logo
Product categories

EbookNice.com

Most ebook files are in PDF format, so you can easily read them using various software such as Foxit Reader or directly on the Google Chrome browser.
Some ebook files are released by publishers in other formats such as .awz, .mobi, .epub, .fb2, etc. You may need to install specific software to read these formats on mobile/PC, such as Calibre.

Please read the tutorial at this link.  https://ebooknice.com/page/post?id=faq


We offer FREE conversion to the popular formats you request; however, this may take some time. Therefore, right after payment, please email us, and we will try to provide the service as quickly as possible.


For some exceptional file formats or broken links (if any), please refrain from opening any disputes. Instead, email us first, and we will try to assist within a maximum of 6 hours.

EbookNice Team

(Ebook) Magnetohydrodynamics of the Sun by Priest E. ISBN 9780521854719, 0521854717

  • SKU: EBN-4584138
Zoomable Image
$ 32 $ 40 (-20%)

Status:

Available

4.5

16 reviews
Instant download (eBook) Magnetohydrodynamics of the Sun after payment.
Authors:Priest E.
Pages:582 pages.
Year:2014
Editon:2ed. Draft
Publisher:Cambridge University Press
Language:english
File Size:16.99 MB
Format:pdf
ISBNS:9780521854719, 0521854717
Categories: Ebooks

Product desciption

(Ebook) Magnetohydrodynamics of the Sun by Priest E. ISBN 9780521854719, 0521854717

Magnetohydrodynamics of the Sun is a completely new up-to-date rewrite from scratch of the 1982 book Solar Magnetohydrodynamics, taking account of enormous advances in understanding since that date. It describes the subtle and complex interaction between the Sun's plasma atmosphere and its magnetic field, which is responsible for many fascinating dynamic phenomena. Chapters cover the generation of the Sun's magnetic field by dynamo action, magnetoconvection and the nature of photospheric flux tubes such as sunspots, the heating of the outer atmosphere by waves or reconnection, the structure of prominences, the nature of eruptive instability and magnetic reconnection in solar flares and coronal mass ejections, and the acceleration of the solar wind by reconnection or wave-turbulence. Developed for a graduate course at St. Andrews University, this advanced textbook provides a detailed account of our progress toward answering many key unsolved puzzles in solar physics. It is essential reading for graduate students and researchers in solar physics and related fields of astronomy, plasma physics, and fluid dynamics. Problem sets and other resources are available at www.cambridge.org/9780521854719
*Free conversion of into popular formats such as PDF, DOCX, DOC, AZW, EPUB, and MOBI after payment.

Related Products