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94 results about "Radio astronomy" patented technology

Radio astronomy is a subfield of astronomy that studies celestial objects at radio frequencies. The first detection of radio waves from an astronomical object was in 1932, when Karl Jansky at Bell Telephone Laboratories observed radiation coming from the Milky Way. Subsequent observations have identified a number of different sources of radio emission. These include stars and galaxies, as well as entirely new classes of objects, such as radio galaxies, quasars, pulsars, and masers. The discovery of the cosmic microwave background radiation, regarded as evidence for the Big Bang theory, was made through radio astronomy.

Sub-aperture sidelobe and alias mitigation techniques

Methods for mitigating sidelobes and aliases, providing levels of suppression in excess of 20 dB. The methods may include 1) a version of the CLEAN algorithm developed in radio astronomy, modified to work on sub-aperture images; 2) weighting functions based on the phase and amplitude statistics of the sub-aperture image pixels to select points in the CLEAN algorithm; and 3) weighting functions based on the phase and amplitude statistics of the sub-aperture image pixels to mitigate sidelobes and aliases, in conjunction with CLEAN or separately. The methods may be used with all synthetic aperture techniques and are not limited to SAR.
Owner:NORTHROP GRUMMAN SYST CORP

Solar radio total power radiometer system in radio astronomy protection frequency band based on broadband detection chip

The invention provides a solar radio total power radiometer system in radio astronomy protection frequency band based on a broadband detection chip. The system works in the radio astronomy protection frequency band and carries out filtering, gating, amplification, detection and analysis on frequency band signals. The system is characterized in that the system is formed by connecting a calibration module and a control unit thereof with a radio-frequency signal detection unit. The beneficial effects of the system are that the system has the advantages that the system receives less radio interference; and compared with a conventional superheterodyne mode, the detection broadband is wider and large in dynamic range, and the structure is simple and the like.
Owner:YUNNAN ASTRONOMICAL OBSERVATORY CHINESE ACAD OF SCI

Short-centimeter-waveband dual-polarized refrigeration receiver dewar

InactiveCN103248375AImprove sealingEasy initial assemblyTransmissionEngineeringPolarizer
The invention relates to a 1.3-centimeter-waveband dual-polarized refrigeration receiver dewar used for observing molecular spectra lines, pulsar and VLBI (very long baseline interferometry) in the radio astronomy. The receiver dewar consists of a dewar cavity, a shielding cover, a microwave window, a frame carrier, a support, a ring-shaped fixing frame, a soft connector, a feed source, a transition waveguide, a circle and square converter, a polarizer, a low-noise amplifier, a waveguide coaxial converter, an isolator, a semi-rigid coaxial cable, a microwave window sealing film, a microwave window fastening ring, an air-filled cavity, an air-filled cavity sealing film, an air-filled cavity fastening ring, an air cylinder and a refrigerator. The 1.3-centimeter-waveband dual-polarized refrigeration receiver dewar with high sensitivity has the advantages that the design scheme is more reasonable, good sealing performance is ensured, internal devices can be well fixed and supported, the refrigeration effect is more excellent, the stability is better, the sensitivity is higher, and the thermal radiation can be effectively isolated, thereby being capable of being better applied to high frequence radiation characteristic study of molecular spectra lines and pulsar and radio astronomy observation of VLBI.
Owner:XINJIANG ASTRONOMICAL OBSERVATORY CHINESE ACADEMY OF SCI

Light-weight die for high-precision large-sized antenna for radio astronomy and manufacturing method thereof

The invention discloses a light-weight die for a high-precision large-sized antenna for radio astronomy and a manufacturing method thereof. The light-weight die consists of a plurality of die units, wherein each die unit comprises a die molding surface and a rigid structure used for supporting the die molding surface; each rigid structure comprises a steel frame and a plurality of steel diaphragms; each die molding surface comprises a molding surface square pipe layer, a glass fiber reinforced plastics layer and a resin layer; each resin layer adopts epoxy tooling board or machinable plastic pasting; a high-precision molding surface of each die unit is realized by machining; the airtightness of the die is realized by spraying gel coat on non-antenna areas of the resin layers; the die splicing is realized by center line positioning and high-precision adjustment; sealing grooves among the die units are filled and leveled up by adopting resin pasting; and the manufacturing of the high-precision large-sized antenna for radio astronomy is realized.
Owner:NO 54 INST OF CHINA ELECTRONICS SCI & TECH GRP +1

