A Study of Early/Slow VLF Perturbations Observed at Agra, India
We present here the results of sub-ionospheric VLF perturbations observed on NWC (19.8 kHz) transmitter signal propagating in the Earth-ionosphere waveguide, monitored at our low latitude station Agra. During the period of observation (June-December 2011), we found 89 cases of VLF perturbation, whil...
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description | We present here the results of sub-ionospheric VLF perturbations observed on NWC (19.8 kHz) transmitter signal propagating in the Earth-ionosphere waveguide, monitored at our low latitude station Agra. During the period of observation (June-December 2011), we found 89 cases of VLF perturbation, while only 73 cases showing early character associated with strong lightning discharges. Out of 73 events, 64 (~84%) of the early VLF perturbations are found to be early/slow in nature; the remaining 9 events are early/fast. The onset duration of these early/slow VLF perturbations is up to ~ 5 s. A total of 54 observed early events show amplitude change lying between ± 3.0 dB, and phase change ± 12 degree, respectively, and found to occur mainly during nighttime. One of the interesting results we found is that the events with larger recovery time lie far away from the VLF propagation path, while events with smaller duration of recovery are within the ± 50–100 km of signal path. The World Wide Lightning Location Network (WWLLN) data is analysed to find the location of causative lightning and temporal variation. The lightning discharge and associated processes that lead to early VLF events are discussed. |
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During the period of observation (June-December 2011), we found 89 cases of VLF perturbation, while only 73 cases showing early character associated with strong lightning discharges. Out of 73 events, 64 (~84%) of the early VLF perturbations are found to be early/slow in nature; the remaining 9 events are early/fast. The onset duration of these early/slow VLF perturbations is up to ~ 5 s. A total of 54 observed early events show amplitude change lying between ± 3.0 dB, and phase change ± 12 degree, respectively, and found to occur mainly during nighttime. One of the interesting results we found is that the events with larger recovery time lie far away from the VLF propagation path, while events with smaller duration of recovery are within the ± 50–100 km of signal path. The World Wide Lightning Location Network (WWLLN) data is analysed to find the location of causative lightning and temporal variation. The lightning discharge and associated processes that lead to early VLF events are discussed.</description><identifier>ISSN: 1895-6572</identifier><identifier>EISSN: 1895-7455</identifier><identifier>DOI: 10.1515/acgeo-2016-0016</identifier><language>eng</language><publisher>Cham: Springer International Publishing</publisher><subject>Atmospheric sciences ; early VLF perturbations ; Earth and Environmental Science ; Earth Sciences ; Earth-ionosphere waveguide ; Geophysics ; Geophysics/Geodesy ; Geotechnical Engineering & Applied Earth Sciences ; Ionosphere ; Lightning ; Propagation ; Structural Geology ; Transient Luminous Events (TLEs)</subject><ispartof>Acta geophysica, 2016-06, Vol.64 (3), p.755-771</ispartof><rights>Pandey et al. 2016</rights><rights>Acta Geophysica is a copyright of Springer, 2016.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c405t-e90aac6cccedf04305b84f0c90b1aaef17a889207330b4d3a428140ae1699203</citedby><cites>FETCH-LOGICAL-c405t-e90aac6cccedf04305b84f0c90b1aaef17a889207330b4d3a428140ae1699203</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1515/acgeo-2016-0016$$EPDF$$P50$$Gspringer$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1515/acgeo-2016-0016$$EHTML$$P50$$Gspringer$$Hfree_for_read</linktohtml><link.rule.ids>314,777,781,27905,27906,41469,42538,51300</link.rule.ids></links><search><creatorcontrib>Pandey, Uma</creatorcontrib><creatorcontrib>Singh, Ashutosh K.</creatorcontrib><creatorcontrib>Singh, Om P.</creatorcontrib><creatorcontrib>Singh, Birbal</creatorcontrib><creatorcontrib>Saraswat, Vibhav K.