{"id":1148,"date":"2021-07-27T15:58:10","date_gmt":"2021-07-27T07:58:10","guid":{"rendered":"https:\/\/kelly.anjun.com.tw\/?page_id=1148"},"modified":"2021-11-08T11:42:05","modified_gmt":"2021-11-08T03:42:05","slug":"high-sensitivity-compact-spectrometer","status":"publish","type":"page","link":"https:\/\/www.anjun.com.tw\/en\/%e9%9b%b7%e5%b0%84\/%e9%9b%b7%e5%b0%84%e9%80%b1%e9%82%8a%e8%a8%ad%e5%82%99%e9%8a%b7%e5%94%ae\/solar-ls%e9%9b%b7%e5%b0%84\/spectral-instruments\/compact-spectrometers\/high-sensitivity-compact-spectrometer\/","title":{"rendered":"HIGH-SENSITIVITY COMPACT SPECTROMETER"},"content":{"rendered":"<div data-elementor-type=\"wp-page\" data-elementor-id=\"1148\" class=\"elementor elementor-1148\">\n\t\t\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-8f2fd56 elementor-section-boxed elementor-section-height-default elementor-section-height-default\" data-id=\"8f2fd56\" data-element_type=\"section\" data-e-type=\"section\">\n\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-default\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-ce3848d\" data-id=\"ce3848d\" data-element_type=\"column\" data-e-type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-84dcbb8 elementor-widget elementor-widget-heading\" data-id=\"84dcbb8\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"heading.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t<h2 class=\"elementor-heading-title elementor-size-default\">Model SC125<\/h2>\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-04e07c6 elementor-section-boxed elementor-section-height-default elementor-section-height-default\" data-id=\"04e07c6\" data-element_type=\"section\" data-e-type=\"section\">\n\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-default\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-6a76b38\" data-id=\"6a76b38\" data-element_type=\"column\" data-e-type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-86d737d elementor-tabs-view-horizontal elementor-widget elementor-widget-tabs\" data-id=\"86d737d\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"tabs.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t<div class=\"elementor-tabs\">\n\t\t\t<div class=\"elementor-tabs-wrapper\" role=\"tablist\" >\n\t\t\t\t\t\t\t\t\t<div id=\"elementor-tab-title-1411\" class=\"elementor-tab-title elementor-tab-desktop-title\" aria-selected=\"true\" data-tab=\"1\" role=\"tab\" tabindex=\"0\" aria-controls=\"elementor-tab-content-1411\" aria-expanded=\"false\">DESCRIPTION<\/div>\n\t\t\t\t\t\t\t\t\t<div id=\"elementor-tab-title-1412\" class=\"elementor-tab-title elementor-tab-desktop-title\" aria-selected=\"false\" data-tab=\"2\" role=\"tab\" tabindex=\"-1\" aria-controls=\"elementor-tab-content-1412\" aria-expanded=\"false\">SPECIFICATIONS<\/div>\n\t\t\t\t\t\t\t\t\t<div id=\"elementor-tab-title-1413\" class=\"elementor-tab-title elementor-tab-desktop-title\" aria-selected=\"false\" data-tab=\"3\" role=\"tab\" tabindex=\"-1\" aria-controls=\"elementor-tab-content-1413\" aria-expanded=\"false\">OPTIONS & ACCESSORIES<\/div>\n\t\t\t\t\t\t\t<\/div>\n\t\t\t<div class=\"elementor-tabs-content-wrapper\" role=\"tablist\" aria-orientation=\"vertical\">\n\t\t\t\t\t\t\t\t\t<div class=\"elementor-tab-title elementor-tab-mobile-title\" aria-selected=\"true\" data-tab=\"1\" role=\"tab\" tabindex=\"0\" aria-controls=\"elementor-tab-content-1411\" aria-expanded=\"false\">DESCRIPTION<\/div>\n\t\t\t\t\t<div id=\"elementor-tab-content-1411\" class=\"elementor-tab-content elementor-clearfix\" data-tab=\"1\" role=\"tabpanel\" aria-labelledby=\"elementor-tab-title-1411\" tabindex=\"0\" hidden=\"false\"><div class=\"container feauteres\"><div class=\"row\"><div class=\"col-12\"><h4 class=\"title text-left\"><span style=\"color: #000000;\">FEATURES<\/span><\/h4><p><span style=\"color: #000000;\">The compact high-sensitivity spectrometer SC125 is developed for low light applications such as measurements of Raman scattering, fluorescence, etc., which require especially high sensitivity or enhanced specifications in the UV spectral range.