Large radio astronomical telescope common-drive parallel connected array mechanism

InactiveCN1892281AReduce the numberAchieve a wide range of fitting motionTelescopesElectric machineryAstronomical telescopes
Large radio astronomy telescope co-driving parallel connection array mechanism belongs to physical construction designing technology field, in particular relating to co-driving parallel connection mechanism array having strong coupling character. It featuring that: each unit lower end connected with base through guiding constraint branched chain for restricting reflection plane unit rotating at horizontal direction, one active branched chain located below all nonadjacent peak, through one telescopic link flex action to control above three reflection plane units cooperation movement. The present invention can realize reflection plane long range matching movement on occasions of reducing drive motor number.
Owner:NAT ASTRONOMICAL OBSERVATORIES CHINESE ACAD OF SCI +1

Radio astronomy narrow band spectral line observation platform based on agile transceiver

ActiveCN105510712ARealize switching observation with high spectral resolutionExcellent time resolution in millisecondsFrequency analysisFrequency spectrumAutomatic control
A radio astronomy narrow band spectral line observation platform based on an agile transceiver consists of an agile transceiver AD9361 circuit board, an FPGA control circuit board and a control computer which are connected in sequence. The input signal bandwidth of the agile transceiver AD9361 circuit board can reach DC-6GHz, a signal input end of the agile transceiver AD9361 circuit board is connected with a radio frequency output end of a radio astronomy telescope, a control end and a data output end of the agile transceiver AD9361 circuit board are connected with the FPGA control circuit board, the FPGA control circuit board is connected with the main control computer through a network port, control software is integrated at the main control computer, and parameters including a center frequency point, observation bandwidth and AGC (automatic gain control) gain are sent to the AD 9361 through an FPGA chip on the platform according to the narrow band spectral line radio source red shift, the center frequency point, the contour extension and other parameters. As for observation targets of a narrow band spectral line in radio astronomy, the invention has the advantages of high band-pass selection flexibility, high spectral resolution and the like as compared with a conventional device.
Owner:YUNNAN ASTRONOMICAL OBSERVATORY CHINESE ACAD OF SCI

Classification of interference

An interference classifier is disclosed for determining the type of interference present in a signal. The interference classifier 601 comprises a buffer 602 operable to receive and store data comprising samples of a signal; a scale factor calculator 603 operable to use the signal samples to calculate a scale factor in dependence upon the levels of the signal samples; a normaliser 604 operable to calculate normalised signal samples by using the scale factor to normalise the signal samples; a nonlinear transformer 605 operable to perform a nonlinear transform on the normalised signal samples to calculate transformed signal samples; an averaging circuit 606 operable to calculate an average of the transformed signal samples; and a comparator 607 operable to compare the calculated average of the transformed signal samples to a predetermined threshold level in order to determine the type of interference present in the received signal. The interference classifier 601 disclosed herein performs an advantageous type of nonlinear transform that provides an improvement in detection probability over known kurtosis-based interference classifiers. Applications of the interference classifier 601 include automotive radar systems, radio astronomy, microwave radiometry, weather forecasting and cognitive radio networks.
Owner:MITSUBISHI ELECTRIC CORP

Si substrate field effect transistor terahertz detector antenna based on CMOS manufacturing process

