Annotation
Cosmic strings are theoretically predicted linear structures of a cosmological size. The search for cosmic strings in optical and radio observations has been an important area of research in recent years. One of the most effective methods of searching for these objects is the analysis of the anisotropy of cosmic microwave background radiation that could be induced by cosmic strings. For this purpose, the authors propose a method of signal expansion in modified Haar functions with cyclic translations. However, for a system of these functions to be used correctly, one needs to prove its orthonormality and completeness, which is the purpose of this paper.
Received: 2011 April 12
Approved: 2012 March 20
PACS:
02.60.-x Numerical approximation and analysis
95.75.Mn Image processing
98.70.Vc Background radiations
98.80.-k Cosmology
95.75.Mn Image processing
98.70.Vc Background radiations
98.80.-k Cosmology
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
O.S. Sazhina, M.V. Sazhin
Sternberg Astronomical Institute, Moscow State University, Moscow, 119991, Russia
Sternberg Astronomical Institute, Moscow State University, Moscow, 119991, Russia