Power spectral characteristics of ESF irregularities during magnetically quiet and disturbed days

dc.contributor.authorKakad, Bharatien_US
dc.contributor.authorNayak, C. K.en_US
dc.contributor.authorBhattacharyya, A.en_US
dc.date.accessioned2026-07-24T06:35:40Z
dc.date.issued2012
dc.description.abstractAmplitude scintillations on 251 MHz signal recorded by spaced receivers at Tirunelveli (8.7°N, 77.8°E, dip latitude 0.6°N) for eight months during 1995–2005 are utilized in present work. Power spectral analysis of weak scintillations (0.15≤S4≤0.5) is carried out and spectral index, m of ESF irregularities, is computed for quiet and disturbed days. Maximum cross-correlation, CI(x0,tm), of intensity variations between two receivers is used to identify the fresh generation of EPBs resulted from magnetic activity. Increase in F-region height is seen prior to the generation of these fresh EPBs and associated ESF irregularities found to possess shallower power spectrum.en_US
dc.identifier.citationJournal of Atmospheric and Solar-Terrestrial Physics, v.81-82, p.41-49, 2012, doi: 10.1016/j.jastp.2012.04.008en_US
dc.identifier.other91243
dc.identifier.urihttps://repository.iigm.res.in/handle/123456789/2131
dc.languageenen_US
dc.subjectScintillationen_US
dc.subjectPower spectrumen_US
dc.subjectMagnetic activityen_US
dc.subjectFreshly generated EPBsen_US
dc.titlePower spectral characteristics of ESF irregularities during magnetically quiet and disturbed daysen_US
dc.typeArticleen_US

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