The invention discloses a Si substrate field effect transistor terahertz detector antenna based on a CMOS manufacturing process, and belongs to the field of antennas. The Si substrate field effect transistor terahertz detector antenna comprises a semi-circular micro-strip patch antenna body with a T-shaped groove, a silicon substrate FET and a low-noise amplifier; the semi-circular micro-strip patch antenna body is used for receiving THz waves, converting the received THz waves into electric signals, and sending the electric signals to the FET, the FET converts high-frequency signals into low-frequency signals and sends the low-frequency signals to the low-noise amplifier, and detection of THz signals can be finally achieved after the signals are amplified by the low-noise amplifier. The Si substrate field effect transistor terahertz detector antenna has important application in the fields of security scanning, radio astronomy, biologic remote sensing, production monitoring and the like.
Owner:TIANJIN POLYTECHNIC UNIV

Self-powered, self-propelled computer grid with loop topology

An energy-harvesting compute grid includes computing assemblies that cooperate with mobile energy harvesters configured to be deployed on a body of water. The plurality of energy harvesters are positioned on and move adjacent to an upper surface of a body of water, and the locations of the energy harvesters can be monitored and controlled. The wide-spread gathering by the harvesters of environmental data within that geospatial area permits the forecasting of environmental factors, the discovery of advantageous energy-harvesting opportunities, the observation and tracking of hazardous objects and conditions, the efficient distribution of data and / or tasks to and between the harvesters included in the compute grid, the efficient execution of logistical operations to support, upgrade, maintain, and repair the cluster, and the opportunity to execute data-gathering across an area much larger than that afforded by an individual harvester (e.g., radio astronomy, 3D tracking of and recording of the communication patterns of marine mammals, etc.). The computational tasks can be shared and distributed among a compute grid implemented in part by a collection of individual floating self-propelled energy harvesters thereby providing many benefits related to cost and efficiency that are unavailable to relatively isolated energy harvesters, and likewise unavailable to terrestrial compute grids of the prior art.
Owner:LONE GULL HLDG LTD

Coal bed gas radio spectrum direction-finding early warning system

The invention discloses a coal bed gas radio spectrum direction-finding early warning system. A radio astronomy modulation radiation receiving system is used to receive gas radio steady state and unsteady state radiation temperature signals in a gas enriched region in a coal bed so as to indirectly measure the coal bed gas pressure; a radio astronomy full-power radiation receiving system is used to receive gas radio unsteady state and quickly variable radiation intensity and form signals in the gas enriched region in the coal bed so as to judge the gas radio radiation type and variation rate; and a radio astronomy spectrum radiation receiving system is used to receive gas radio unsteady state and quickly variable radiation spectrum peak and frequency drift in the gas enriched region in the coal bed so as to early warn the coal gas outburst. Due to the fit of the maximum values of the three signals under different antenna bearings and elevations, and the trigonometry measurement, the direction and normal distance of the gas enriched region are measured.
Owner:南京紫淮矿用电子高科技有限公司 +2

Si-based field effect transistor annular terahertz detector antenna based on CMOS manufacturing process

The invention discloses a Si-based FET annular THz detector antenna based on a CMOS manufacturing process, and belongs to the field of antennas. The Si-based FET annular THz detector antenna comprises an annular antenna body, a Si-based FET and a low noise amplifier. The annular antenna body is used for receiving THz waves and meanwhile converting the received THz waves into electric signals to be transmitted to the FET, high-frequency signals are converted into low-frequency signals by the FET and are transmitted to the low noise amplifier, and finally the THz signals can be detected after the signals pass through the low noise amplifier. The Si-based FET annular THz detector antenna is importantly applied to security scanning, radio astronomy, biological remote sensing, production monitoring and other fields.
Owner:TIANJIN POLYTECHNIC UNIV

Low-temperature 3GHz-9GHz wide-temperature-range ultra-wide-band microwave isolator and application

