Preprints
https://doi.org/10.5194/egusphere-2026-5461
https://doi.org/10.5194/egusphere-2026-5461
26 Oct 2026
 | 26 Oct 2026
Status: this preprint is open for discussion and under review for Geoscientific Instrumentation, Methods and Data Systems (GI).

NORVIS: a portable broadband imaging spectrograph for auroral observations

Gaël Cessateur, Christian Buil, Guillaume Bertrand, Matthieu Le Lain, Valérie Desnoux, Olivier Garde, Hervé Lamy, Mathieu Barthelemy, Magnar Gullikstad Johnsen, David Bolsée, Urban Brändström, Antoine Calegaro, Fabien Darrouzet, Rowan Dayton-Oxland, Johan De Keyser, Maxime Grandin, Kirsti Kauristie, Romain Maggiolo, Sota Nanjo, and Noora Partamies

Abstract. We present NORVIS (NORdlys Versatile Imaging Spectrograph), a portable broadband imaging spectrograph developed for ground-based auroral observations. Based on the Star'Ex optical concept, NORVIS is optimized for auroral emissions and covers approximately 380–860 nm in a single acquisition at a moderate spectral resolution of 1.2 nm FWHM. The instrument combines auroral spectroscopy, wide-field context imaging, field operation, automated spectral reduction, and centralized data archiving within a researcher-citizen science framework. First observations were obtained during a campaign at Skibotn Observatory, Norway, in February 2026, during which approximately 1200 spectra were acquired and reduced over three observing nights, with typical exposure times of 30 s. These observations demonstrate the simultaneous detection of key auroral emissions, including the N2+ 1NG bands at 391.4 and 427.8 nm and the [O I] emissions at 557.7 and 630.0/636.4 nm, while also providing access to the Hα region and to O I emissions at 777.4 and 844.6 nm. Representative observations illustrate the potential of NORVIS for emission-ratio diagnostics and geometry-aware interpretation of auroral structures. NORVIS is intended to form the basis of a distributed observing network, with coordinated deployments planned in Kiruna, Skibotn, Svalbard, and northern Finland, followed by permanent installations at Kiruna, Skibotn, the Kjell Henriksen Observatory in Svalbard, and Nyrölä.

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Gaël Cessateur, Christian Buil, Guillaume Bertrand, Matthieu Le Lain, Valérie Desnoux, Olivier Garde, Hervé Lamy, Mathieu Barthelemy, Magnar Gullikstad Johnsen, David Bolsée, Urban Brändström, Antoine Calegaro, Fabien Darrouzet, Rowan Dayton-Oxland, Johan De Keyser, Maxime Grandin, Kirsti Kauristie, Romain Maggiolo, Sota Nanjo, and Noora Partamies

Status: open (until 01 Dec 2026)

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Gaël Cessateur, Christian Buil, Guillaume Bertrand, Matthieu Le Lain, Valérie Desnoux, Olivier Garde, Hervé Lamy, Mathieu Barthelemy, Magnar Gullikstad Johnsen, David Bolsée, Urban Brändström, Antoine Calegaro, Fabien Darrouzet, Rowan Dayton-Oxland, Johan De Keyser, Maxime Grandin, Kirsti Kauristie, Romain Maggiolo, Sota Nanjo, and Noora Partamies
Gaël Cessateur, Christian Buil, Guillaume Bertrand, Matthieu Le Lain, Valérie Desnoux, Olivier Garde, Hervé Lamy, Mathieu Barthelemy, Magnar Gullikstad Johnsen, David Bolsée, Urban Brändström, Antoine Calegaro, Fabien Darrouzet, Rowan Dayton-Oxland, Johan De Keyser, Maxime Grandin, Kirsti Kauristie, Romain Maggiolo, Sota Nanjo, and Noora Partamies
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Latest update: 26 Oct 2026
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Short summary
We developed a compact, portable instrument that records the colours of auroras across a broad range of visible and near-infrared light. Field tests in northern Norway showed that it can capture several important auroral emissions at the same time and can be operated with simple portable equipment. This makes it suitable for coordinated observations from multiple sites, helping researchers study how auroras vary in space and time.
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