The inner coronagraph on board ADITYA-L1 and automatic detection of CMEs

dc.contributor.author	Banerjee, D
dc.contributor.author	Ritesh Patel
dc.contributor.author	Pant, V
dc.contributor.author	ADITYA Team
dc.date.accessioned	2020-11-12T14:52:45Z
dc.date.available	2020-11-12T14:52:45Z
dc.date.issued	2017-07
dc.identifier.citation	Proceedings of the International Astronomical Union, Vol.335 , pp. 340-343	en_US
dc.identifier.issn	1743-9221
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/6938
dc.description	Restricted Access © International Astronomical Union https://doi.org/10.1017/S1743921317008584	en_US
dc.description.abstract	Visible 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.iso	en	en_US
dc.publisher	International Astronomical Union	en_US
dc.subject	Sun	en_US
dc.subject	Coronal mass ejections	en_US
dc.subject	Coronagraph	en_US
dc.title	The inner coronagraph on board ADITYA-L1 and automatic detection of CMEs	en_US
dc.type	Article	en_US