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33 results about "Sunspot" patented technology

Sunspots are temporary phenomena on the Sun's photosphere that appear as spots darker than the surrounding areas. They are regions of reduced surface temperature caused by concentrations of magnetic field flux that inhibit convection. Sunspots usually appear in pairs of opposite magnetic polarity. Their number varies according to the approximately 11-year solar cycle.

Solar multi-conjugate adaptive optical system

ActiveCN102621687ARealize high-resolution imagingSimplify the difficulty of decouplingOptical measurementsOptical elementsHigh resolution imagingCoupling
The invention provides a solar multi-conjugate adaptive optical system. The solar multi-conjugate adaptive optical system comprises a lower atmospheric wave front sensor, a middle and upper atmospheric wave front sensor, a lower atmospheric wave front corrector, a middle and upper atmospheric wave front corrector, a wave front controller, an optical relay system, an imaging subsystem and other necessary optical components. The system has the advantages that sunspots or grain structures on the surface of the sun are taken as beacons and wave front detection is conducted on multiple areas at the same time, so as to obtain wave front distortion caused by turbulence in a large field range; wave front aberration caused by different turbulent layers is calculated by utilizing a tomography algorithm; and at last, the wave front correctors positioned in conjugate positions of the corresponding turbulent layers are controlled to correct the atmospheric turbulence in a layered manner, so as to finally realize high-resolution imaging in the large field range. The solar multi-conjugate adaptive optical system has the advantages that the sequence of the conjugate positions of the high and the lower turbulent layers is adjusted through the optical relay system, so that the lower turbulent layer is firstly compensated and corrected and the accuracy of the detection and the correction is increased; and due to the use of the tomography algorithm, errors caused by the coupling of the wave front aberrations of the different turbulent layers are reduced.
Owner:INST OF OPTICS & ELECTRONICS - CHINESE ACAD OF SCI

Spaceborne target detection tracing camera in sun viewing blind zone

InactiveCN101173984AFill in the observation blind spotWith detectionElectromagnetic wave reradiationBlind zoneData treatment
The invention discloses a probing and tracking camera for targets on solar observation blind areas, which can be arranged on a satellite to observe and track targets on the solar observation blind areas. The camera comprises an attenuation filter, an optical system, a probe and a data processing circuit; wherein, a ray of light from an object space passes through the attenuation filter and the optical system and forms an image on the probe. The attenuation filter is used to adjust the intensity of light coming into the camera, and the optical system adopts a double-Gauss near infrared teleobjective system; the probe adopts a CMOS probe, and the dynamic range is designed as follows: the brightness of the sun, sunspot images is designed out of the dynamic range of the camera, and the brightness of the observed targets is designed within the saturation value of the camera. The data processing circuit conducts reverse-phase processing over the images output by the probe, so as to enable the system to acquire higher positioning precision of the targets. The probing and tracking camera in the invention, together with a sun sensor, a two-dimensional tracker and an image processing system, forms a whole probing and tracking system for targets.
Owner:SHANGHAI INST OF TECHNICAL PHYSICS - CHINESE ACAD OF SCI

Method for automatically recognizing macula based on Huairou full-disk single-color image

InactiveCN104615990AExtraction sensitiveInstrument Noise CancellationScene recognitionColor imageSolar physics
The invention relates to a method for automatically recognizing macula based on a Huairou full-disk single-color image, and aims at solving the problems of extremely low efficiency caused by manually recognizing the profile of macula on disk and that mass data cannot be met in the solar physics in the domestic astronomy field. The method comprises the steps of extracting gradient information of the disk by the morphology bot-hat transformation according to the full-disk single-color image of the Huairou solar observing station of National Astronomical Observatories of China; removing the influence of inherent limb darkening rule of the disk by the fragmentation threshold method, so as to automatically recognize macula. Compared with other algorithms for recognizing the macula based on high-quality solar space data, the method has the characteristic that the macula of the ground images with relatively low quality and suffering from the interference of instrument noise can be precisely recognized. The method is applicable to automatic recognition of macula in the single-color images or white light images at other wave bands and can provide directly service to the fields of generator theory, solar action predication and space environment monitoring.
Owner:NAT ASTRONOMICAL OBSERVATORIES CHINESE ACAD OF SCI