<\/span><\/p><\/div><\/div><\/div><div class=\"wrapper product-advantages-wr\"><div class=\"container\"><div class=\"row\"><div class=\"col-6 left\"><ul><li><p><span style=\"color: #000000;\">UP-TO-DATE MODEL BASED ON BACK-THINNED ARRAYS FOR OPERATION WITH LOW SIGNALS<\/span><\/p><\/li><li><p><span style=\"color: #000000;\">ENHANCED UV SENSITIVITY<\/span><\/p><\/li><li><p><span style=\"color: #000000;\">MONOLITHIC HOUSING FOR OPTIMUM STABILITY<\/span><\/p><\/li><li><p><span style=\"color: #000000;\">INTERNAL LIGHT TRAPS TO REDUCE STRAY LIGHT<\/span><\/p><\/li><li><p><span style=\"color: #000000;\">FLEXIBLE CONFIGURATION, INCLUDING A CHOICE OF DIFFRACTION GRATINGS, SPECTRAL RANGES AND RESOLUTIONS TAILORED TO YOUR REQUIREMENT<\/span><\/p><\/li><li><p><span style=\"color: #000000;\">USER-FRIENDLY INTERFACE COMPATIBLE WITH WINDOWS XP, WINDOWS 7, 32\/64 BITS<\/span><\/p><\/li><\/ul><h2><span style=\"color: #000000;\">DESCRIPTION<\/span><\/h2><h5 id=\"gallery-3\" class=\"gallery galleryid-320 gallery-columns-3 gallery-size-gallery_product_img\"><span style=\"color: #000000;\"><img decoding=\"async\" src=\"https:\/\/www.anjun.com.tw\/wp-content\/uploads\/2019\/01\/SC125A-300x200.jpg\" \/><img decoding=\"async\" src=\"https:\/\/www.anjun.com.tw\/wp-content\/uploads\/2019\/01\/SC125-300x200.jpg\" \/>\u00a0<\/span><\/h5><div><p><span style=\"color: #000000;\">The high-aperture optical bench of the SC125 has no moving parts and minimises the number of reflective surfaces. The SC125 features a monolithic housing, thus ensuring long-time measurement stability. The case has internal fins \u2013 light traps which allow reducing stray light which is a typical problem of compact short-focal length instruments.<\/span><\/p><p><span style=\"color: #000000;\">The SC125 may contain as a detector either one of two non-cooled Hamamatsu back-thinned CCD-arrays without a charge-storage section (back-thinned FFT CCD), operating in the binning mode. Both arrays have wide spectral range and excellent sensitivity in the UV (see below for the curves of each detector spectral sensitivity and their specifications). These two arrays differ in quantum efficiency, data reading rate, dynamic range, and in pixel active area size.<\/span><\/p><p><span style=\"color: #000000;\">.<\/span><\/p><p>\u00a0<\/p><p><span style=\"color: #000000;\">The detector based on the S7030-1006 CCD-array is more sensitive, has lower noise, better values of dynamic range and uniformity. The detector based on the S10420-1106 CCD array is faster, has anti-blooming and, since it has a greater number of pixels and smaller pixel size, ensures better spectral resolution than the S7030-1006. The IMAGING Version (Optional) features an astigmatism compensator \u2013 cylindrical lens \u2013 installed after the entrance slit. This further enhances of system sensitivity.<\/span><\/p><p>\u00a0<\/p><p><span style=\"color: #000000;\"><em>Spectral curve of sensitivity of the back-thinned CCD detector model S10420-1106<\/em><\/span><\/p><p>\u00a0<\/p><p><span style=\"color: #000000;\"><em>Spectral curve of sensitivity of the back-thinned FFT-CCD detector model S7030-1006 in comparison with front-illuminated CCD with and without UV-coating<\/em><\/span><\/p><\/div><\/div><\/div><\/div><\/div><\/div>\n\t\t\t\t\t\t\t\t\t<div class=\"elementor-tab-title elementor-tab-mobile-title\" aria-selected=\"false\" data-tab=\"2\" role=\"tab\" tabindex=\"-1\" aria-controls=\"elementor-tab-content-1412\" aria-expanded=\"false\">SPECIFICATIONS<\/div>\n\t\t\t\t\t<div id=\"elementor-tab-content-1412\" class=\"elementor-tab-content elementor-clearfix\" data-tab=\"2\" role=\"tabpanel\" aria-labelledby=\"elementor-tab-title-1412\" tabindex=\"0\" hidden=\"hidden\"><h4><span style=\"color: #000000;\">SPECIFICATIONS<\/span><\/h4><table border=\"1\"><thead><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">SPECTROMETER MODEL<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">SC125- S10420<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">SC125- S7030<\/span><\/td><\/tr><\/thead><tbody><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Spectral range, nm<\/span><\/td><td style=\"text-align: center;\" colspan=\"2\"><span style=\"color: #000000;\">200-1100<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Focal length, mm<\/span><\/td><td style=\"text-align: center;\" colspan=\"2\"><span style=\"color: #000000;\">125<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">F\/number<\/span><\/td><td style=\"text-align: center;\" colspan=\"2\"><span style=\"color: #000000;\">1 : 3.9<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Entrance slit (one to choose)<\/span><\/td><td style=\"text-align: center;\" colspan=\"2\"><span style=\"color: #000000;\">fixed width: 14\u00b5m, 30\u00b5m and 50\u00b5m<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Spectral resolution<\/span><\/td><td style=\"text-align: center;\" colspan=\"2\"><span style=\"color: #000000;\">depends on selected diffraction grating (see table below)<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">CCD-detector model<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">S10420-1106<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">S7030-1006<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Number of pixels<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">2068 x 70<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">1024 x 64<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Number