Results 11 to 20 of about 477,612 (260)
The present study is aimed at the development of a novel empirical base for application to ground-based astronomical telescopes. A Weather Research and Forecasting (WRF) model is used for description of atmospheric flow structure with a high spatial ...
A. Y. Shikhovtsev +11 more
doaj +2 more sources
Astronomical seeing from the summits of the Antarctic plateau [PDF]
From the South Pole, microthermal turbulence within a narrow surface boundary layer some 200m thick provides the dominant contribution to the astronomical seeing. We present results for the seeing at a wavelength of 2.4um. The narrow turbulence layer above the site, confined close to the surface, provides greatly superior conditions for adaptive optics
R. D. Marks
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Astronomical seeing and ground-layer turbulence in the Canadian High Arctic [PDF]
We report results of a two-year campaign of measurements, during arctic winter darkness, of optical turbulence in the atmospheric boundary-layer above the Polar Environment Atmospheric Laboratory in northern Ellesmere Island (latitude +80 deg N).
Hickson, P. +3 more
openaire +3 more sources
Astronomical Seeing Prediction with Machine Learning
Abstract We investigate the use of supervised machine learning models to predict current atmospheric seeing at the Observatorio del Roque de Los Muchachos, La Palma. The prediction is made from current, local meteorological conditions as measured by an on-site weather station.
Fernando Abárzuza +5 more
openaire +2 more sources
رصد الأهلة في ظل تطور علوم الفلك والفضاء دراسة فقهية [PDF]
خَلَصَ هذا البحثُ إلى أنَّ علمَ الفلكِ وسيلةٌ لترسيخِ الإيمانِ بالخالقِ-سبحانهُ-، من خلالِ الاطِّلاعِ على هذا الكونِ المُتَرَامِي الأطرافَ إضافةً لارتباطِ هذا العلمِ بعباداتِ وأحوالِ شرعيَّةٍ تم توقيتُهَا بأزمنةٍ محددةٍ، متمثلةً في بداياتِ الشهورِ العربيّ
منى سالم محمد السيد محمد سلام
doaj +1 more source
Neural Network Based Point Spread Function Deconvolution For Astronomical Applications
Optical astronomical images are strongly affected by the point spread function (PSF) of the optical system and the atmosphere (seeing) which blurs the observed image.
Hong Wang +5 more
doaj +1 more source
On the Impact of ENSO Cycles and Climate Change on Telescope Sites in Northern Chile
The Atacama desert stands as the most arid, non-polar, region on Earth and has accommodated a considerable portion of the world’s ground-based astronomical observatories for an extended period.
Julia Victoria Seidel +2 more
doaj +1 more source
First day-time seeing observations at the Observatory of University of Zanjan in Iran [PDF]
Recognition of the appropriate locations for ground-based observations of the Sun with high angular resolution depends on the factors such as seeing, meteorological and astronomical parameters.
Pardis Ahmadi +3 more
doaj +1 more source
THE PROBABILITY OF SEEING THE CRESCENT WITH THE NAKED EYE. [PDF]
The aim of this study is to improve the static equation of the possibility of seeing the crescent. The factors (age of the moon, moon altitude, anomaly of the sun, the duration of stay Crescent (mukth)) for many years from (2004 to 2013 A.D) has been ...
BATOOL A. BENDER, MAJEED M. JARAD
doaj +1 more source
Method for Measuring the Second-Order Moment of Atmospheric Turbulence
The turbulence moment of order m (μm) is defined as the refractive index structure constant Cn2 integrated over the whole path z with path-weighting function zm. Optical effects of atmospheric turbulence are directly related to turbulence moments.
Hong Shen +3 more
doaj +1 more source

