The EM 27/SUN uses an innovative camera based feedback system to track the movement of the sun and couple the solar beam into the spectrometer. The CamTracker software evaluates the solar image on the detector in real-time to actively control the rotation of the tracking mirror and stage, ensuring the tracker follows the sun.
Solar Broad Band Spectrometer. 阅读次数： 18780. 太阳射电宽带动态频谱仪(SBRS)：是观测太阳大气的无线电辐射的动态频谱随时间变化的特征。该设备相关指标（表一）在国际同类设备中处于领先地位。获北京市2002年科技进步一等奖（如左射电辐射和太阳大气的密度、温度、磁场等密切相关,因而射电爆发
SOLar SPECtrometer (SOLSPEC; 165–3088nm) instrument of the SOLAR monitoring observatory payload (Schmidtke et al. 2006) on board the International Space Station (ISS) started in 2008. One of the objectives of these space-based missions is the quasi-continuous measurement of the solar spectral irradi-ance variation with the highest possible accuracy.
Questar Corporation of New Hope, Pennsylvania, is pleased to announce the world''s first, Maximum-Resolution Solar Spectrometer TM capable of fitting comfortably in the palm of a hand. Questar''s Maximum-Resolution Solar Spectrometer attaches easily to any telescope that, according to its manufacturer, is compatible with solar observation and that has a 1.25" drawtube.
太阳摄谱仪(solar spectrometer )为拍摄 太阳光谱 的光学仪器 [1-2] 。 一般采用平面衍射光栅作为色散元件。准直镜和成像镜焦距在
太阳摄谱仪(solar spectrometer )为拍摄太阳光谱的光学仪器。一般采用平面衍射光栅作为色散元件。准直镜和成像镜焦距在10米左右,光栅线色散一般为5～13毫米/埃,也有小到1毫米/埃的。由于太阳辐射非常强,入射狭缝可以开得很窄,光谱分辨率接近光栅分辨本领
SBRS（Solar Broad Band Spectrometer）数据格式. 中国太阳射电观测仪器有五个频谱仪和一个单频接收机,观测数据均以二进制形式存储。在IDL语言下有大致通用的读取格式,idl读取模块如下。 openr, lun, filename, /Get_lun ;打开文件到某设备号
• Measure Solar spectral irradiance in W/m^2, moles per second, PAR, PPFD, YPF with spectral resolution as good as 1nm. • Solar radiation meters include a miniature spectrometer, a fiber optic cable (or direct attachment), a light collecting accessory/integrating sphere, and a NIST traceable intensity calibration
Our sun tracker for accurate, affordable direct or plane-of-array irradiance measurement. The SolarSIM sensors represent the state-of-the-art in solar resource measurement for PV applications. They are the only Class A sensors capable of resolving both broadband irradiance and the spectral uncertainty inherent in all PV technologies.
The objective of the Miniature X-ray Solar Spectrometer (MinXSS) CubeSats is to explore the highly variable solar soft X-ray (SXR) spectral distribution and reveal its impact on Earth''s ionosphere and thermosphere. The MinXSS X-ray instruments consist of a spectrometer, called X123, with a nominal 0.15 keV full-width at half-maximum (FWHM) resolution at 5.9 keV
• Measure Solar spectral irradiance in W/m^2, moles per second, PAR, PPFD, YPF with spectral resolution as good as 1nm. • Solar
MinXSS (Miniature X-ray Solar Spectrometer) Nanosatellite. Spacecraft Launch Mission Status Sensor Complement MinXSS-2 References. MinXSS is a 3U CubeSat solar physics mission of the CU (University of
StellarNet spectrometers are portable & compact fiber optic instruments for UV, VIS, and NIR measurements in the 190-2300nm range. The StellarNet series of miniature spectrometers is a step up in low cost instrument design, offering
The S P ectral I maging of the C oronal E nvironment or S P I C E instrument is an imaging spectrometer on board the Solar Orbiter mission. It is a European-led instrument with different partners across Europe and the USA participating in the SPICE consortium.
Solar spectral irradiance (SSI) is identified by the Global Climate Observing System (GCOS) as an essential climate variable. High precision/accuracy measurements, with extensive and well documented data characterization are required for climate and for solar and atmospheric sciences.
The first, and only, sensor capable of resolving full-range solar spectra and broadband irradiance, the SolarSIM-G employs Spectrafy''s patented SolarSIM multi-spectral measurement technology to bring routine solar spectral measurement to any application where the highest quality of irradiance data is desired.
The main applications are observation of solar radio bursts for astronomical science, education, outreach and citizen science as well as rfi-monitoring. The instrument natively operates between 45 and 870 MHz using a modern,
Our sensors combine multi-spectral measurement with proprietary radiative transfer algorithms to accurately resolve the full-range solar spectrum. This powerful approach enables our sensors to unlock the wealth of information embedded within spectral data and creates measurement capabilities that are unmatched in terms of functionality and accuracy.
A precision solar spectroradiometer (PSR) has been designed for high precision and accurate measurements of direct normal spectral solar irradiance in the wavelength range 300–1000 nm. Each PSR is radiometrically characterised and calibrated in the optical laboratory of PMOD/WRC.
We demonstrate solar spectrum measurement in the visible-near-infrared region by integrated waveguide spectral lens (WSL). Light through the chip is dispersed and focused on a camera placed at the designed distance without any free-space lens.
The main applications are observation of solar radio bursts for astronomical science, education, outreach and citizen science as well as rfi-monitoring. The instrument natively operates between 45 and 870 MHz using a modern, commercially available broadband cable-TV tuner CD1316 having a frequency resolution of 62.5 KHz. The data obtained from
The SolarRad is an all in one, robust solar irradiance measurement system featuring everything needed to perform solar spectral measurements over the 300-1100nm wavelength range (200-1700nm optional). At the heart of the system is the StellarNet BLACK-Comet concave grating spectrometer featuring a UV enhanced CCD detector.
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