logo

EbookBell.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://ebookbell.com/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.

EbookBell Team

Solar Dynamics And Magnetism From The Interior To The Atmosphere 1st Edition Nagi N Mansour

  • SKU: BELL-4598880
Solar Dynamics And Magnetism From The Interior To The Atmosphere 1st Edition Nagi N Mansour
$ 31.00 $ 45.00 (-31%)

0.0

0 reviews

Solar Dynamics And Magnetism From The Interior To The Atmosphere 1st Edition Nagi N Mansour instant download after payment.

Publisher: Springer-Verlag New York
File Extension: PDF
File size: 44.18 MB
Pages: 454
Author: Nagi N. Mansour, Alexander G. Kosovichev (auth.), Nagi N. Mansour, Alexander G. Kosovichev, Rudolf Komm, Dana Longcope (eds.)
ISBN: 9781489980045, 9781489980052, 1489980040, 1489980059
Language: English
Year: 2014
Edition: 1

Product desciption

Solar Dynamics And Magnetism From The Interior To The Atmosphere 1st Edition Nagi N Mansour by Nagi N. Mansour, Alexander G. Kosovichev (auth.), Nagi N. Mansour, Alexander G. Kosovichev, Rudolf Komm, Dana Longcope (eds.) 9781489980045, 9781489980052, 1489980040, 1489980059 instant download after payment.

Discusses recent advances and new problems in the exploration of the Sun's interior structure, solar dynamics and dynamo, mechanisms of sunspot and active regions formation, sources of solar irradiance variations and links between the subsurface dynamics, flaring and CME activity.

NASA's Solar Dynamics Observatory (SDO) mission has provided a large amount of new data on solar dynamics and magnetic activities during the rising phase of the current and highly unusual solar cycle. These data are complemented by the continuing SOHO mission and by ground-based observatories that include the GONG helioseismology network and the New Solar Telescope. Also, the observations are supported by realistic numerical simulations on supercomputers. This unprecedented amount of data provides a unique opportunity for multi-instrument investigations that address fundamental problems of the origin of solar magnetic activity at various spatial and temporal scales. This book demonstrates that the synergy of high-resolution multi-wavelength observations and simulations is a key to uncovering the long-standing puzzles of solar magnetism and dynamics.

This volume is aimed at researchers and graduate students active in solar physics and space science.

Originally published in Solar Physics journal, Vol. 287/1-2, 2013.

Related Products