diff options
author | Philip Lampkin <plampkin@chem.wisc.edu> | 2021-04-24 11:49:29 -0500 |
---|---|---|
committer | Philip Lampkin <plampkin@chem.wisc.edu> | 2021-04-24 11:49:29 -0500 |
commit | 7bd5517a48d0ade29b432b302ebc20b155f301fb (patch) | |
tree | 169bbd20a7dcfcd2e100e9566d19dbc96f10583f /lightsource-leds | |
parent | be8617c48b0a25bf225737f4dbe5cdb7e98ee5b3 (diff) | |
parent | f8372e54025c0299d9a9c05ba5602f854f09ba8f (diff) |
Merge branch 'terminology' of https://github.com/plampkin/wisconsin-photoreactor into terminology
Diffstat (limited to 'lightsource-leds')
-rw-r--r-- | lightsource-leds/README.md | 32 |
1 files changed, 15 insertions, 17 deletions
diff --git a/lightsource-leds/README.md b/lightsource-leds/README.md index 2f34384..15be9fa 100644 --- a/lightsource-leds/README.md +++ b/lightsource-leds/README.md @@ -1,10 +1,10 @@ -# Lightsource LEDS +# Photon Source LEDS -The WPR light source is built around 3 high-power, monochromatic LEDs mounted onto an industry-standard 20 mm LED star package. +The WPP photon source consists of 3 high-power, single-color LEDs mounted onto an industry-standard 20 mm LED star package. -WPR-comptabile LED stars emitting narrow wavelength ranges across the UV-Visible spectrum are available from multiple vendors. A few are detailed below. +WPP-comptabile LED stars emitting narrow wavelength ranges across the UV-Visible spectrum are available from multiple vendors. A few are detailed below. -CPR-comptabible custom LED stars mounted with 3.5 mm surface mount LEDs of any wavelength can be fabricated using a reflow oven. +WPP-comptabible custom LED stars mounted with 3.5 mm surface mount LEDs of any wavelength can be fabricated using a reflow oven. See the fabrication instructions for more information. ## List of compatible commerical LED stars @@ -25,30 +25,28 @@ In general, prices are overestimates, thereby providing an upper-estimate on cos ## Commerical LED emission spectra -LED emission spectra were measured using an [Ocean Insight USB2000 Spectrometer](https://www.oceaninsight.com/products/spectrometers/general-purpose-spectrometer/flame-series/flame-vis-nir/) loaned by the [Goldsmith Group](https://goldsmith.chem.wisc.edu). +LED emission spectra below were measured using an Ocean Insight USB2000 Spectrometer loaned by the [Goldsmith Group](https://goldsmith.chem.wisc.edu). -![UVA](./UVA - 365 nm - IN-C39CTOU2.png "UVA Led emission spectra") +![UVA](./UVA-365-nm-IN-C39CTOU2.png) -![Violet](./Violet - 395 nm - IN-C39CTOU5.png "Violet Led emission spectra") +![Violet](./Violet-395-nm-IN-C39CTOU5.png) -![Blue](./Blue - 450 nm - XTEARY-00-0000-000000N09.png "Blue Led emission spectra") +![Blue](./Blue-450-nm-XTEARY-00-0000-000000N09.png) -![Cyan](./Cyan - 495 nm - LXML-PE01-0080.png "Cyan Led emission spectra") +![Cyan](./Cyan-495-nm-LXML-PE01-0080.png) -![Green](./Green - 530 nm - XPEBGR-L1-0000-00D01.png "Green Led emission spectra") +![Green](./Green-530-nm-XPEBGR-L1-0000-00D01.png) -![Amber](./Amber - 595 nm - LXML-PL01-0060.png "Green Led emission spectra") +![Amber](./Amber-595-nm-LXML-PL01-0060.png) -![Orange](./Orange - 620 nm - XPEBRO-L1-0000-00901.png "Orange Led emission spectra") +![Orange](./Orange-620-nm-XPEBRO-L1-0000-00901.png) -![Red](./ Red - 660 nm - XPEPHR-L1-0000-00801.png "Red Led emission spectra") +![Red](./Red-660-nm-XPEPHR-L1-0000-00801.png) -![NIR](./ NIR - 730 nm - XPEFAR-L1-0000-00601.png "NiR Led emission spectra") +![NIR](./NIR-730-nm-XPEFAR-L1-0000-00601.png) ## Ordering Blank LED stars -The WPR lightsource is built to fit an industry-standard, 20 mm [Indus Star A008 high power LED modules](https://leddynamics.com/indus-star-a007-a008). +The WPP lightsource is designed to fit an industry-standard, 20 mm [Indus Star A008 high power LED modules](https://leddynamics.com/indus-star-a007-a008). To order blank Indus Star A008 LED stars for custom LED star creation, contact [LEDsupply](https://www.ledsupply.com/contact-us), [LEDdynamics](https://leddynamics.com/contact-us) or other vendors. - -Different 20 mm 3-up LED stars in industry standard packages could be incorporated into the WPR, but have not been tested. |