Title :
Millimeter radio astronomy as a probe for convective zone of the Sun
Author :
Arkhypov, O.V. ; Antonov, A.V.
Author_Institution :
Inst. of Radio Astron., Nat. Acad. Sc. of Ukraine, Kharkov, Ukraine
Abstract :
One means of solar activity monitoring are radiotelescopes of mm-wavelength. The subject of this study is the large-scale, longitudinal structure of the chromosphere to assess the capabilities of millimeter radio astronomy to probe the deep layers of the convective zone of the Sun.
Keywords :
chromosphere; radioastronomy; solar activity; solar evolution; solar pulsations; solar spectra; AD 1994 to 1998; AD 1995 to 2007; AD 1998 to 2003; AD 2000 07 to 2003 12; Big Bear Solar Observatory; Metsahovi Observatory; Mount Wilson Observatory; Sun convective zone; chromosphere longitudinal structure; millimeter radio astronomy; power spectrum; solar activity; Correlation; Harmonic analysis; Iron; Mirrors; Observatories; Radio astronomy; Sun;
Conference_Titel :
Physics and Engineering of Microwaves, Millimeter and Submillimeter Waves (MSMW), 2010 International Kharkov Symposium on
Conference_Location :
Kharkiv
Print_ISBN :
978-1-4244-7900-9
DOI :
10.1109/MSMW.2010.5546109