</creatorcontrib><title>A Study of Early/Slow VLF Perturbations Observed at Agra, India</title><title>Acta geophysica</title><addtitle>Acta Geophys</addtitle><description>We present here the results of sub-ionospheric VLF perturbations observed on NWC (19.8 kHz) transmitter signal propagating in the Earth-ionosphere waveguide, monitored at our low latitude station Agra. During the period of observation (June-December 2011), we found 89 cases of VLF perturbation, while only 73 cases showing early character associated with strong lightning discharges. Out of 73 events, 64 (~84%) of the early VLF perturbations are found to be early/slow in nature; the remaining 9 events are early/fast. The onset duration of these early/slow VLF perturbations is up to ~ 5 s. A total of 54 observed early events show amplitude change lying between ± 3.0 dB, and phase change ± 12 degree, respectively, and found to occur mainly during nighttime. One of the interesting results we found is that the events with larger recovery time lie far away from the VLF propagation path, while events with smaller duration of recovery are within the ± 50–100 km of signal path. The World Wide Lightning Location Network (WWLLN) data is analysed to find the location of causative lightning and temporal variation. The lightning discharge and associated processes that lead to early VLF events are discussed.</description><subject>Atmospheric sciences</subject><subject>early VLF perturbations</subject><subject>Earth and Environmental Science</subject><subject>Earth Sciences</subject><subject>Earth-ionosphere waveguide</subject><subject>Geophysics</subject><subject>Geophysics/Geodesy</subject><subject>Geotechnical Engineering & Applied Earth Sciences</subject><subject>Ionosphere</subject><subject>Lightning</subject><subject>Propagation</subject><subject>Structural Geology</subject><subject>Transient Luminous Events (TLEs)</subject><issn>1895-6572</issn><issn>1895-7455</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>C6C</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><recordid>eNqNkEFLw0AQhRdRsFbPXhe8Gjub7G6Sg0iRVguFCi1el8lmE1piUncTS_69W9ODBw9eZobhfe_BI-SWwQMTTExQl6YJQmAyAD_OyIglqQhiLsT56ZYiDi_JlXM7AMmBhSPyNKXrtst72hR0hrbqJ-uqOdD35Zy-Gdt2NsN229SOrjJn7JfJKbZ0Wlq8p4s63-I1uSiwcubmtMdkM59tnl-D5epl8TxdBpqDaAOTAqKWWmuTF8AjEFnCC9ApZAzRFCzGJElDiKMIMp5HyMOEcUDDZOrf0ZjcDbZ723x2xrVq13S29omKJVKEPBaJ9KrJoNK2cc6aQu3t9gNtrxioY0nqpyR1LEkdS_LE40AcsGqNzU1pu94fv-z_JiWPYiE8DwPvfFJd_gOMvgEuLnzY</recordid><startdate>20160601</startdate><enddate>20160601</enddate><creator>Pandey, Uma</creator><creator>Singh, Ashutosh K.</creator><creator>Singh, Om P.</creator><creator>Singh, Birbal</creator><creator>Saraswat, Vibhav K.</creator><general>Springer International Publishing</general><general>De Gruyter</general><general>Springer Nature B.V</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TG</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>FR3</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>KR7</scope><scope>L6V</scope><scope>L7M</scope><scope>M2P</scope><scope>M7S</scope><scope>P5Z</scope><scope>P62</scope><scope>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PTHSS</scope><scope>Q9U</scope></search><sort><creationdate>20160601</creationdate><title>A Study of Early/Slow VLF Perturbations Observed at Agra, India</title><author>Pandey, Uma ; 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During the period of observation (June-December 2011), we found 89 cases of VLF perturbation, while only 73 cases showing early character associated with strong lightning discharges. Out of 73 events, 64 (~84%) of the early VLF perturbations are found to be early/slow in nature; the remaining 9 events are early/fast. The onset duration of these early/slow VLF perturbations is up to ~ 5 s. A total of 54 observed early events show amplitude change lying between ± 3.0 dB, and phase change ± 12 degree, respectively, and found to occur mainly during nighttime. One of the interesting results we found is that the events with larger recovery time lie far away from the VLF propagation path, while events with smaller duration of recovery are within the ± 50–100 km of signal path. The World Wide Lightning Location Network (WWLLN) data is analysed to find the location of causative lightning and temporal variation. 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subjects | Atmospheric sciences early VLF perturbations Earth and Environmental Science Earth Sciences Earth-ionosphere waveguide Geophysics Geophysics/Geodesy Geotechnical Engineering & Applied Earth Sciences Ionosphere Lightning Propagation Structural Geology Transient Luminous Events (TLEs) |
title | A Study of Early/Slow VLF Perturbations Observed at Agra, India |
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