of active pixels<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">2048 x 64<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">1024 x 58<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Pixel size, \u00b5m<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">14 x 14<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">24 x 24<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Active area size, mm<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">28.672 x 0.896<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">24.6 x 1.4<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Maximum spectral sensitivity, nm<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">500<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">650<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Maximum quantum efficiency<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">&gt;75 %<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">&gt;90 %<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Non-uniformity of sensitivity<sup>1)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">\u00b110 %<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">\u00b13 %<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Anti-blooming<sup>2)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">yes<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">No<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">ADC<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">16bit, 250 kHz<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">16bit, 125 kHz<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Mean-square reading noise, ADC counts<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">&lt; 12<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">&lt; 7<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Dynamic range<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">~ 8000 : 1<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">~15 000 : 1<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Exposure time<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">8.3ms \u2014 3s<sup>3)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">8.2ms \u2014 2s<sup>3)<\/sup><\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Frame processing time in the binning mode, ms<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">9.39<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">9.12<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Thermoelectric cooling<\/span><\/td><td style=\"text-align: center;\" colspan=\"2\"><span style=\"color: #000000;\">no<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Operating temperature<\/span><\/td><td style=\"text-align: center;\" colspan=\"2\"><span style=\"color: #000000;\">10- 30\u00b0C<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Computer interface<\/span><\/td><td style=\"text-align: center;\" colspan=\"2\"><span style=\"color: #000000;\">Full Speed USB<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Synchronisation<\/span><\/td><td style=\"text-align: center;\" colspan=\"2\"><span style=\"color: #000000;\">IN\/OUT<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Optical input<\/span><\/td><td style=\"text-align: center;\" colspan=\"2\"><span style=\"color: #000000;\">Optical quartz fiber core dia 0.6mm (option 0.4mm), length 1m, SMA-905 connector<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Dimensions, mm<\/span><\/td><td style=\"text-align: center;\" colspan=\"2\"><span style=\"color: #000000;\">158 \u00d7 182 \u00d7 74<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">Weight, kg<\/span><\/td><td style=\"text-align: center;\" colspan=\"2\"><span style=\"color: #000000;\">2.2<\/span><\/td><\/tr><\/tbody><\/table><p><span style=\"color: #000000;\"><sup>1)<\/sup>\u00a0Signal level \u2013 50% of saturation.<\/span><\/p><p><span style=\"color: #000000;\"><sup>2)<\/sup>\u00a0Anti-blooming \u2013 sensor\u2019s feature eliminating overflow of charges from over-exposed pixels to the neighboring ones.<\/span><\/p><p><span style=\"color: #000000;\"><sup>3)<\/sup>Maximum storage time is deemed to be the time at which dark signal reaches 10% of the dynamic range at the ambient temperature +25\u00b0C.<\/span><\/p><h4>\u00a0<\/h4><h2><span style=\"color: #000000;\">RECOMMENDATIONS FOR CHOOSING A DIFFRACTION GRATING<\/span><\/h2><p><span style=\"color: #000000;\">At the time of placing your order you should choose a grating lines density (i.e. spectral resolution of your instrument), as well as the spectral range for operation. For your convenience the table below lists the average values of grating dispersion, spectral resolution and multichannel array bandpass.