Title :
Investigation of time scales of the millimeter waveband solar emission
Author_Institution :
Inst. of Radio Astron., Nat. Acad. of Sci. of Ukraine, Kharkov
Abstract :
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
Keywords :
chromosphere; solar corona; solar radiofrequency radiation; Sun; convection zone; energy transportation; heating; lower chromosphere; magnetic field structure; mm emission time scales; mm wavelength observations; photosphere; solar corona; solar radio emission; temperature gradients; transition region; Brightness; Corona; Magnetic fields; Magnetic flux; Magnetic separation; Magnetohydrodynamic power generation; Radio astronomy; Solar power generation; Sun; Transportation;
Conference_Titel :
Physics and Engineering of Millimeter and Sub-Millimeter Waves, 2001. The Fourth International Kharkov Symposium on
Conference_Location :
Kharkov
Print_ISBN :
0-7803-6473-2
DOI :
10.1109/MSMW.2001.947319
