the support by National Key R&D Program of China(No.2022YFF0503403,2022YFF0711500);the support of National Natural Science Foundation of China(NSFC,grant Nos.11988101,12073047,12273077,12022306,12373048,12263005);the support from the Ministry of Science and Technology of China(Nos.2020SKA0110100);the science research grants from the China Manned Space Project(Nos.CMS-CSST-2021-B01,CMSCSST-2021-A01);CAS Project for Young Scientists in Basic Research(No.YSBR-062);the support from K.C.Wong Education Foundation。
The China Space Station Telescope(CSST)is a two-meter space telescope with multiple back-end instruments.The Fine Guidance Sensor(FGS)is an essential subsystem of the CSST Precision Image Stability System to ensure th...
supported by the National Key R&D Program of China(No.2022YFC2205303);the National Natural Science Foundation of China(11973078);the Chinese Academy of Sciences(CAS)“Light of West China”Program(2020XBQNXZ-018);the Natural Science Foundation of Xinjiang Uygur Autonomous Region(2022D01A358,2022D01A157);the Research on the science and technology partnership program and international science and technology cooperation program of Shanghai Cooperation Organization(2020E01041);partly supported by the Operation,Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments,budgeted from the Ministry of Finance of China(MOF)and administrated by Chinese Academy of Sciences。
The receiver is a signal receiving device placed at the focus of the telescope.In order to improve the observation efficiency,the concept of phased array receiver has been proposed in recent years,which places a small...
supported by the National Key Research and Development Program of China(2021YFC2203600);National Natural Science Foundation of China(Grant Nos.51975447 and 52005377);Youth Innovation Team of Shaanxi Universities under No.201926。
The influence of thermal deformation on the performance of reflector antennas has become increasingly significant with the increasing aperture and working frequency.The use of a thermal compensation database is an eff...
the National Natural Science Foundation of China 11703017,11790303(11790300),11803017,41774180,41904158,11973031;the China Postdoctoral Science Foundation(2019M652385);Open Research Program CAS Key Laboratory of Solar Activity;National Astronomical Observatories(KLSA201907);Young Scholars Program of Shandong University,Weihai(20820201005)。
Solar radio spectra and their temporal evolution provide important clues to understand the energy release and electron acceleration process in the corona,and are commonly used to diagnose critical parameters such as t...
The Five-hundred-meter Aperture Spherical radio Telescope(FAST)was launched on 2016 September 25.From early 2017,we began to use the FAST wideband receiver,which was designed,constructed and installed on the FAST in G...
With the proliferation of video traffic across the Internet and wireless networks,various compression standards for videos have emerged over the past two decades.Among them,Motion Joint Photographic Expects Group(M-JP...
For wavelength interrogation based surface plasmon resonance (SPR) sensors, refractive index (RI) resolution is an important parameter to evaluate the performance of the system. In this paper, we explore the influ...
supported by the National Natural Science Foundation of China(Nos.61205046,61401020,and 61575051);the Shenzhen Municipal Science and Technology Plan Project(Nos.JCYJ20150327155705357,KQCX2015032409501296,and JSGG20150529153336124,and JCYJ20150529114045265);the Hong Kong Government General Research Fund(GRF)(No.PolyU152079/14E)
We propose and experimentally demonstrate a universal and blind polarization-state tracking scheme for M-quadrature amplitude modulation(QAM) signals based on a decision-free radius-directed linear Kalman filter(RD...
Inline characterization for fabrication of silicon wafer PV (photovoltaic) devices may be used to optimize device efficiencies, reduce their performance variance, and their cost of production. In this article, the f...
supported by the dedicated operation funding forastronomical observation stations and facilities from the Chinese Academy of Sciences
An atmospheric turbulence phase screen generated using a fractal method is introduced. It is etched onto fused silica and tested in the laboratory. The etched screen has relatively low cost, high resolution, and can b...