<\/span><\/p><table border=\"1\"><thead><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">DIFFRACTION GRATINGS, LINES\/MM<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">1800<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">1200<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">900<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">600<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">400<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">300<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">200<\/span><\/td><\/tr><\/thead><tbody><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">\u2014 possible spectral range of grating operation, nm<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">180-600<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">180-900<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">180-1100<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">180-1100<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">190-1100<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">200-1100<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">200-1100<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">\u2014 multichannel array bandpass (average), nm<sup>1)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">105<sup>2)<\/sup>92<sup>3)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">170<sup>2)<\/sup>145<sup>3)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">230<sup>2)<\/sup>200<sup>3)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">350<sup>2)<\/sup>300<sup>3)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">540<sup>2)<\/sup>460<sup>3)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">720<sup>2)<\/sup>620<sup>3)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">1000<sup>2)<\/sup>920<sup>3)<\/sup><\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">\u2014 reciprocal linear dispersion (average), nm\/mm<sup>1)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">3.8<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">6.0<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">8.2<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">12.5<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">19.0<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">25.4<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">38.0<\/span><\/td><\/tr><tr><td style=\"text-align: center;\"><span style=\"color: #000000;\">\u2014 spectral resolution (average), nm<\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">0.16<sup>2)<\/sup>0.22<sup>3)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">0.25<sup>2)<\/sup>0.36<sup>3)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">0.34<sup>2)<\/sup>0.5<sup>3)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">0.5<sup>2)<\/sup>0.75<sup>3)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">0.8<sup>2)<\/sup>1.1<sup>3)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">1.0<sup>2)<\/sup>1.5<sup>3)<\/sup><\/span><\/td><td style=\"text-align: center;\"><span style=\"color: #000000;\">1.6<sup>2)<\/sup>2.3<sup>3)<\/sup><\/span><\/td><\/tr><\/tbody><\/table><p><span style=\"color: #000000;\"><sup>1)<\/sup>\u00a0for 300nm wavelength.<\/span><\/p><p><span style=\"color: #000000;\"><sup>2)<\/sup>\u00a0for the SC125- S10420 model.<\/span><\/p><p><span style=\"color: #000000;\"><sup>3)<\/sup>\u00a0for the SC125- S7030 model.<\/span><\/p><p><span style=\"color: #000000;\"><strong>EXAMPLE:<\/strong>\u00a0If you are interested in the1200 lines\/mm grating and the S10420-1106 detector (spectral resolution of 0.25nm), then you should choose the location of 170nm multichannel array bandpass within the possible 180-900nm spectral range of the grating. For instance, the SC125- S10420 spectrometer operating in the range of 250-420nm with 0.25nm resolution.<\/span><\/p><p><span style=\"color: #000000;\">The values indicated in the table are calculated for 300nm wavelength. With increased wavelength, dispersion of a specific grating and multichannel array bandpass are slightly decreased and resolution is improved. Contact a SOLAR LS specialist for more precise calculation of parameters for your instrument.<\/span><\/p><p><span style=\"color: #000000;\"><img decoding=\"async\" class=\"aligncenter\" src=\"https:\/\/www.anjun.com.tw\/wp-content\/uploads\/2019\/01\/qwe2_1.jpg\" \/><\/span><\/p><p style=\"text-align: center;\"><span style=\"color: #000000;\">Spectral curve of sensitivity of the back-thinned CCD detector model S10420-1106<\/span><\/p><p style=\"text-align: center;\"><span style=\"color: #000000;\"><img decoding=\"async\" src=\"https:\/\/www.anjun.com.tw\/wp-content\/uploads\/2019\/01\/qwe2-1.jpg\" \/><\/span><\/p><dl class=\"gallery-item\"><dd id=\"gallery-5-1431\" class=\"wp-caption-text gallery-caption\"><p><span style=\"color: #000000;\">Spectral curve of sensitivity of the back-thinned FFT-CCD detector model S7030-1006 in comparison with front-illuminated CCD with and without UV-coating<\/span><\/p><\/dd><\/dl><p><style type=\"text\/css\">\n<!