The invention provides a 3GHz-9GHz frequency-band ultra-wide-band microwave isolator working in a low-temperature environment. The 3GHz-9GHz frequency-band ultra-wide-band microwave isolator working in the low-temperature environment comprises ferrite, wherein the ferrite is made from YAlIG-10A, wherein the content of Al2O3 is 2.43%, when the material is 300 K, the saturation magnetization 4piMs equals to 880 Gauss, when the material is 100 K, 4piMs equals to 1300 Gauss, and when the material is 4 K, 4piMs equals to 1350 Gauss. The gap of research of a domestic low-temperature ultra-wide-bandmicrowave isolator is filled, a key device is provided for a front end system of a low-noise radar receiver such as radio astronomy, at the low temperature of 4K-100 K, the relative working bandwidthis 100%, the reverse isolation is high, insertion loss is low, and the requirement of a super-conductive receiver system to the low-temperature ultra-wide-band microwave isolator can be met.
Owner:ZIJINSHAN ASTRONOMICAL OBSERVATORY CHINESE ACAD OF SCI

Broadband dual-linearly-polarized or dual-circularly-polarized feed source

The invention discloses a broadband dual-linearly-polarized or dual-circularly-polarized feed source in the fields of wireless communication and radio astronomy. The broadband feed source consists of four groups of radiation oscillators, 2 impedance-matched printed boards and a circularly-polarized electric bridge, wherein the radiation oscillators are log periodic dipole arrays, and are connected with the two impedance-matched printed boards which are orthogonally arranged, so that impedance values of the wide ends of metal microstrip lines of the impedance-matched printed boards are 1 / 4 of impedance values between left and right pins of the radiation oscillators, so that feeding is simplified, and high performance is achieved. The broadband feed source is simple and compact in structure, low in feed loss and machining cost, high in feed efficiency and particularly applicable to a feed network of a feed source or antenna working under a broadband dual-linear-polarization or dual-circular-polarization application condition.
Owner:NO 54 INST OF CHINA ELECTRONICS SCI & TECH GRP

C-band isolator for liquid helium and liquid helium temperature region, and application of isolator

The invention provides a C-band isolator for liquid helium and liquid helium temperature regions. The C-band isolator comprises ferrite which is made from YA1IG-6A, wherein the content of Al2O3 is 5.24%; when the material is 300K, the saturation magnetization intensity 4piMs is equal to 590 Gauss; and when the material is 4K, the saturation magnetization intensity 4piMs is equal to 980 Gauss. The C-band isolator makes up the blank of the research of a low temperature isolator in China, provides a key device for a front-end system of a low noise radar receiver of radio astronomy and the like, has the relative operating bandwidth of more than 21% at the low temperature of 4K-90K, is high in isolation degree and low in insertion loss, and can meet the demand on a low temperature isolator of a superconducting receiver system.
Owner:ZIJINSHAN ASTRONOMICAL OBSERVATORY CHINESE ACAD OF SCI

Self-powered, self-propelled computer grid with loop topology

An energy-harvesting compute grid includes computing assemblies that cooperate with mobile energy harvesters configured to be deployed on a body of water. The plurality of energy harvesters are positioned on and move adjacent to an upper surface of a body of water, and the locations of the energy harvesters can be monitored and controlled. The wide-spread gathering by the harvesters of environmental data within that geospatial area permits the forecasting of environmental factors, the discovery of advantageous energy-harvesting opportunities, the observation and tracking of hazardous objects and conditions, the efficient distribution of data and / or tasks to and between the harvesters included in the compute grid, the efficient execution of logistical operations to support, upgrade, maintain, and repair the cluster, and the opportunity to execute data-gathering across an area much larger than that afforded by an individual harvester (e.g., radio astronomy, 3D tracking of and recording of the communication patterns of marine mammals, etc.). The computational tasks can be shared and distributed among a compute grid implemented in part by a collection of individual floating self-propelled energy harvesters thereby providing many benefits related to cost and efficiency that are unavailable to relatively isolated energy harvesters, and likewise unavailable to terrestrial compute grids of the prior art.
Owner:LONE GULL HLDG LTD

