Cart (Loading....) | Create Account
Close category search window
 

Investigation of time scales of the millimeter waveband solar emission

Sign In

Cookies must be enabled to login.After enabling cookies , please use refresh or reload or ctrl+f5 on the browser for the login options.

Formats Non-Member Member
$31 $13
Learn how you can qualify for the best price for this item!
Become an IEEE Member or Subscribe to
IEEE Xplore for exclusive pricing!
close button

puzzle piece

IEEE membership options for an individual and IEEE Xplore subscriptions for an organization offer the most affordable access to essential journal articles, conference papers, standards, eBooks, and eLearning courses.

Learn more about:

IEEE membership

IEEE Xplore subscriptions

1 Author(s)
Luk'yanov, M.Y. ; Inst. of Radio Astron., Nat. Acad. of Sci. of Ukraine, Kharkov

A study of solar radio emission in the mm wavelength range is used to investigate processes occurring in the lower chromosphere and in the transition region. This region is characterized by a complex structure of magnetic field and sharp temperature gradients. The phenomena observed reflect processes in the photosphere and convection zone which are bound up closely with energy transportation from the photosphere towards the chromosphere and with heating and maintenance of the solar corona

Published in:

Physics and Engineering of Millimeter and Sub-Millimeter Waves, 2001. The Fourth International Kharkov Symposium on  (Volume:2 )

Date of Conference:

2001

Need Help?


IEEE Advancing Technology for Humanity About IEEE Xplore | Contact | Help | Terms of Use | Nondiscrimination Policy | Site Map | Privacy & Opting Out of Cookies

A not-for-profit organization, IEEE is the world's largest professional association for the advancement of technology.
© Copyright 2014 IEEE - All rights reserved. Use of this web site signifies your agreement to the terms and conditions.