathematical exposition of the growing field of coronal seismology which will prove invaluable for graduate students and researchers alike. Roberts' detailed and original research draws upon the principles of fluid mechanics and electromagnetism, as well as observations from the TRACE and SDO spacecraft and key results in solar wave theory. The unique challenges posed by the extreme conditions of the Sun's atmosphere, which often frustrate attempts to develop a comprehensive theory, are tackled with rigour and precision; complex models of sunspots, coronal loops and prominences are presented, based on a magnetohydrodynamic (MHD) view of the solar atmosphere, and making use of Faraday's concept of magnetic flux tubes to analyse oscillatory phenomena. The rapid rate of progress in coronal seismology makes this essential reading for those hoping to gain a deeper understanding of the field.