{"id":2402,"date":"2025-06-19T19:35:24","date_gmt":"2025-06-19T11:35:24","guid":{"rendered":"https:\/\/www.ledphotometer.com\/blog\/high-precision-ccd-spectroradiometer\/"},"modified":"2025-07-03T15:09:12","modified_gmt":"2025-07-03T07:09:12","slug":"high-precision-ccd-spectroradiometer","status":"publish","type":"post","link":"https:\/\/www.ledtestsystem.com\/ko\/%ec%a0%9c%ed%92%88\/high-precision-ccd-spectroradiometer\/","title":{"rendered":"High-accuracy\u00a0 Spectroradiometer"},"content":{"rendered":"

LMS-9000C High Precision CCD Spectroradiometer is according to LM-79 clause 9.1. It is designed for any visible optical spectrum distribution analysis, mimicking various light sources in the visible region by feedback control of the radiant power emitted by individual LEDs. This LED optical spectrum analyzer is used as a transfer standard for photometric, colorimetric a<\/a>nd radiometric applications.<\/p>\n

LMS-9000C can do quick test with high accuracy. It used in scientific lab. It works with \uc801\ubd84 \uad6c<\/a> and standard lamp as a system: LPCE-2 High Precision Spectroradiometer Integrating Sphere System<\/a>.<\/p>\n

\ud45c\uc900<\/strong>:
\nCIE 177<\/a> \"\ubc31\uc0c9 LED \uad11\uc6d0\uc758 \uceec\ub7ec \ub80c\ub354\ub9c1\"
\nCIE84<\/a> \"\uad11\uc18d \uce21\uc815\"
\nCIE-13.3<\/a> \"\uad11\uc6d0\uc758 \uceec\ub7ec \ub80c\ub354\ub9c1 \uc18d\uc131\uc744 \uce21\uc815\ud558\uace0 \uc9c0\uc815\ud558\ub294 \ubc29\ubc95\"
\nLM-79-19<\/a> \"\uc194\ub9ac\ub4dc \uc2a4\ud14c\uc774\ud2b8 \uc870\uba85 \uc81c\ud488\uc758 \uad11\ud559 \ubc0f \uc804\uae30 \uce21\uc815\"
\nIESNA LM-63-2<\/a> \"\uad11\ub3c4 \ub370\uc774\ud130 \ubc0f \uad00\ub828 \uc815\ubcf4\uc758 \uc804\uc790\uc801 \uc804\uc1a1\uc744 \uc704\ud55c IESNA \ud45c\uc900 \ud30c\uc77c \ud615\uc2dd\"
\nIES LM-80-08<\/a> \"LED \uad11\uc6d0\uc758 \ub8e8\uba58 \uc720\uc9c0 \uad00\ub9ac \uce21\uc815\"
\nANSI-C78.377<\/a> \"\uc804\uae30 \ub7a8\ud504\uc6a9 \uace0\uccb4 \uc870\uba85 \uc81c\ud488\uc758 \uc0c9\ub3c4 \uc0ac\uc591\"
\n(EU) 2019\/2015<\/a> \"\uc704\uc6d0\ud68c \uc704\uc784 \uaddc\uc815\"<\/p>\n

\uce21\uc815:
\n<\/strong>- \ube44\uc0c9: \uc0c9\ub3c4 \uc88c\ud45c, CCT, \uc0c9\ube44, \ud53c\ud06c \ud30c\uc7a5, \ubc18\ub300\uc5ed\ud3ed, \uc8fc \ud30c\uc7a5, \uc0c9 \uc21c\ub3c4, CRI, CQS, TM-30(Rf, Rg), \uc2a4\ud399\ud2b8\ub7fc \ud14c\uc2a4\ud2b8
\n- \uad11\ub3c4\uacc4: \uad11\uc18d, \uad11\ud6a8\uc728, \ubcf5\uc0ac \uc804\ub825, WPE, EQE, EEI, \uc5d0\ub108\uc9c0 \ud6a8\uc728 \ub4f1\uae09, \ub3d9\uacf5 \ud50c\ub7ed\uc2a4, \ub3d9\uacf5 \ud50c\ub7ed\uc2a4 \ud6a8\uc728, \ub3d9\uacf5 \uacc4\uc218, \uc11c\ud1a0\ud53d \ud50c\ub7ed\uc2a4, \uc2dd\ubb3c \uc131\uc7a5 \ub7a8\ud504 PAR \ubc0f PPF
\n\u2022 Electrical: Voltage, Current, Power, Power Factor, Displacement Factor, Harmonic
\n\u2022 LED optical maintenance test: Flux VS time, CCT VS time, CRI VS time, Power VS time, Power Factor VS time, Current VS time and Flux Efficiency VS time<\/p>\n