Interference testing system between millimeter wave radar and radio astronomy

ActiveCN108226885AGuaranteed authenticityAvoid the adverse effects of interferenceWave based measurement systemsFrequency spectrumSpectrograph
The invention provides an interference testing system between millimeter wave radar and radio astronomy. The interference testing system comprises an electromagnetic shielding chamber, a horn antenna,a radar simulator and a high-precision frequency spectrograph, wherein the horn antenna is matched with the frequency band of the tested millimeter wave radar, is arranged in the electromagnetic shielding chamber and is opposite to the millimeter wave radar; the distance between the horn antenna and the tested millimeter wave radar is smaller than a preset value; the radar simulator is arranged in the electromagnetic shielding chamber; the signal input end of the radar simulator is connected with the horn antenna and is used for simulating an electromagnetic environment in a current testing environment and current testing distance; the high-precision frequency spectrograph is arranged in the electromagnetic shielding chamber; the signal input end of the high-precision frequency spectrograph is connected with the signal output end of the radar simulator; the high-precision frequency spectrograph is used for simulating the radio astronomy and outputs signal intensity inputted from the signal input end of the high-precision frequency spectrograph to the high-precision frequency spectrograph. The interference testing system between the millimeter wave radar and the radio astronomy, provided by the invention, has the advantages that complexity and high possibility of making errors for obtaining the result are reduced, and a large amount of consumption of labor force and physical force in an actual external field test is avoided.
Owner:THE STATE RADIO MONITORING CENT TESTING CENT

Processing method and processing devices used for radio astronomy data and storage medium

The invention discloses a processing method used for radio astronomy data. Firstly, a target data amount and the number of preset threads are obtained; then the target data amount is divided to obtaina plurality of target data blocks; and finally, the target data blocks are allocated for all threads by a predefined rule to enable all the threads to carry out simultaneous calculation of the targetdata amount. Therefore, in the scheme, the target data amount is divided, and then allocated to the multiple threads for simultaneous processing, the method greatly reduces time, which is required for calculation of the data amount, as compared with a manner of using a single thread for processing on the target data amount in the prior art, at the same time, the target data can be processed quickly, thus it is guaranteed that cache space thereof can be released as soon as possible, and a utilization rate of the cache space is improved. In addition, the invention also discloses processing devices used for the radio astronomy data and a storage medium, of which effects are as above.
Owner:INSPUR BEIJING ELECTRONICS INFORMATION IND

Complex electronic system double-layer electromagnetic shielding structure with motion platform

The invention discloses a complex electronic system double-layer electromagnetic shielding structure with a motion platform. The double-layer electromagnetic shielding structure comprises an outer layer shielding body and an inner layer shielding compartment, wherein the outer layer shielding body comprises a cabin formed by welding a metal plate and shielding cloth used for connecting the cabin with the motion platform, the inner layer shielding compartment is welded to the inner wall of the cabin, and electric and electronic equipment capable of generating strong interference is arranged in the inner layer shielding compartment. The shielding structure has generality, through the mode of combining the metal shielding body and the flexible shielding material and additionally arranging the shielding compartment, electromagnetic interference of the electric and electronic equipment in the cabin is shielded in a double layer mode, the highest 120 dB shielding efficiency requirement of national and military standard GJB 151A-1997<requirement for military equipment and subsystem electromagnetic emission and sensitiveness> can be met, and therefore the requirement for overall shielding efficiency of radio astronomy and other high-sensitivity detection equipment can be met.
Owner:NAT ASTRONOMICAL OBSERVATORIES CHINESE ACAD OF SCI

Temperature compensation voltage-multiplying diode detector for ultra high frequency range

The invention relates to a temperature compensation voltage-multiplying diode detector for an ultra high frequency range. An ultra high frequency silicon crystal audion is adopted to enable a node C and a node B to form a short circuit, and an EB node of the short circuit is utilized to form an ultra high frequency diode. Four CB nodes of the four audions separately form short circuits to form four diodes formed by the EB nodes, and every two of the four diodes are connected in series to form a double EB node voltage-multiplying detector of double-difference geminate transistors. The invention has the advantages of high upper frequency limit reaching 300 MHz or higher, low temperature drifting, good detection linearity, large dynamic range, high output detection voltage and low detection threshold value, thereby having low requirement on the output level of the system before detection and greatly widening the dynamic range of radio astronomy total strength amplitude receiving equipment.
Owner:南京紫淮矿用电子高科技有限公司 +2

