High resolution IR-spectrometer . ... Determination of concentration of atmospheric greenhouse gases (carbon dioxide and methane) from ground-based or spacecraft platforms. ... Compact eschelle spectrometer is built by autocollimation scheme with diffraction grating operating in high orders of diffraction, allowing thereby to reach the resolution up to ?/ 20 000. ... For observations at the ground-based platforms and aboard the ISS the instrument modification RUSALKA will be used. ...

Next: The Reconstruction Up: Multiresolution with scaling Previous: Multiresolution with scaling . ... The cut-off frequency is reduced by a factor 2 at each step, allowing a reduction of the number of samples by this factor. The wavelet coefficients at the scale j+1 are: . ... The B-spline functions are compact in this directe space. ... We choose the scaling function which has a profile in the Fourier space: . ... The wavelet transform algorithm with scales is the following one: . ...

ERS -1,2 SAR . ... SIR-C/X SAR . ... European Remote Sensing Satellite (ERS-1) was launched on 17 July 1991, and the follow mission ERS-2 (with the same sensors and an Ozone monitoring instrument added) was launched on 21 April 1995. ... The Spaceborne Imaging Radar-C/X-band Synthetic Radar (SIR-C/X-SAR), carried in the cargo bay of the Space Shuttle Endeavour in April and October of 1994, simultaneously recorded SAR data at three wavelengths (L-, C-, and X-bands; 23.5, 5.8, and 3.1 cm, respectively). ...

... As part of my PhD I worked on various submillimetre instrumentation projects for the JCMT . As part of my PhD , I worked on commissioning HARP (Heterodyne Array Receiver Project), a new array spectrograph for the JCMT . ... As part of my PhD I helped to re-design the JCMT's high-frequency receiver (RxW) to operate as part of the eSMA, using HARP-design mixers and a new optics arrangement. ... Facilities that constitute the eSMA, from left to right the CSO, JCMT and SMA. ... 2010 Emily Curtis | ...

The beam pattern and the polarization characteristics . of the radio telescope RATAN-600 . The Mueller matrix elements was computed via formulas [1]: . ... The BP were computed by the aperture method, proceeding from the fild distribution in the aperture of the primary mirror. The components of the main and cross-polarization components of the electric field in the vertical aperture of the primary mirror was computed in Frenel diffraction approximation. ...

... You are here: start €Ё difx €Ё highspecres . ... difx:highspecres . ... largest read size to accomodate long FFTs maxReadSize = 40000000 # Correlate a 1 kHz portion of the input band centered on 4101.3 MHz ANTENNA FD { toneSelection=none filelist =fd. filelist addZoomFreq = freq@4101.2995 / bw@0.001 } ANTENNA KP { toneSelection=none filelist =kp. filelist addZoomFreq = freq@4101.2995 / bw@0.001 } ANTENNA NL { toneSelection=none filelist =nl. filelist addZoomFreq = ...

... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...

... It is particularly useful for the detection of close binaries, stellar asymmetries, and object diameters. ... Extraction of sub-regions of images would allow its use even for complicated objects like globular clusters. ... A number of other scientific projects for which it would be useful include tracking the expanding nebula in SN1987a, detection of close binaries in globular clusters, and search for asymmetries in giant and supergiant stars. ...