Loading…

Characterization of fine resolution field spectrometers using solar Fraunhofer lines and atmospheric absorption features

The accurate spectral characterization of high-resolution spectrometers is required for correctly computing, interpreting, and comparing radiance and reflectance spectra acquired at different times or by different instruments. In this paper, we describe an algorithm for the spectral characterization...

Full description

Saved in:
Bibliographic Details
Published in:Applied optics. Optical technology and biomedical optics 2010-05, Vol.49 (15), p.2858
Main Authors: Meroni, Michele, Busetto, Lorenzo, Guanter, Luis, Cogliati, Sergio, Crosta, Giovanni Franco, Migliavacca, Mirco, Panigada, Cinzia, Rossini, Micol, Colombo, Roberto
Format: Article
Language:English
Subjects:
Citations: Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c290t-d857c5e475a572a84047bb76471bb4947e7d10838f3ad48fc6d10951dcade8b53
cites
container_end_page
container_issue 15
container_start_page 2858
container_title Applied optics. Optical technology and biomedical optics
container_volume 49
creator Meroni, Michele
Busetto, Lorenzo
Guanter, Luis
Cogliati, Sergio
Crosta, Giovanni Franco
Migliavacca, Mirco
Panigada, Cinzia
Rossini, Micol
Colombo, Roberto
description The accurate spectral characterization of high-resolution spectrometers is required for correctly computing, interpreting, and comparing radiance and reflectance spectra acquired at different times or by different instruments. In this paper, we describe an algorithm for the spectral characterization of field spectrometer data using sharp atmospheric or solar absorption features present in the measured data. The algorithm retrieves systematic shifts in channel position and actual full width at half-maximum (FWHM) of the instrument by comparing data acquired during standard field spectroscopy measurement operations with a reference irradiance spectrum modeled with the MODTRAN4 radiative transfer code. Measurements from four different field spectrometers with spectral resolutions ranging from 0.05 to 3.5nm are processed and the results validated against laboratory calibration. An accurate retrieval of channel position and FWHM has been achieved, with an average error smaller than the instrument spectral sampling interval.
doi_str_mv 10.1364/AO.49.002858
format article
fullrecord <record><control><sourceid>pubmed</sourceid><recordid>TN_cdi_pubmed_primary_20490248</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>20490248</sourcerecordid><originalsourceid>FETCH-LOGICAL-c290t-d857c5e475a572a84047bb76471bb4947e7d10838f3ad48fc6d10951dcade8b53</originalsourceid><addsrcrecordid>eNo1kMFLwzAYxYMgbk5vniX_QGfSJE16HMOpMNhFz-NL8sVV2qYkLah_vcXp6fEe7_0Oj5A7ztZcVPJhc1jLes1YaZS5IMuSK1UIXqkFuc75gzGhZK2vyKJksmalNEvyuT1BAjdiar5hbGJPY6Ch6ZEmzLGdfqPQYOtpHtCNKXY4lzOdctO_07kCie4STP0pBky0naeZQu8pjF3Mw2kGOwo2xzScWQjjNLNvyGWANuPtn67I2-7xdftc7A9PL9vNvnBlzcbCG6WdQqkVKF2CkUxqa3UlNbdW1lKj9pwZYYIAL01w1Wxrxb0Dj8YqsSL3Z-4w2Q79cUhNB-nr-H-B-AHXtV7N</addsrcrecordid><sourcetype>Index Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Characterization of fine resolution field spectrometers using solar Fraunhofer lines and atmospheric absorption features</title><source>OSA_美国光学学会数据库1</source><creator>Meroni, Michele ; Busetto, Lorenzo ; Guanter, Luis ; Cogliati, Sergio ; Crosta, Giovanni Franco ; Migliavacca, Mirco ; Panigada, Cinzia ; Rossini, Micol ; Colombo, Roberto</creator><creatorcontrib>Meroni, Michele ; Busetto, Lorenzo ; Guanter, Luis ; Cogliati, Sergio ; Crosta, Giovanni Franco ; Migliavacca, Mirco ; Panigada, Cinzia ; Rossini, Micol ; Colombo, Roberto</creatorcontrib><description>The accurate spectral characterization of high-resolution spectrometers is required for correctly computing, interpreting, and comparing radiance and reflectance spectra acquired at different times or by different instruments. In this paper, we describe an algorithm for the spectral characterization of field spectrometer data using sharp atmospheric or solar absorption features present in the measured data. The algorithm retrieves systematic shifts in channel position and actual full width at half-maximum (FWHM) of the instrument by comparing data acquired during standard field spectroscopy measurement operations with a reference irradiance spectrum modeled with the MODTRAN4 radiative transfer code. Measurements from four different field spectrometers with spectral resolutions ranging from 0.05 to 3.5nm are processed and the results validated against laboratory calibration. An accurate retrieval of channel position and FWHM has been achieved, with an average error smaller than the instrument spectral sampling interval.