First Study of Optical Turbulence Over an Astronomical Site in the Central Himalayas Using ST Radar Observations

Autor: Aditya Jaiswal, Manish Naja, Samaresh Bhattacharjee, Brijesh Kumar, S. Ananthakrishnan
Rok vydání: 2023
Předmět:
Zdroj: Journal of Astronomical Instrumentation.
ISSN: 2251-1725
2251-1717
Popis: Optical turbulence in the atmosphere is a key factor which governs the sharpness of images produced from ground-based optical telescopes. The intensity of optical turbulence can be conveniently assessed by the estimation of the refractive index structure constant ([Formula: see text]). Here, observations from a stratosphere troposphere radar (206.5[Formula: see text]MHz) that is co-located with the optical telescope facilities in the central Himalayas, are used for the estimation of [Formula: see text]. The integrated profile of [Formula: see text] and winds over about 2–20[Formula: see text]km have been used to estimate seasonal and diurnal variation of “seeing”, wavefront coherence time, isoplanatic angle and scintillation rate. The mean [Formula: see text] over the site varies from 10[Formula: see text] to 10[Formula: see text][Formula: see text]m[Formula: see text] with the largest values in the monsoon and post-monsoon season. The best “seeing” conditions are observed in the winter and post-monsoon season with median “seeing” varying from 0.39[Formula: see text] to 0.81[Formula: see text]. The largest contribution to the diurnal variation of “seeing” comes from turbulences at 2–5[Formula: see text]km height region. A weak correlation of diurnal variation of “seeing” has been observed with surface temperature and relative humidity (RH). Among astroclimatic parameters, the largest isoplanatic angle is associated with winter season with median value of 2.57[Formula: see text] and wavefront coherence time of [Formula: see text]4.2[Formula: see text]ms. The least scintillation in intensity is observed in the winter season with a rate of [Formula: see text]10% and most in monsoon season with [Formula: see text]45% rate. This study is expected to have a positive impact on the optimization of the operation of adaptive optical techniques, observing time and scheduling of scientific programmes for optical telescope facilities in this region of the central Himalayas.
Databáze: OpenAIRE
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