Please note: In order to keep Hive up to date and provide users with the best features, we are no longer able to fully support Internet Explorer. The site is still available to you, however some sections of the site may appear broken. We would encourage you to move to a more modern browser like Firefox, Edge or Chrome in order to experience the site fully.

Ultraviolet and X-ray Spectroscopy of the Solar Atmosphere, Paperback / softback Book

Ultraviolet and X-ray Spectroscopy of the Solar Atmosphere Paperback / softback

Part of the Cambridge Astrophysics series

Paperback / softback

Description

The solar atmosphere, above the Sun's surface layers, reaches mega-kelvin temperatures and high levels of dynamic activity through processes involving a pervading magnetic field.

This book explores one of the principal means of understanding the solar atmosphere, its ultraviolet and soft X-ray emission.

The ultraviolet and X-ray spectra of the Sun's atmosphere provide valuable information about its nature - the heat and density of its various parts, its dynamics, and chemical composition.

The principles governing spectral line and continuous emission, and how spectral studies lead to deductions about physical properties, are described, together with spacecraft instrumentation from Skylab, SolarMax, Yohkoh, SOHO, TRACE, and Hinode.

With introductions to atomic physics and diagnostic techniques used by solar spectroscopists, a list of emission lines in ultraviolet and soft X-ray regions, and a glossary of terms, this is an ideal reference for graduate students and researchers in astrophysics and solar physics.

Information

Save 5%

£32.99

£31.19

 
Free Home Delivery

on all orders

 
Pick up orders

from local bookshops

Information

Also in the Cambridge Astrophysics series  |  View all