</description><identifier>EISSN: 2155-3165</identifier><identifier>DOI: 10.1364/AO.49.002858</identifier><identifier>PMID: 20490248</identifier><language>eng</language><publisher>United States</publisher><subject>Algorithms ; Atmosphere - chemistry ; Environmental Monitoring - instrumentation ; Environmental Monitoring - methods ; Equipment Design ; Equipment Failure Analysis ; Refractometry ; Solar Energy ; Spectrum Analysis - instrumentation ; Spectrum Analysis - methods</subject><ispartof>Applied optics. Optical technology and biomedical optics, 2010-05, Vol.49 (15), p.2858</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c290t-d857c5e475a572a84047bb76471bb4947e7d10838f3ad48fc6d10951dcade8b53</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/20490248$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Meroni, Michele</creatorcontrib><creatorcontrib>Busetto, Lorenzo</creatorcontrib><creatorcontrib>Guanter, Luis</creatorcontrib><creatorcontrib>Cogliati, Sergio</creatorcontrib><creatorcontrib>Crosta, Giovanni Franco</creatorcontrib><creatorcontrib>Migliavacca, Mirco</creatorcontrib><creatorcontrib>Panigada, Cinzia</creatorcontrib><creatorcontrib>Rossini, Micol</creatorcontrib><creatorcontrib>Colombo, Roberto</creatorcontrib><title>Characterization of fine resolution field spectrometers using solar Fraunhofer lines and atmospheric absorption features</title><title>Applied optics. Optical technology and biomedical optics</title><addtitle>Appl Opt</addtitle><description>The accurate spectral characterization of high-resolution spectrometers is required for correctly computing, interpreting, and comparing radiance and reflectance spectra acquired at different times or by different instruments. In this paper, we describe an algorithm for the spectral characterization of field spectrometer data using sharp atmospheric or solar absorption features present in the measured data. The algorithm retrieves systematic shifts in channel position and actual full width at half-maximum (FWHM) of the instrument by comparing data acquired during standard field spectroscopy measurement operations with a reference irradiance spectrum modeled with the MODTRAN4 radiative transfer code. Measurements from four different field spectrometers with spectral resolutions ranging from 0.05 to 3.5nm are processed and the results validated against laboratory calibration. An accurate retrieval of channel position and FWHM has been achieved, with an average error smaller than the instrument spectral sampling interval.</description><subject>Algorithms</subject><subject>Atmosphere - chemistry</subject><subject>Environmental Monitoring - instrumentation</subject><subject>Environmental Monitoring - methods</subject><subject>Equipment Design</subject><subject>Equipment Failure Analysis</subject><subject>Refractometry</subject><subject>Solar Energy</subject><subject>Spectrum Analysis - instrumentation</subject><subject>Spectrum Analysis - methods</subject><issn>2155-3165</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNo1kMFLwzAYxYMgbk5vniX_QGfSJE16HMOpMNhFz-NL8sVV2qYkLah_vcXp6fEe7_0Oj5A7ztZcVPJhc1jLes1YaZS5IMuSK1UIXqkFuc75gzGhZK2vyKJksmalNEvyuT1BAjdiar5hbGJPY6Ch6ZEmzLGdfqPQYOtpHtCNKXY4lzOdctO_07kCie4STP0pBky0naeZQu8pjF3Mw2kGOwo2xzScWQjjNLNvyGWANuPtn67I2-7xdftc7A9PL9vNvnBlzcbCG6WdQqkVKF2CkUxqa3UlNbdW1lKj9pwZYYIAL01w1Wxrxb0Dj8YqsSL3Z-4w2Q79cUhNB-nr-H-B-AHXtV7N</recordid><startdate>20100520</startdate><enddate>20100520</enddate><creator>Meroni, Michele</creator><creator>Busetto, Lorenzo</creator><creator>Guanter, Luis</creator><creator>Cogliati, Sergio</creator><creator>Crosta, Giovanni Franco</creator><creator>Migliavacca, Mirco</creator><creator>Panigada, Cinzia</creator><creator>Rossini, Micol</creator><creator>Colombo, Roberto</creator><scope>CGR</scope><scope>CUY</scope><scope>CVF</scope><scope>ECM</scope><scope>EIF</scope><scope>NPM</scope></search><sort><creationdate>20100520</creationdate><title>Characterization of fine resolution field spectrometers using solar Fraunhofer lines and atmospheric absorption features</title><author>Meroni, Michele ; Busetto, Lorenzo ; Guanter, Luis ; Cogliati, Sergio ; Crosta, Giovanni Franco ; Migliavacca, Mirco ; Panigada, Cinzia ; Rossini, Micol ; Colombo, Roberto</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c290t-d857c5e475a572a84047bb76471bb4947e7d10838f3ad48fc6d10951dcade8b53</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Algorithms</topic><topic>Atmosphere - chemistry</topic><topic>Environmental Monitoring - instrumentation</topic><topic>Environmental Monitoring - methods</topic><topic>Equipment Design</topic><topic>Equipment Failure Analysis</topic><topic>Refractometry</topic><topic>Solar Energy</topic><topic>Spectrum Analysis - instrumentation</topic><topic>Spectrum Analysis - methods</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Meroni, Michele</creatorcontrib><creatorcontrib>Busetto, Lorenzo</creatorcontrib><creatorcontrib>Guanter, Luis</creatorcontrib><creatorcontrib>Cogliati, Sergio</creatorcontrib><creatorcontrib>Crosta, Giovanni Franco</creatorcontrib><creatorcontrib>Migliavacca, Mirco</creatorcontrib><creatorcontrib>Panigada, Cinzia</creatorcontrib><creatorcontrib>Rossini, Micol</creatorcontrib><creatorcontrib>Colombo, Roberto</creatorcontrib><collection>Medline</collection><collection>MEDLINE</collection><collection>MEDLINE (Ovid)</collection><collection>MEDLINE</collection><collection>MEDLINE</collection><collection>PubMed</collection><jtitle>Applied optics. Optical technology and biomedical optics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Meroni, Michele</au><au>Busetto, Lorenzo</au><au>Guanter, Luis</au><au>Cogliati, Sergio</au><au>Crosta, Giovanni Franco</au><au>Migliavacca, Mirco</au><au>Panigada, Cinzia</au><au>Rossini, Micol</au><au>Colombo, Roberto</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Characterization of fine resolution field spectrometers using solar Fraunhofer lines and atmospheric absorption features</atitle><jtitle>Applied optics. Optical technology and biomedical optics</jtitle><addtitle>Appl Opt</addtitle><date>2010-05-20</date><risdate>2010</risdate><volume>49</volume><issue>15</issue><spage>2858</spage><pages>2858-</pages><eissn>2155-3165</eissn><abstract>The accurate spectral characterization of high-resolution spectrometers is required for correctly computing, interpreting, and comparing radiance and reflectance spectra acquired at different times or by different instruments. In this paper, we describe an algorithm for the spectral characterization of field spectrometer data using sharp atmospheric or solar absorption features present in the measured data. The algorithm retrieves systematic shifts in channel position and actual full width at half-maximum (FWHM) of the instrument by comparing data acquired during standard field spectroscopy measurement operations with a reference irradiance spectrum modeled with the MODTRAN4 radiative transfer code. Measurements from four different field spectrometers with spectral resolutions ranging from 0.05 to 3.5nm are processed and the results validated against laboratory calibration. An accurate retrieval of channel position and FWHM has been achieved, with an average error smaller than the instrument spectral sampling interval.</abstract><cop>United States</cop><pmid>20490248</pmid><doi>10.1364/AO.49.002858</doi></addata></record>
fulltext fulltext
identifier EISSN: 2155-3165
ispartof Applied optics. Optical technology and biomedical optics, 2010-05, Vol.49 (15), p.2858
issn 2155-3165
language eng
recordid cdi_pubmed_primary_20490248
source OSA_美国光学学会数据库1
subjects Algorithms
Atmosphere - chemistry
Environmental Monitoring - instrumentation
Environmental Monitoring - methods
Equipment Design
Equipment Failure Analysis
Refractometry
Solar Energy
Spectrum Analysis - instrumentation
Spectrum Analysis - methods
title Characterization of fine resolution field spectrometers using solar Fraunhofer lines and atmospheric absorption features
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-25T20%3A47%3A13IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-pubmed&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Characterization%20of%20fine%20resolution%20field%20spectrometers%20using%20solar%20Fraunhofer%20lines%20and%20atmospheric%20absorption%20features&rft.jtitle=Applied%20optics.%20Optical%20technology%20and%20biomedical%20optics&rft.au=Meroni,%20Michele&rft.date=2010-05-20&rft.volume=49&rft.issue=15&rft.spage=2858&rft.pages=2858-&rft.eissn=2155-3165&rft_id=info:doi/10.1364/AO.49.002858&rft_dat=%3Cpubmed%3E20490248%3C/pubmed%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c290t-d857c5e475a572a84047bb76471bb4947e7d10838f3ad48fc6d10951dcade8b53%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/20490248&rfr_iscdi=true