It takes the average reader 6 hours to read Ultraviolet and X-ray Spectroscopy of the Solar Atmosphere by Kenneth J. H. Phillips
Assuming a reading speed of 250 words per minute. Learn more
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.
Ultraviolet and X-ray Spectroscopy of the Solar Atmosphere by Kenneth J. H. Phillips is 360 pages long, and a total of 90,000 words.
This makes it 121% the length of the average book. It also has 110% more words than the average book.
The average oral reading speed is 183 words per minute. This means it takes 8 hours and 11 minutes to read Ultraviolet and X-ray Spectroscopy of the Solar Atmosphere aloud.
Ultraviolet and X-ray Spectroscopy of the Solar Atmosphere is suitable for students ages 12 and up.
Note that there may be other factors that effect this rating besides length that are not factored in on this page. This may include things like complex language or sensitive topics not suitable for students of certain ages.
When deciding what to show young students always use your best judgement and consult a professional.
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