Results from the intercalibration of optical low light calibration sources 2011

被引:7
作者
Brandstrom, B. U. E. [1 ]
Enell, C. -F. [2 ]
Widell, O. [3 ]
Hansson, T. [3 ]
Whiter, D. [4 ]
Makinen, S. [4 ]
Mikhaylova, D. [1 ]
Axelsson, K. [1 ]
Sigernes, F. [5 ]
Gulbrandsen, N. [6 ]
Schlatter, N. M. [7 ]
Gjendem, A. G. [8 ]
Cai, L. [9 ]
Reistad, J. P. [10 ]
Daae, M. [8 ]
Demissie, T. D. [8 ]
Andalsvik, Y. L. [11 ]
Roberts, O. [12 ]
Poluyanov, S. [13 ]
Chernouss, S. [14 ]
机构
[1] Swedish Inst Space Phys, S-98128 Kiruna, Sweden
[2] Univ Oulu, Sodankyla Geophys Observ, Sodankyla, Finland
[3] ESRANGE, SSC, Kiruna, Sweden
[4] Finnish Meteorol Inst, FIN-00101 Helsinki, Finland
[5] UNIS, Kjell Henriksen Observ, Longyearbyen, Norway
[6] Univ Tromso, Tromso, Norway
[7] Royal Inst Technol, Sch Elect Engn, Stockholm, Sweden
[8] Norwegian Univ Sci & Technol, N-7034 Trondheim, Norway
[9] Univ Oulu, Dept Phys, FIN-90570 Oulu, Finland
[10] Univ Bergen, Bergen, Norway
[11] Univ Oslo, Dept Phys, Oslo, Norway
[12] Aberystwyth Univ, Aberystwyth, Dyfed, Wales
[13] Polar Geophys Inst, Murmansk, Russia
[14] Polar Geophys Inst, Apatity, Russia
关键词
D O I
10.5194/gi-1-43-2012
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Following the 38th Annual European Meeting on Atmospheric Studies by Optical Methods in Siuntio in Finland, an intercalibration workshop for optical low light calibration sources was held in Sodankyla, Finland. The main purpose of this workshop was to provide a comparable scale for absolute measurements of aurora and airglow. All sources brought to the intercalibration workshop were compared to the Fritz Peak reference source using the Lindau Calibration Photometer built by Wilhelm Barke and Hans Lauche in 1984. The results were compared to several earlier intercalibration workshops. It was found that most sources were fairly stable over time, with errors in the range of 5-25 %. To further validate the results, two sources were also intercalibrated at UNIS, Longyearbyen, Svalbard. Preliminary analysis indicates agreement with the intercalibration in Sodankyla within about 15-25 %.
引用
收藏
页码:43 / 51
页数:9
相关论文
共 28 条
[1]   RAYLEIGH - INTERPRETATION OF UNIT IN TERMS OF COLUMN EMISSION RATE OR APPARENT RADIANCE EXPRESSED IN SI UNITS [J].
BAKER, DJ ;
ROMICK, GJ .
APPLIED OPTICS, 1976, 15 (08) :1966-1968
[2]   RAYLEIGH, UNIT FOR LIGHT RADIANCE [J].
BAKER, DJ .
APPLIED OPTICS, 1974, 13 (09) :2160-2163
[3]  
Br&auml
[4]  
ndstr&ouml
[5]  
m U., 2003, 279 IRF
[6]  
Chamberlain J. W., 1961, CLASSICS GEOPHYS
[7]   Energy and flux variations across thin auroral arcs [J].
Dahlgren, H. ;
Gustavsson, B. ;
Lanchester, B. S. ;
Ivchenko, N. ;
Brandstrom, U. ;
Whiter, D. K. ;
Sergienko, T. ;
Sandahl, I. ;
Marklund, G. .
ANNALES GEOPHYSICAE, 2011, 29 (10) :1699-1712
[8]  
Espy P., 1981, 101 UT STAT U CTR AT
[9]   Electron gyroharmonic effects in ionization and electron acceleration during high-frequency pumping in the ionosphere [J].
Gustavsson, B. ;
Leyser, T. B. ;
Kosch, M. ;
Rietveld, M. T. ;
Steen, A. ;
Brandstrom, B. U. E. ;
Aso, T. .
PHYSICAL REVIEW LETTERS, 2006, 97 (19)
[10]  
Henricson H., 2008, P 33 ANN EUR M ATM S, V292, P131