Morphological studies on ionospheric VHF scintillations over an Indian low latitude station during a solar cycle period (2001-2010)

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• 作者：S.N.V.S. Prasad¹ ; ^{prasadsnvs@yahoo.com} ; P.V.S. Rama Rao ; ^{palurivsrao@gmail.com} ; D.S.V.V.D. Prasad² ; ^{dsvvdprasad@yahoo.com} ; K. Venkatesh³ ; ^{venkatkau@gmail.com} ; K. Niranjan⁴ ; ^{niranjankandula@hotmail.com}
• 关键词：VHF scintillations ; Occurrence characteristics ; Fading rate and patch duration of scintillations ; Spread-F
• 刊名：Advances in Space Research
• 出版年：2012
• 期刊代码：6_02731177
• 类别：et
• 出版时间：1 July, 2012
• 卷：50
• 期：1
• 页码：56-69
• 文件大小：2783 K

摘要

The amplitude scintillations data recorded at 244 MHz from the geostationary satellite, FLEETSAT (73掳E) at a low latitude station, Waltair (17.7掳N, 83.3掳E) during the ten year period of high to low solar activity from 2001 to 2010 is considered to study the occurrence characteristics of the VHF scintillations. A close association between the intense scintillations on VHF signals during pre-midnight hours, associated with range type of spread-F on ionograms and a relatively weak and slow fading scintillations during post-midnight hours associated with frequency type of spread-F is observed during the relatively high sunspot years from 2001 to 2004, whereas during the low sunspot years from 2005 to 2010 the scintillation activity as well as spread-F activity are found to be minimum. During both the high and low sunspot years, it is observed that the maximum scintillation activity occurs during equinoctial months followed by winter with the minimum occurrence during summer months. The annual mean percentage occurrence of scintillations is found to be clearly associated with the variations in the annual mean sunspot number. The nocturnal variations in the occurrence of scintillations show the onset of scintillation activity starts from 19:00 h LT with maximum of occurrence around 21:00 h LT. A clear semiannual variation in the occurrence of scintillations is observed during pre-midnight hours with two peaks in equinoctial months of March/April and September/October. The number of scintillation patches observed is found to be more during pre-midnight hours compared to those during post-midnight hours. The most probable scintillation patch duration lies around 30 min. Further, it is also found that the number of scintillation patches with durations of 60 min and more decreases with the increase in the patch duration. It is also observed in general that the scintillation activity is inhibited during geomagnetic disturbed days.