Dual-purpose science popularization system for radio astronomy and amateur radio communication

The invention discloses a dual-purpose science popularization system for radio astronomy and amateur radio communication. The system comprises a miniature parabola antenna, an equatorial instrument, a program controlled one-out-of-two switch, more than one low-noise amplifier, more than one power amplifier, a software radio transceiver, a GPS timing antenna and a computer. The system provided by the invention can realize observation of multiple strong source signals of radio astronomy and experience of a radio communication technology, can enable science popularization audience to fully understand knowledge in such two aspects, i.e., radio astronomy science and radio science and is simple in apparatus structure, thereby being suitable for industrial production and market promotion and application.
Owner:YUNNAN ASTRONOMICAL OBSERVATORY CHINESE ACAD OF SCI +2

Self-balancing mechanism of macrotype radio astronomy telescope source-feed locating platform

The invention relates to a big radio astronomical telescope feed local platform self-balancing device with inhibiting vibration and self-balancing ability. It is made up of the upper platform, Hook ream-spring device, four supporting rods, connecting rod and low platform. The invention provides a self-balancing device to connect the first and second rank local devices. When the low platform vibrates, the Hook ream can adjust self and the spring has pretightening force which can accelerate the adjustment to balance the feed platform quickly and improve the precision of feed source location. So it can keep the balance of second location device of feed source to reach the precision of the feed source device.
Owner:TSINGHUA UNIV

High-precision posture continuous adjusting device for reflector antenna panel and manufacturing method thereof

PendingCN110289476AContinuously adjustable implementationOvercome the lack of axial adjustmentAntenna supports/mountingsEngineeringRadio astronomy
The invention discloses a high-precision posture continuous adjusting device for a reflector antenna panel and a manufacturing method thereof and relates to the field of communication, measurement and control and radio astronomy. The adjusting device includes a positioning mechanism and an adjusting mechanism, wherein the positioning mechanism mainly includes a main support rod, an independent support rod, a first direction connecting plate, a second direction connecting plate, a nut, a spherical washer and a tapered washer, the adjusting mechanism mainly includes a V-shaped rod, a transverse rod, an upper support and a lower support, the positioning mechanism and the adjusting mechanism are hinged with an antenna panel, and design length of the adjusting mechanism can be obtained according to a given calculation formula. The adjusting device is advantaged in that the adjusting device realizes the omnidirectional high-precision continuous adjusting function of the antenna panel, improves position precision of the panel in the antenna pitching motion process and improves panel adjusting efficiency in the antenna installation process.
Owner:NO 54 INST OF CHINA ELECTRONICS SCI & TECH GRP

Balun combiner integrated feed network

ActiveCN104466411AMinimize impedance matching problemsRealize Impedance TransformationSimultaneous aerial operationsElectrical conductorImpedance matching
The invention discloses a balun combiner integrated feed network in the field of wireless communication and radio astronomy. The balun combiner integrated feed network comprises a first impedance matching printed board and is characterized in that the front face of the impedance matching printed board is provided with two gradual-change type metal microstrip lines, narrow ends of the two metal microstrip lines are each provided with an antenna connector, wide ends of the two metal microstrip lines are connected with coaxial port inner conductors respectively, the back face of the impedance matching printed board is provided with two gradual-change type metal microstrip ground wires, narrow ends of the two metal microstrip ground wires are each provided with an antenna connector, and wide ends of the two metal microstrip ground wires connected with coaxial port outer conductors respectively. The balun combiner integrated feed network has the advantages that impedance conversion is achieved, balance-unbalance port conversion is achieved, port forming is achieved, loss is low, feed efficiency is high, the structure is compact, machining cost is low, and the balun combiner integrated feed network is very suitable for an antenna working under the situation of wide-band double-wire polarization or double-circle polarization application.
Owner:NO 54 INST OF CHINA ELECTRONICS SCI & TECH GRP

