首页|Optical complex for the study of pulsating aurora with sub-millisecond time resolution on the basis of the Verkhnetulomsky observatory
Optical complex for the study of pulsating aurora with sub-millisecond time resolution on the basis of the Verkhnetulomsky observatory
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NSTL
Elsevier
A new telescope-spectrometer was installed at Verkhnetulomsky observatory (68?36'N, 31?47'E) to supplement the data from all-sky cameras with measurements of the fine space-time structure of the auroral luminescence. The telescope uses 5 cm ultraviolet (UV) transparent lens as an optical system and a matrix of multi-anode photomultiplier tubes as a photo detector. The angular resolution of the telescope is 1.2? and the temporal resolution is 0.3 ms. The telescope observes a central part (20?) of the all-sky camera field of view (FOV). Description of both optical instruments and results of the first joint measurements are presented.
Belov, A. A.、Klimov, P. A.、Kozelov, B. V.、Barrillon, P.、Blin-Bondil, S.、Marszal, W.、Murashov, A. S.、Parizot, E.、Prevot, G.、Roldugin, A. V.、Szabelski, J.、Takizawa, Y.、Trofimov, D. A.、Sharakin, S. A.
NSTL
Elsevier