-- table{ border-collapse:separate; collapse;border:1px solid black; } td{ collapse;border:1px solid black; } --><br \/><\/style><\/p><\/div>\n\t\t\t\t\t\t\t\t\t<div class=\"elementor-tab-title elementor-tab-mobile-title\" aria-selected=\"false\" data-tab=\"3\" role=\"tab\" tabindex=\"-1\" aria-controls=\"elementor-tab-content-1413\" aria-expanded=\"false\">OPTIONS & ACCESSORIES<\/div>\n\t\t\t\t\t<div id=\"elementor-tab-content-1413\" class=\"elementor-tab-content elementor-clearfix\" data-tab=\"3\" role=\"tabpanel\" aria-labelledby=\"elementor-tab-title-1413\" tabindex=\"0\" hidden=\"hidden\"><h4 class=\"title-tab title text-left\"><span style=\"color: #000000;\">OPTIONS &amp; ACCESSORIES<\/span><\/h4><p><span style=\"color: #000000;\">At your request the SC125 spectrometer can be equipped with optional calibration of spectral sensitivity.<\/span><\/p><h2><span style=\"color: #000000;\">SENSITIVITY CALIBRATION<\/span><\/h2><p><span style=\"color: #000000;\">Spectral ranges of calibration:<\/span><\/p><ul><li><span style=\"color: #000000;\">Cal-UV: within 220-400nm.<\/span><\/li><li><span style=\"color: #000000;\">Cal-VIS: within 300-1050nm.<\/span><\/li><li><span style=\"color: #000000;\">Calibration is performed with certified light sources (a deuterium lamp for the 220-400nm spectral range and a halogen lamp for the 300-1050nm range). It is made using a fiber input and is valid for 1 year provided that the optical fiber is not removed from the spectrometer. Calibration accuracy is +\/-10%.<\/span><\/li><\/ul><h3><span style=\"color: #000000;\">WHAT POSSIBILITIES ARE OFFERED BY SPECTRAL SENSITIVITY CALIBRATION<\/span><\/h3><p><span style=\"color: #000000;\">Whereas in the past the spectrum of your light source was superimposed by spectral curves of diffraction grating efficiency, detector sensitivity, reflective index of mirrors, now you have the opportunity to restore true spectra of the analysed source. You will be able to:<\/span><\/p><ul><li><span style=\"color: #000000;\">record true spectra<\/span><\/li><li><span style=\"color: #000000;\">mathematically decompose complex lines of the spectrum into its components*<\/span><\/li><li><span style=\"color: #000000;\">determine the tristimulus values and colour-rendering index of light sources*<\/span><\/li><li><span style=\"color: #000000;\">determine the light power density in the UV ranges A, B, and C*.<\/span><\/li><\/ul><p><span style=\"color: #000000;\"><em>* Features marked with an asterisk are not included into the software of your spectrometer; they are implemented by exporting to external programs.<\/em><\/span><\/p><h4><span style=\"color: #000000;\">HOW CALIBRATION OF SPECTRAL SENSITIVITY RUNS<\/span><\/h4><p><span style=\"color: #000000;\">Spectra recorded by the SC125 spectrometers with TCD1304 Toshiba CCD detectors (14 bit) and S10420-1106 Hamamatsu CCD detectors (16 bit), and the reference spectrum of the deuterium lamp emission in the spectral range of 220-400nm are presented in Figure 1. The figure shows that, other things being equal, the S10420-1106 detector provides higher intensity than TCD1304 and the absence of intensity modulations, which can introduce additional distortions into sensitivity calibration. Besides, the S10420-1106 detector features a wider dynamic range (due to its low noise and through the use of 16 bit digitisation instead of 14 bit).<\/span><\/p><p>\u00a0<\/p><p><span style=\"color: #000000;\"><em>Fig. 1. True spectrum of the calibration lamp (black) and its spectra as recorded by the SC125 spectrometer with TCD1304 (blue) and S10420-1106 (red) detectors<\/em><\/span><\/p><p>\u00a0<\/p><p><span style=\"color: #000000;\"><em>Fig. 2. Calibration factor spectrum of the SC125-S10420 spectrometer<\/em><\/span><\/p><p><span style=\"color: #000000;\">Figure 2 shows the spectral dependence of sensitivity calibration factor of the SC125-S10420 spectrometer in the range of 220-400nm. Increase of the calibration factor with decreasing wavelength is resulting from decrease of the detector sensitivity and reflective index of mirrors, along with the increase of photon energy. Multiplying the measured spectrum of your source by the spectrum of calibration factor (this is done automatically by the software) you will get the true undistorted spectrum.