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Astrophysics Research Centre

School of Mathematics and Physics


The Interferometric BIdimensional Spectrometer (IBIS; Cavallini 2006) is a high cadence imaging spectro-polarimeter based on a dual Fabry Perot interferometric system located at the DST. This system can isolate a narrow portion of the solar spectrum in the range of 5800−8600 Å and perform high resolution imaging spectroscopy.

public/solarflares/ibis.txt · Last modified: 2015/05/14 08:42 by David Kuridze

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