Formation of a rotating jet during the filament eruption on 2013 April 10–11

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dc.contributor.author Filippov, B.
dc.contributor.author Srivastava, A. K.
dc.contributor.author Dwivedi, B. N.
dc.contributor.author and et al
dc.date.accessioned 2020-03-09T06:54:21Z
dc.date.available 2020-03-09T06:54:21Z
dc.date.issued 2015-05-04
dc.identifier.issn 00358711
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/728
dc.description.abstract We analyse multiwavelength and multiviewpoint observations of a helically twisted plasma jet formed during a confined filament eruption on 2013 April 10-11. Given a rather large-scale event with its high spatial and temporal resolution observations, it allows us to clearly understand some new physical details about the formation and triggering mechanism of twisting jet. We identify a pre-existing flux rope associated with a sinistral filament, which was observed several days before the event. The confined eruption of the filament within a null-point topology, also known as an Eiffel tower (or inverted-Y) magnetic field configuration results in the formation of a twisted jet after the magnetic reconnection near a null point. The sign of helicity in the jet is found to be the same as that of the sign of helicity in the filament. Untwisting motion of the reconnected magnetic field lines gives rise to the accelerating plasma along the jet axis. The event clearly shows the twist injection from the pre-eruptive magnetic field to the jet. en_US
dc.language.iso en_US en_US
dc.publisher Oxford University Press en_US
dc.subject Sun: activity en_US
dc.subject Sun: filaments, prominences en_US
dc.subject Sun: magnetic fields en_US
dc.title Formation of a rotating jet during the filament eruption on 2013 April 10–11 en_US
dc.type Article en_US


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