Articles | Volume 12, issue 1
https://doi.org/10.5194/gi-12-91-2023
https://doi.org/10.5194/gi-12-91-2023
Research article
 | 
04 May 2023
Research article |  | 04 May 2023

Spectral observations at the Canary Island Long-Baseline Observatory (CILBO): calibration and datasets

Joe Zender, Detlef Koschny, Regina Rudawska, Salvatore Vicinanza, Stefan Loehle, Martin Eberhart, Arne Meindl, Hans Smit, Lionel Marraffa, Rico Landman, and Daphne Stam

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Cited articles

Abe, S., Ogawa, T., Maeda, K., and Arai, T.: Sodium variation in Geminid meteoroids from (3200) Phaethon, Planet. Space Sci., 194, 105040, https://doi.org/10.1016/j.pss.2020.105040, 2020. a, b, c, d, e, f
Altwegg, K., Balsiger, H., Hänni, N., Rubin, M., Schuhmann, M., Schroeder, I., Sémon, T., Wampfler, S., Berthelier, J.-J., Briois, C., Combi, M., Gombosi, T. I., Cottin, H., De Keyser, J., Dhooghe, F., Fiethe, B., and Fuselier, S. A.: Evidence of ammonium salts in comet 67P as explanation for the nitrogen depletion in cometary comae, Nat. Astro., 4, 533–540, https://doi.org/10.1038/s41550-019-0991-9, 2020. a
Appenzeller, I.: Introduction to Astronomical Spectroscopy, Cambridge University Press, 145–178, ISBN 1139779524, 9781139779524, 2013. a
Bardyn, A., Baklouti, D., Cottin, H., Fray, N., Briois, C., Paquette, J., Stenzel, O., Engrand, C., Fischer, H., Hornung, K., Isnard, R., Langevin, Y., Lehto, H., Le Roy, L., Ligier, N., Merouane, S., Modica, P., Orthous-Daunay, F.-R., Rynö, J., Schulz, R., Silén, J., Thirkell, L., Varmuza, K., Zaprudin, B., Kissel, J., and Hilchenbach, M.: Carbon-rich dust in comet 67P/Churyumov-Gerasimenko measured by COSIMA/Rosetta, Mon. Not. R. Astron. Soc., 469, S712–S722, https://doi.org/10.1093/mnras/stx2640, 2017. a
Benneke, B. and Seager, S.: Atmospheric retrieval for super-earths: Uniquely constraining the atmospheric composition with transmission spectroscopy, Astrophys. J., 753, 100, https://doi.org/10.1088/0004-637X/753/2/100, 2012. a
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The paper describes the ground-based camera equipment to obtain images from dust ablation phenomena (meteors) in the Earth's atmosphere. The meteors are observed from two locations, but one station is equipped with a camera containing a spectral grating, which allows following and determining the spectral information through the meteor ablation process. We describe the data merging, calibration, and processing to finally derive the meteor composition.