Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/2518
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dc.contributor.authorNarayanan, V.L.-
dc.contributor.authorGurubaran, S.-
dc.contributor.authorShiokawa, K.-
dc.date.accessioned2020-12-02T09:56:03Z-
dc.date.available2020-12-02T09:56:03Z-
dc.date.issued2016-
dc.identifier.citationJournal of Geophysical Research A: Space Physics,121(8),pp.7923-7931.en_US
dc.identifier.otherhttps://doi.org/10.1002/2016JA022861-
dc.identifier.urihttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1002/2016JA022861-
dc.identifier.urihttp://hdl.handle.net/123456789/2518-
dc.description.abstractIn this work we present direct ground‐based observational evidence for the merging of individual equatorial plasma bubbles (EPBs) obtained through the imaging of OI 630.0 nm airglow. Three potential mechanisms have been identified: (1) One of the EPBs tilts and reaches location of the adjacent growing EPB finally merging with it. (2) Some of the branches of an EPB arising from secondary instabilities reach out to adjacent EPB and merge with it. (3) The eastward zonal drift of the EPB on the eastern side slows down while the adjacent EPB on the western side drifts relatively faster and catches up. In one of the cases, a branch of an EPB was observed to get interchanged with another EPB as a result of merging and consequent pinching off from the parent EPB.en_US
dc.language.isoenen_US
dc.publisherAmerican Geophysical Unionen_US
dc.subjectEquatorial plasma bubblesen_US
dc.subjectOI 630.0 nm airglowen_US
dc.subjectEquatorial ionosphereen_US
dc.titleDirect observational evidence for the merging of equatorial plasma bubblesen_US
dc.typeArticleen_US
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