By Topic

Estimation of the permissible level of noise at nonlinear reconstruction of the two-dimensional image of space object

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
$33 $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

2 Author(s)
A. V. Antonov ; Inst. of Radio Astron., Nat. Acad. of Sci. of Ukraine, Kharkiv, Ukraine ; Yu. M. Gerasimov

Nonlinear processing results of radio astronomical observations of sources of a space radiation allows to increase resolving ability of radio telescopes. Thus it is possible to restore the details of the image lost at its recording. Increase of resolution grows out the account of prior information on object at its recovery. Wider prior information allows to restore details of sources of radiation more precisely. At recovery of the image of surface of the Sun on radio astronomical observations in 3 mm range it is possible to use prior information on its angular size and mean radiance temperature. The given information allows to restore coordinates, sizes and radiance temperature of active formations on its surface. Quality of restoration is limited to presence of noise in the initial image. We consider its influence on result of two-dimensional restoration of the image.

Published in:

Physics and Engineering of Microwaves, Millimeter, and Submillimeter Waves, 2004. MSMW 04. The Fifth International Kharkov Symposium on  (Volume:2 )

Date of Conference:

21-26 June 2004