Data Quality Objectives (DQO) for Solar Ultraviolet Radiation

被引:0
作者
Diaz, Susana [1 ]
Fioletov, Vitali [2 ]
Herman, Jay [3 ]
Jalkanen, Liisa [4 ]
Janjai, Serm [5 ]
Kjeldstad, Berit [6 ]
Koide, Takashi [7 ]
Seckmeyer, Gunther [8 ]
Simon, Paul [9 ]
Weatherhead, Betsy [10 ]
Webb, Ann [11 ]
机构
[1] Consejo Nacl Invest Cient & Tecn, INGEBI CADIC, Vuelta Obligado 2490, RA-1428 Buenos Aires, DF, Argentina
[2] Meteorol Serv Canada, Air Qual Res, Expt Studies Div, Toronto, ON M3H 5T4, Canada
[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[4] AER, RES, WMO Secretariat, CH-1211 Geneva, Switzerland
[5] Silpakorn Univ, Fac Sci, Dept Phys, Nakhon Pathom 73000, Thailand
[6] Norwegian Univ Sci & Technol, Dept Phys, N-7491 Trondheim, Norway
[7] Japan Meteorol Agcy, Ozone Layer Monitoring Off, Tokyo 1008122, Japan
[8] Leibniz Univ Hannover, Inst Meteorol & Climatol, D-30419 Hannover, Germany
[9] Inst Aeron Spatiale Belgique, B-1180 Brussels, Belgium
[10] NOAA, ERL R E, ARXI, Boulder, CO 80305 USA
[11] Univ Manchester, Sch Earth Atm & Environm Sci, Manchester M13 9PL, Lancs, England
来源
CURRENT PROBLEMS IN ATMOSPHERIC RADIATION (IRS 2008) | 2009年 / 1100卷
关键词
Ultraviolet Radiation; Data Quality; Instruments;
D O I
暂无
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
General objectives for measuring solar ultraviolet (UV) irradiance are: a) To establish a UV climatology by long-term monitoring, e.g. within a network, b) To detect trends in global UV irradiance. c) To provide datasets for specific process studies and for the validation of radiative transfer models and/or satellite derived UV irradiance at the Earth's surface, d) To understand geographic differences in global UV irradiance, c) To gain information about actual UV levels and their diurnal and seasonal variability, f) To provide data for public information and awareness (e.g. UV index). Solar ultraviolet radiation can be measured by different classes of instrument and it is crucial to match the instrument employed to the intended objective. It should also be ensured that sufficient facilities are available to Support the objective in terms of personnel and QA/QC requirements. The three classes of instrument available for solar UV measurement are spectral, broadband and multifilter. Spectral instruments are the most costly, complex and demanding of those available, but provide the most versatile data. Broadband radiometers, tend to be cheaper and have fewer operational problems than spectroradiometers. However, their maintenance and QA/QC can introduce substantial additional cost. Multifilter radiometers combine some of the properties of both broadband and spectral instruments. Not all the above mentioned instruments are suited to all of the objectives. To achieve objectives a,d,e and f, any class of instrument can be used, but it is necessary that it accomplishes a minimum requirement in quality. The second listed objective, trend detection, is the most demanding goal of UV monitoring, and spectral instruments are most suited to this task. The instrument specifications and the QA/QC requirements necessary to enable detection of small trends are very stringent and must be maintained over it prolonged period to justify trend detection. Providing datasets for process studies or satellite validation (objective c) is again best served by spectral instruments. For the validation of radiative transfer models the accuracy of spectral measurements must be comparable to the accuracy needed for trend detection.
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页码:663 / +
页数:2
相关论文
共 7 条
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