Method for identifying solar granule in astronomic image

The invention relates to a method for identifying a solar granule in an astronomic image, and belongs to the fields of astronomy technology and image processing. The method comprises the steps of: firstly, receiving a solar photospheric image I1, using band-pass filtering to carry out de-noising, and obtaining a de-noised image I2; then according to intensity distribution of the image I2, judging whether sunspots exist in the image; carrying out top-hat transformation and bottom-hat transformation respectively on the image I2, and obtaining a top-hat transformation image and a bottom-hat transformation image; then adding the top-hat transformation image to the solar photospheric image, obtaining an image I3, and carrying out subtraction between the image I3 and the bottom-hat transformation image to obtain an image I4; respectively subjecting the image I4 respectively to open operation of a phase congruency method, binaryzation and morphology and hole filling operation, and obtaining an image I7; and carrying out watershed transformation operation on the image I7, and obtaining a binary image of a granule cellular boundary. By adopting the method for identifying the solar granule in the astronomic image, the granule organization high in contrast and clear in edge can be well identified, and the granule characteristics low in contrast and fuzzy in edge can also be well identified.
Owner:KUNMING UNIV OF SCI & TECH

Solar multi-conjugate adaptive optical system

ActiveCN102621687BRealize high-resolution imagingSimplify the difficulty of decouplingOptical measurementsOptical elementsHigh resolution imagingCoupling
The invention provides a solar multi-conjugate adaptive optical system. The solar multi-conjugate adaptive optical system comprises a lower atmospheric wave front sensor, a middle and upper atmospheric wave front sensor, a lower atmospheric wave front corrector, a middle and upper atmospheric wave front corrector, a wave front controller, an optical relay system, an imaging subsystem and other necessary optical components. The system has the advantages that sunspots or grain structures on the surface of the sun are taken as beacons and wave front detection is conducted on multiple areas at the same time, so as to obtain wave front distortion caused by turbulence in a large field range; wave front aberration caused by different turbulent layers is calculated by utilizing a tomography algorithm; and at last, the wave front correctors positioned in conjugate positions of the corresponding turbulent layers are controlled to correct the atmospheric turbulence in a layered manner, so as to finally realize high-resolution imaging in the large field range. The solar multi-conjugate adaptive optical system has the advantages that the sequence of the conjugate positions of the high and the lower turbulent layers is adjusted through the optical relay system, so that the lower turbulent layer is firstly compensated and corrected and the accuracy of the detection and the correction is increased; and due to the use of the tomography algorithm, errors caused by the coupling of the wave front aberrations of the different turbulent layers are reduced.
Owner:INST OF OPTICS & ELECTRONICS - CHINESE ACAD OF SCI

Method for removing sunspot regions in image, image processor and photographing device

The invention discloses a method for removing sunspot regions in an image. The method comprises the steps of acquiring a current frame image; and determining a dark region in the current frame image according to the brightness value of the pixel points in the current frame image, wherein the pixel points are determined to be in the dark region when the brightness value of the pixel points is smaller than the threshold value of the dark region, and generating a sunspot identification signal; calculating the length of each row of the dark region according to the sunspot identification signal, and taking the sum of the length of each row of the dark region and the transition threshold value as the length of the sunspot region of the row; determining the diameter of the sunspot region according to the length of the sunspot region of each row; determining the center coordinate according to the coordinate value of the sunspot region where the diameter is located; determining the sunspot region according to the diameter and the center coordinate in the next frame of the image, and removing the sunspot region in the next frame of the image. According to the method, no transition region residue exists when the sunspot region is removed, and the image effect is better. The invention further discloses an image processor and a photographing device.
Owner:BYD CO LTD

A method for identifying solar rice grains in astronomical images

The invention relates to a method for identifying a solar granule in an astronomic image, and belongs to the fields of astronomy technology and image processing. The method comprises the steps of: firstly, receiving a solar photospheric image I1, using band-pass filtering to carry out de-noising, and obtaining a de-noised image I2; then according to intensity distribution of the image I2, judging whether sunspots exist in the image; carrying out top-hat transformation and bottom-hat transformation respectively on the image I2, and obtaining a top-hat transformation image and a bottom-hat transformation image; then adding the top-hat transformation image to the solar photospheric image, obtaining an image I3, and carrying out subtraction between the image I3 and the bottom-hat transformation image to obtain an image I4; respectively subjecting the image I4 respectively to open operation of a phase congruency method, binaryzation and morphology and hole filling operation, and obtaining an image I7; and carrying out watershed transformation operation on the image I7, and obtaining a binary image of a granule cellular boundary. By adopting the method for identifying the solar granule in the astronomic image, the granule organization high in contrast and clear in edge can be well identified, and the granule characteristics low in contrast and fuzzy in edge can also be well identified.
Owner:KUNMING UNIV OF SCI & TECH
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