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2) Spectral Irradiance – Ultraviolet and Visible – Schreder<\/h2>\n
A 200 W quartz halogen lamp (KS-J1011-LAMP, Schreder, Austria) is calibrated over 250-500 nm. Calibration entrance can accept a CC-UV\/VIS or a weatherproof global entrance optics (UV-J1002-SMA-SHUT, Schreder, Austria).<\/p>\n
tes\/520\/2019\/08\/Spectral-Irradiance-Ultraviolet-and-Visible-Schreder-300×144.png” alt=”” width=”238″ height=”114″ \/><\/a><\/p>\n <\/p>\n A Deuterium and Halogen lamp (DH-2000, Ocean Optics, USA) calibrated over 250-1000nm. The calibration entrance can accept a CC-UV\/VIS probe.<\/p>\n <\/p>\n A calibrated Argon source (Avalight, CAL-AR-Mini, Avantes, Netherlands) has emission lines between 965 nm and 1400 nm that can be employed to calibrate spectrometers in the near-infrared spectral region.<\/p>\n <\/p>\n Mercury and Argon Calibration source (HG-1, Ocean optics, lines 253 and 922 nm).<\/p>\n <\/p>\n Spectrometers (USB4000 and USB2000+, Ocean Optics, Dunedin, USA) calibrated to measure the spectral irradiance in the range of 290\u2013700 nm equipped with optical fibers and cosine-corrected irradiance probes (CC-3-UV, Ocean Optics, Dunedin, USA).<\/p>\n <\/p>\n A 10″ Calibrated integrating sphere system (Illumina, Labsphere, North Sutton, NH, USA) equipped with a spectrometer (CDS 610, Labsphere, Nrth Sutton, NH, USA) to measure the spectral power over 350-1000 nm spectral range.<\/p>\n <\/p>\n The laboratory is equipped with several detectors to measure the power from 10 nW for emissions in the visible spectral range and from 10 \u00b5W in infrared; and pulsed lasers energy with values above 10\u00b5J.<\/p>\n 1) Spectral Irradiance – Visible and Near-Infrared Visible and Near-Infrared calibrated light source (Avalight-HAL-CAL-MINI, Avantes, Netherlands) is a halogen lamp calibrated over 350-1100 nm spectral range with a resolution of 10 nm. Calibration for a CC-VIS\/NIR probe at 0.1757 m distant from the entrance. 2) Spectral Irradiance – Ultraviolet and Visible – Schreder A […]<\/p>\n","protected":false},"author":974,"featured_media":0,"parent":64,"menu_order":2,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":"","_links_to":"","_links_to_target":""},"class_list":["post-198","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/sites.usp.br\/fotobiofisica\/wp-json\/wp\/v2\/pages\/198","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/sites.usp.br\/fotobiofisica\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/sites.usp.br\/fotobiofisica\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/sites.usp.br\/fotobiofisica\/wp-json\/wp\/v2\/users\/974"}],"replies":[{"embeddable":true,"href":"https:\/\/sites.usp.br\/fotobiofisica\/wp-json\/wp\/v2\/comments?post=198"}],"version-history":[{"count":4,"href":"https:\/\/sites.usp.br\/fotobiofisica\/wp-json\/wp\/v2\/pages\/198\/revisions"}],"predecessor-version":[{"id":723,"href":"https:\/\/sites.usp.br\/fotobiofisica\/wp-json\/wp\/v2\/pages\/198\/revisions\/723"}],"up":[{"embeddable":true,"href":"https:\/\/sites.usp.br\/fotobiofisica\/wp-json\/wp\/v2\/pages\/64"}],"wp:attachment":[{"href":"https:\/\/sites.usp.br\/fotobiofisica\/wp-json\/wp\/v2\/media?parent=198"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}3) Spectral Irradiance – Ultraviolet and Visible – Ocean Optics<\/h2>\n
<\/a><\/p>\n4) Wavelength calibration – Near-Infrared<\/h2>\n
<\/a><\/a><\/p>\n5) Wavelength calibration – Ultraviolet and visible<\/h2>\n
<\/a><\/p>\n6) Spectroradiometer for Ultraviolet and Visible<\/h2>\n
<\/a><\/a><\/p>\n7) – Spectral power – Visible<\/h2>\n
<\/a><\/p>\n8) Laser detectors – power and energy<\/h2>\n
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