<\/span><\/p><p><span style=\"color: #000000;\">Dependence of the signal acquired with the SC125-S10420 on intensity of the signal from the calibrated source (Figure 3) proves excellent linearity of the S10420 detector (as opposed to the TCD1304, which shows considerable nonlinearities at the edges of its dynamic range, i.e. at high and low signal levels). Good detector linearity provides a possibility to calibrate the spectrometer sensitivity for one exposure time, and then to use this calibration for other exposure intervals.<\/span><\/p><p>\u00a0<\/p><p><span style=\"color: #000000;\"><em>Fig. 3. Calibration factor of the SC125-S10420 spectral sensitivity vs exposure time<\/em><\/span><\/p><p><span style=\"color: #000000;\">A detector based on the S7030-1006 Hamamatsu array has advantages similar to the S10420-1106 detector. Due to the above mentioned properties we recommend both of these detectors for use in spectral instruments with the sensitivity calibration option.<\/span><\/p><p><span style=\"color: #000000;\">Prospects<\/span><\/p><p><span style=\"color: #000000;\">Starting from mid-2014 we intend to perform sensitivity calibration of spectral instruments in the UV and visible spectral range with issuing certificates of calibration which will be recognised in the territory of CIS and Europe. Calibration will be made on the basis of an accredited calibration laboratory of the Institute of Physics of the Belarusian National Academy of Science with reference to national standards of Belarus, Russia and Germany. Calibration accuracy will depend on a chosen spectral range.<\/span><\/p><p><span style=\"color: #000000;\">The emission will be input into a certified spectrometer via an optical integrating sphere (the scheme is shown in Figure 4), being the most proper approach in terms of minimising measurement errors. It should be noted however that sensitivity of the spectral instrument is greatly reduced (102-104 times).<\/span><\/p><p>\u00a0<\/p><p><span style=\"color: #000000;\"><em>Fig. 4. Scheme of the certified spectrometer with spectral sensitivity calibration<\/em><\/span><\/p><\/div>\n\t\t\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-e33828b elementor-section-boxed elementor-section-height-default elementor-section-height-default\" data-id=\"e33828b\" data-element_type=\"section\" data-e-type=\"section\">\n\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-default\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-31558db\" data-id=\"31558db\" data-element_type=\"column\" data-e-type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-8934b2b elementor-widget elementor-widget-spacer\" data-id=\"8934b2b\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"spacer.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t<div class=\"elementor-spacer\">\n\t\t\t<div class=\"elementor-spacer-inner\"><\/div>\n\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-66fead6 elementor-section-boxed elementor-section-height-default elementor-section-height-default\" data-id=\"66fead6\" data-element_type=\"section\" data-e-type=\"section\">\n\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-default\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-dad7805\" data-id=\"dad7805\" data-element_type=\"column\" data-e-type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-79594f8 elementor-widget elementor-widget-text-editor\" data-id=\"79594f8\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"text-editor.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t\t\t<p style=\"text-align: center;\">SOLARLS\u7684\u6240\u6709\u8cc7\u8a0a\u4f86\u81eaSOLARLS\u7db2\u9801\uff0c\u6240\u6709\u7248\u6b0a\u6b78SOLARLS\uff0c\u7e41\u9ad4\u5b57\u7248\u6b0a\u5c6c\u5b89\u5747\u79d1\u6280\u3002<\/p>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<\/div>","protected":false},"excerpt":{"rendered":"<p>Model SC125 DESCRIPTION SPECIFICATIONS OPTIONS &amp; AC&hellip;&nbsp;<a href=\"https:\/\/www.anjun.com.tw\/en\/%e9%9b%b7%e5%b0%84\/%e9%9b%b7%e5%b0%84%e9%80%b1%e9%82%8a%e8%a8%ad%e5%82%99%e9%8a%b7%e5%94%ae\/solar-ls%e9%9b%b7%e5%b0%84\/spectral-instruments\/compact-spectrometers\/high-sensitivity-compact-spectrometer\/\" class=\"\" rel=\"bookmark\">Read More &raquo;<span class=\"screen-reader-text\">HIGH-SENSITIVITY COMPACT SPECTROMETER<\/span><\/a><\/p>","protected":false},"author":2,"featured_media":0,"parent":1117,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"neve_meta_sidebar":"","neve_meta_container":"","neve_meta_enable_content_width":"off","neve_meta_content_width":70,"neve_meta_title_alignment":"","neve_meta_author_avatar":"","neve_post_elements_order":"","neve_meta_disable_header":"","neve_meta_disable_footer":"","neve_meta_disable_title":"","footnotes":""},"class_list":["post-1148","page","type-page","status-publish","hentry"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.0 - 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