A digital fft spectrum analyzer system and operating method

The invention discloses a digital FFT (fast Fourier transform) frequency spectrograph system. The digital FFT (fast Fourier transform) frequency spectrograph system comprises a graphical interface module, a data processing module and a communication module. The graphical interface module is connected with the data processing module and the communication module. The data processing module is connected with the communication module. The graphical interface module creates user interfaces as well as threads of the data processing module and the communication module. The data processing module comprises two spectrum analyzer board cards, and has a local mode and a remote mode. The communication module is in communication connection with a dispatching computer, is provided with a signal lamp marking position, and comprises a storage module. Through a giga network, a large quantity of OTF (optical transfer function) data and standard source data are stored into a disk array remotely. The invention further discloses an operation method of the digital FFT frequency spectrograph system. The digital FFT frequency spectrograph system and the operation method thereof have the advantages of broadband, high frequency resolution, wide dynamic range, long-time-scale system stability, capability of subjecting radio astronomy signals or terahertz atmosphere signals to broadband high-resolution real-time frequency spectrum treatment and the like.
Owner:ZIJINSHAN ASTRONOMICAL OBSERVATORY CHINESE ACAD OF SCI

Electromagnetic shielding cabin for high-accuracy laser distance measurement equipment

The invention discloses an electromagnetic shielding cabin for high-accuracy laser distance measurement equipment. The electromagnetic shielding cabin comprises a shell, wherein the shell is formed bywelding a metal plate, a high-transmitting conductive shielding cover is arranged at an upper part in a front side wall of the shell and is electrically connected with the shell, a rear side wall ofthe shell is detachably connected with the shell, a power filter and a signal filter are arranged at a lower part of a side wall of the shell, ventilation waveguide windows are formed in an upper partand a lower part of the side wall of the shell, and a fixed bolt is arranged at the bottom of the shell and is used for fixing the distance measurement equipment. The electromagnetic shielding cabinhas universality and can be used as a reference for electromagnetic compatibility design or improvement of optical measurement equipment which has high shielding efficiency requirement and is used fordeveloping dynamic high-accuracy measurement; and by combining a metal shielding body and a conductive transmitting shielding material, electromagnetic interference of the measurement equipment in the cabin is shielded, the shielding efficiency larger than 50dB can be achieved, so that the requirement of high-sensitivity detection equipment such as radio astronomy is met.
Owner:NAT ASTRONOMICAL OBSERVATORIES CHINESE ACAD OF SCI

Low-frequency radio astronomy observatory for cancelling electric field noise by utilizing auxiliary antenna

The invention discloses a low-frequency radio astronomy observatory for cancelling the electric field noise by utilizing an auxiliary antenna. The low-frequency radio astronomy observatory comprises areceiving antenna, an auxiliary antenna, a multi-channel pre-amplifier and an electronics unit; the receiving antenna is used for receiving a low-frequency radio astronomy electric field signal; theauxiliary antenna is shorter than the receiving antenna, and used for receiving a low-frequency noise signal; the multi-channel pre-amplifier is used for amplifying and outputting the low-frequency radio astronomy electric field signal and the low-frequency noise signal; and the electronics unit is used for amplifying and reversing the low-frequency noise signal, and then, superposing the low-frequency noise signal with the low-frequency radio astronomy electric field signal. According to the low-frequency radio astronomy observatory in the invention, an auxiliary antenna is increased; the low-frequency noise signal of a satellite platform received by utilization of the auxiliary antenna is reversed and amplified, and then, superposed with the received signal of a low-frequency receiving antenna; therefore, the low-frequency interference noise signal of the satellite platform received by the low-frequency receiving antenna can be cancelled; and the signal to noise ratio of a received signal is effectively increased.
Owner:INST OF ELECTRONICS CHINESE ACAD OF SCI
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