Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6938
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dc.contributor.authorBanerjee, D-
dc.contributor.authorRitesh Patel-
dc.contributor.authorPant, V-
dc.contributor.authorADITYA Team-
dc.date.accessioned2020-11-12T14:52:45Z-
dc.date.available2020-11-12T14:52:45Z-
dc.date.issued2017-07-
dc.identifier.citationProceedings of the International Astronomical Union, Vol.335 , pp. 340-343en_US
dc.identifier.issn1743-9221-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/6938-
dc.descriptionRestricted Access © International Astronomical Union https://doi.org/10.1017/S1743921317008584en_US
dc.description.abstractVisible Emission Line Coronagraph (VELC) on board ADITYA-L1 is an internally occulted coronagraph with mirror as its primary objective element. It has a field of view (FOV) starting from 1.05 R –3R. It will observe the corona in continuum centered at 5000 ˚A and will perform spectroscopic observations of inner corona in two visible (5303 ˚A and 7892 ˚A) and one infrared (10747 ˚A) wavelengths. VELC will be capable of observing the corona with high spatial and temporal resolutions. We present an overview of the inner coronagraph (VELC) design and introduce the concept of an on-board automated coronal mass ejections (CMEs) detection logic proposed for this payload.en_US
dc.language.isoenen_US
dc.publisherInternational Astronomical Unionen_US
dc.subjectSunen_US
dc.subjectCoronal mass ejectionsen_US
dc.subjectCoronagraphen_US
dc.titleThe inner coronagraph on board ADITYA-L1 and automatic detection of CMEsen_US
dc.typeArticleen_US
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