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36 results about "Airglow" patented technology

Airglow (also called nightglow) is a faint emission of light by a planetary atmosphere. In the case of Earth's atmosphere, this optical phenomenon causes the night sky to never be completely dark, even after the effects of starlight and diffused sunlight from the far side are removed.

Wide spectral segment non-focusing all-day airglow imager

PendingCN109656006AReduced surface quality requirementsEliminate positional chromatic aberrationSpectrum investigationMountingsCamera lensImaging lens
The invention relates to an airglow imager. In order to solve the problems that an existing airglow imager is small in detecting view field and narrow in spectral range and needs to adopt a mechanicalfocusing device, so that the structure of the existing imager and using operation are complex, and the luminous flux of the existing imager is low, the wide spectral segment non-focusing all-day airglow imager is provided. The imager comprises an image space telecentric fish-eye lens, an object space telecentric imaging lens and a detector; a filter wheel is arranged between the fish-eye lens andthe imaging lens, a plurality of narrow band filters with different wave bands and the focal power of zero are arranged on the filter wheel, and the narrow band filters can be switched to a focal plane of the fish-eye lens through the filter wheel; the fish-eye lens comprises a negative light focal power front lens set and a positive light focal power back lens set, and an aperture diaphragm is arranged on a light path between the front lens set and the back lens set; the imaging lens comprises a plurality of gluing lenses composed of plus lenses and concave lenses, the absolute value of a relative abbe number difference value of the plus lenses and the concave lenses is greater than or equal to 5, and the absolute value of a relative dispersion difference value of the plus lenses and theconcave lenses is less than or equal to 0.001.
Owner:XI'AN INST OF OPTICS & FINE MECHANICS - CHINESE ACAD OF SCI

All-sky atmospheric gravity wave imaging instrument adopting fish eye lens and telecentric beam path

The invention provides an all-sky atmospheric gravity wave imaging instrument adopting a fish eye lens and a telecentric beam path, which comprises the No. F2.8 fish eye lens with the focus of 10.5mm, a telecentric lens, a circular light filter with the diameter of 3 inches, a focus reducing lens group, an imaging lens and a scientific grade CCD camera, and OH, O2, OI, Na and other airglows are radiated as tracers, thereby realizing the all-sky atmospheric gravity wave imaging. The telecentric lens is placed in the rear position of a focal plane of the fish eye lens, thereby leading emergent light to meet the requirements on the angle of incident light of the light filter; and then the light sequentially passes through the circular light filter, the focus reducing lens group for focusing and adjusting aberration, the imaging lens and the connected scientific grade CCD camera, thereby realizing the all-sky 180-degree atmospheric gravity wave imaging. The all-sky atmospheric gravity wave imaging instrument utilizes the No. F2.8 fish eye lens with the focus of 10.5mm which is commercially universal at present and is matched with the multi-channel light filter with 3 inches, thereby being more economic and convenient to realize the multi-channel all-sky gravity wave imaging on the basis of ensuring the high light throughput of the whole system.
Owner:NAT SPACE SCI CENT CAS

Method for quantitatively calculating optical observation light pollution

The invention provides a method for quantitatively calculating optical observation light pollution. The method comprises the following steps: establishing a yellow channel light semaphore simulation model, an air glow semaphore simulation model, a galaxy light semaphore simulation model and an atmospheric scattering light semaphore simulation model; performing actual observation by using an optical telescope to obtain a night-sky light observation semaphore; carrying out simulation calculation by utilizing the established simulation model to obtain a yellow channel optical semaphore, an airglow semaphore, a silver river system optical semaphore and an atmospheric scattered light semaphore; summing and calculating according to the obtained semaphore of the night-sky light component to obtain a night-sky light semaphore; and calculating the difference between the night-sky light observation semaphore obtained by the optical telescope and the night-sky light semaphore obtained by simulation calculation to obtain the light pollution observation semaphore. According to the method, quantitative calculation of the light pollution observation semaphore is achieved, large errors caused by analyzing light pollution through data observed by observation equipment are avoided, and initial site selection of the observatory and analysis and research in the optical observation process are facilitated.
Owner:SHANDONG UNIV

Upper atmosphere airglow blast-temperature imager for atomic frequency discrimination

The invention discloses an upper atmosphere airglow blast-temperature imager for atomic frequency discrimination, which is used for airglow detection of space atmosphere. The imager comprises a receiving telescope (4), an optical filter (5), a spectral component (6), a center-band atomic frequency discrimination component (31), a left and a right side band atomic frequency components (11, 12), three imaging lens (12, 22, 32) and three imaging CCDs (13, 23, 33). The imager allocates the received airglow to a center-band atomic frequency discrimination channel (3) and the left and the right side band automatic frequency discrimination channels (1, 2), obtains the intensities of the full airglow spectrum, the left edge spectrum and the right edge spectrum respectively, and obtains the intensity of the airglow and the distribution of the temperature and the wind field of the atmosphere at the location issuing the airglow simultaneously. The invention has the advantages that multi detection functions are provided, the wave length is stable without drift, the precision of frequency discrimination is high, the detection error is small, and the work is stable and reliable.
Owner:WUHAN INST OF PHYSICS & MATHEMATICS CHINESE ACADEMY OF SCI
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