\uc0ac\uc591:<\/strong>
\n- \uc2a4\ud399\ud2b8\ub7fc \ud30c\uc7a5 \uc815\ud655\ub3c4: \u00b10.3nm, \ud30c\uc7a5 \uc7ac\ud604\uc131: \u00b10.1nm
\n- \uc0d8\ud50c \uc2a4\uce94 \ub2e8\uacc4: \u00b10.1nm
\n- \uc0c9\ub3c4 \uc88c\ud45c\uc758 \uc815\ud655\ub3c4(\u0394x, \u0394y): \u00b10.002(\ud45c\uc900 A \ub7a8\ud504 \uc0ac\uc6a9 \uc2dc)
\n- \uc0c1\uad00 \uc0c9\uc628\ub3c4 CCT: 1,500K~100,000K, CCT \uc815\ud655\ub3c4: \u00b10.3%
\n- \uceec\ub7ec \ub80c\ub354\ub9c1 \uc9c0\uc218 \ubc94\uc704: 0~100.0, \uc815\ud655\ub3c4: \u00b1(0.3%rd\u00b10.3)
\n- \uad11\uc18d \ubc94\uc704: 0.01-200,000lm; \uad11\ub3c4 \uc120\ud615 \uc815\ud655\ub3c4: \u00b10.5%
\n- \ubbf8\uad11: <0.015%(600nm) \ubc0f <0.03%(435nm)
\n- \ud1b5\ud569 \uc2dc\uac04: 0.1~10,000ms
\n- \uc801\ubd84 \uad6c\uc758 \ub0b4\ubd80 \ubc0f \uc678\ubd80 \uc628\ub3c4\ub97c \uce21\uc815\ud560 \uc218 \uc788\uc2b5\ub2c8\ub2e4.
\n\u2022 Total flux testing method: spectrum, photometric and spectrum with photometric revision<\/p>\n\n\n\n\n
LISUN \ubaa8\ub378<\/strong><\/td>\nLMS-9000C<\/strong><\/td>\nLMS-9000CUV-VIS<\/strong><\/td>\nLMS-9000CVIS-NIR<\/strong><\/td>\nLMS-9000CUV<\/strong><\/td>\n<\/tr>\n
\ud30c\uc7a5<\/strong><\/td>\n350-800nm<\/td>\n200-800nm<\/td>\n350-1050nm<\/td>\n200-400nm<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

The LMS-9000C (which is updated on LMS-9000B) uses the band pass-filter wheel correcting technique, spectrometer & broadband-radiometer & photometer combined technique, and modified NIST stray light correction technology. The LMS-9000C spectroradiometer can realize ultra low stray light and super photometry linearity in overall dynamic range.<\/p>\n

\"\uace0\uc815\ubc00<\/p>\n

LISUN LPCE-2 (LMS-9000C) \uace0\uc815\ubc00 \ubd84\uad11 \ubc29 \uc0ac\uacc4 \ud1b5\ud569 \uad6c \uc2dc\uc2a4\ud15c-\ud310\ub9e4 \ud6c4 \uc790\uc8fc \ubb3b\ub294 \uc9c8\ubb38 (FAQ).<\/span><\/a>
\n<\/strong>LISUN LPCE-2 (LMS-9000C) \uace0\uc815\ubc00 \ubd84\uad11 \ubc29 \uc0ac\uacc4 \ud1b5\ud569 \uad6c \uc2dc\uc2a4\ud15c 10 \ub144 \uc774\uc0c1 \uc2dc\uc7a5\uc5d0 \ucd9c\uc2dc\ub418\uc5c8\uc73c\uba70 LISUN \uc5d4\uc9c0\ub2c8\uc5b4 \uc11c\ube44\uc2a4 \ud300\uc740 \uc774\ubbf8 \uc704\uc758 \ub9c1\ud06c\uc5d0\uc11c \ub300\ubd80\ubd84\uc758 \ud310\ub9e4 \ud6c4 \uc9c8\ubb38\uacfc \ub2f5\ubcc0\uc744 \uc694\uc57d\ud588\uc2b5\ub2c8\ub2e4. \uae30\uae30\ub97c \uc0ac\uc6a9\ud558\ub294 \ub3d9\uc548 \uc9c8\ubb38\uc774\uc788\ub294 \uacbd\uc6b0 \ub300\ubd80\ubd84\uc758 \ubb38\uc81c\ub97c \uc2a4\uc2a4\ub85c \ud574\uacb0\ud560 \uc218 \uc788\uc73c\ubbc0\ub85c\uc8fc\uc758 \uae4a\uac8c \uc77d\uc5b4\ubcf4\uc2ed\uc2dc\uc624. LISUN\uc740\uc774 \ud398\uc774\uc9c0\ub97c \uacc4\uc18d \uc5c5\ub370\uc774\ud2b8 \ud560 \uc608\uc815\uc774\uba70\uc774 \uc8fc\uc81c \ub9c1\ud06c\uc5d0\uc11c \ub354 \ub9ce\uc740 FAQ\ub97c \ucc3e\uc744 \uc218 \uc788\uc2b5\ub2c8\ub2e4.<\/p>","protected":false},"excerpt":{"rendered":"

LMS-9000C High Precision CCD Spectroradiometer is according to LM-79 clause 9.1. It is designed for any visible optical spectrum distribution analysis, mimicking various light sources in the visible region by feedback control of the radiant power emitted by individual LEDs. This LED optical spectrum analyzer is used as a transfer standard for photometric, colorimetric and […]<\/p>\n","protected":false},"author":1,"featured_media":3427,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6],"tags":[159],"class_list":["post-2402","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-products","tag-lms-9000c"],"_links":{"self":[{"href":"https:\/\/www.ledtestsystem.com\/ko\/wp-json\/wp\/v2\/posts\/2402","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.ledtestsystem.com\/ko\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.ledtestsystem.com\/ko\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.ledtestsystem.com\/ko\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.ledtestsystem.com\/ko\/wp-json\/wp\/v2\/comments?post=2402"}],"version-history":[{"count":0,"href":"https:\/\/www.ledtestsystem.com\/ko\/wp-json\/wp\/v2\/posts\/2402\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.ledtestsystem.com\/ko\/wp-json\/wp\/v2\/media\/3427"}],"wp:attachment":[{"href":"https:\/\/www.ledtestsystem.com\/ko\/wp-json\/wp\/v2\/media?parent=2402"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.ledtestsystem.com\/ko\/wp-json\/wp\/v2\/categories?post=2402"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.ledtestsystem.com\/ko\/wp-json\/wp\/v2\/tags?post=2402"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}