Solar Spectra from the Gregor Infrared Spectrograph (GRIS)

GRIS (GREGOR Infrared Spectrograph) is the grating spectrograph installed at the GREGOR solar telescope. The spectrograph is mostly used in combination with the infrared detector of the Tenerife Infrared Polarimeter (TIP-II) to study the sun's photosphere and chromosphere. The slit length corresponds to some 60 arcsec, with a sampling of 0.13 arcsec.

In this EPN-TAP table, we provide GRIS scans starting in 2014. Data becomes public one year after the observeration.

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/leibniz-kis/gris/q/epn_core
Related Identifier http://dachs.sdc.leibniz-kis.de/tableinfo/gris.epn_core
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://leibniz-kis/gris/q/epn_core
Provenance
Creator The GRIS Team
Instrument GRIS
Publisher Leibniz Institute for Solar Physics KIS
Publication Year 2022
OpenAccess true
Contact KIS VO admin <dachs-admin(at)leibniz-kis.de>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Heliophysics; Natural Sciences; Physics