IBIS: A New Post-Focus Instrument for Solar Imaging Spectroscopy

By F. Cavallini. 2006

263 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

Multiwavelength Studies of MHD Waves in the Solar Chromosphere (2015, methodology): “Employing the IBIS instrument on the DST, Stangalini et al. (2011, 2012) and Sobotka et al. (2012, 2013) found evidence for magnetoacoustic waves, with periodicities in the range of 100–1000 s, leaking upwards into the chromosphere along the pore’s inclined magnetic fields.”
CRISPRED: A data pipeline for the CRISP imaging spectropolarimeter (2014, background): “During the past 20 years, a list of Fabry-Pérot interferometers (FPI) have been developed and installed in many ground based facilities and airborne missions, e.g: TESOS at the VTT (Kentischer et al. 1998; Tritschler et al. 2002), IBIS at the Dunn Solar Telescope (Cavallini 2006), CRISP at the Swedi”
Alfvén Waves in the Solar Atmosphere (2012, methodology): “Cauzzi et al. (2009) have used the Interferometric Bi-dimensional Spectrometer (IBIS; Cavallini 2006) to perform imaging spectroscopy of the solar chromospheric network in the Hα and Ca II 8542 Å line.”
The Interface Region Imaging Spectrograph (IRIS) (2012, methodology): “The conditions in the interface region present a signicant challenge to observers. Observations with Hinode and ground-based instruments such as the Interferometric Bidimensional Spectrometer (IBIS: Cavallini, 2006) at the Dunn Solar Telescope (DST) and the Crisp Imaging Spectropolarimeter (CRISP: S”