Initial Calibration of the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)

被引:398
作者
Boerner, Paul [1 ]
Edwards, Christopher [1 ]
Lemen, James [1 ]
Rausch, Adam [1 ]
Schrijver, Carolus [1 ]
Shine, Richard [1 ]
Shing, Lawrence [1 ]
Stern, Robert [1 ]
Tarbell, Theodore [1 ]
Title, Alan [1 ]
Wolfson, C. Jacob [1 ]
Soufli, Regina [2 ]
Spiller, Eberhard [2 ]
Gullikson, Eric [3 ]
McKenzie, David [4 ]
Windt, David [5 ]
Golub, Leon [6 ]
Podgorski, William [6 ]
Testa, Paola [6 ]
Weber, Mark [6 ]
机构
[1] Lockheed Martin Adv Technol Ctr, Solar & Astrophys Lab, Dept ADBS, Palo Alto, CA 94304 USA
[2] Lawrence Livermore Natl Lab, Livermore, CA USA
[3] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA
[4] Montana State Univ, Bozeman, MT 59717 USA
[5] Reflect Xray Opt LLC, New York, NY USA
[6] Smithsonian Astrophys Observ, Cambridge, MA USA
关键词
Instrumentation; EUV; Soft X-ray; Chromosphere; Corona; Transition region; X-RAY; EXTREME-ULTRAVIOLET; EMISSION-LINES; ATOMIC DATABASE; ANGSTROM; TRACE; WAVELENGTHS; SPECTRUM; CHIANTI;
D O I
10.1007/s11207-011-9804-8
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Atmospheric Imaging Assembly (AIA) instrument onboard the Solar Dynamics Observatory (SDO) is an array of four normal-incidence reflecting telescopes that image the Sun in ten EUV and UV wavelength channels. We present the initial photometric calibration of AIA, based on preflight measurements of the response of the telescope components. The estimated accuracy is of order 25%, which is consistent with the results of comparisons with full-disk irradiance measurements and spectral models. We also describe the characterization of the instrument performance, including image resolution, alignment, camera-system gain, flat-fielding, and data compression.
引用
收藏
页码:41 / 66
页数:26
相关论文
共 30 条
[1]  
CATURA RC, 1987, P SOC PHOTO-OPT INS, V830, P204
[2]   SOLAR CORONAL STRUCTURE AND STRAY LIGHT IN TRACE [J].
DeForest, C. E. ;
Martens, P. C. H. ;
Wills-Davey, M. J. .
ASTROPHYSICAL JOURNAL, 2009, 690 (02) :1264-1271
[3]  
Dere KP, 2009, ASTRON ASTROPHYS, V498, P915, DOI 10.1051/0004-6361/200911712
[4]   CHIANTI - an atomic database for emission lines .1. Wavelengths greater than 50 angstrom [J].
Dere, KP ;
Landi, E ;
Mason, HE ;
Fossi, BCM ;
Young, PR .
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1997, 125 (01) :149-173
[5]   The preflight photometric calibration of the extreme-ultraviolet imaging telescope EIT [J].
Dere, KP ;
Moses, JD ;
Delaboudinière, JP ;
Brunaud, J ;
Carabetian, C ;
Hochedez, JF ;
Song, XY ;
Catura, RC ;
Clette, F ;
Defise, JM .
SOLAR PHYSICS, 2000, 195 (01) :13-44
[6]   ELEMENTAL ABUNDANCES IN THE UPPER SOLAR ATMOSPHERE OF QUIET AND CORONAL HOLE REGIONS (TE APPROXIMATE-TO 4.3 X 10(5) K) [J].
FELDMAN, U ;
WIDING, KG .
ASTROPHYSICAL JOURNAL, 1993, 414 (01) :381-388
[7]   Data analysis with the solarsoft system [J].
Freeland, SL ;
Handy, BN .
SOLAR PHYSICS, 1998, 182 (02) :497-500
[8]   The TRACE telescope point spread function for the 171 Å filter [J].
Gburek, S. ;
Sylwester, J. ;
Martens, P. .
SOLAR PHYSICS, 2006, 239 (1-2) :531-548
[9]   The transition region and coronal explorer [J].
Handy, BN ;
Acton, LW ;
Kankelborg, CC ;
Wolfson, CJ ;
Akin, DJ ;
Bruner, ME ;
Caravalho, R ;
Catura, RC ;
Chevalier, R ;
Duncan, DW ;
Edwards, CG ;
Feinstein, CN ;
Freeland, SL ;
Friedlaender, FM ;
Hoffmann, CH ;
Hurlburt, NE ;
Jurcevich, BK ;
Katz, NL ;
Kelly, GA ;
Lemen, JR ;
Levay, M ;
Lindgren, RW ;
Mathur, DP ;
Meyer, SB ;
Morrison, SJ ;
Morrison, MD ;
Nightingale, RW ;
Pope, TP ;
Rehse, RA ;
Schrijver, CJ ;
Shine, RA ;
Shing, L ;
Strong, KT ;
Tarbell, TD ;
Title, AM ;
Torgerson, DD ;
Golub, L ;
Bookbinder, JA ;
Caldwell, D ;
Cheimets, PN ;
Davis, WN ;
Deluca, EE ;
McMullen, RA ;
Warren, HP ;
Amato, D ;
Fisher, R ;
Maldonado, H ;
Parkinson, C .
SOLAR PHYSICS, 1999, 187 (02) :229-260
[10]   X-RAY INTERACTIONS - PHOTOABSORPTION, SCATTERING, TRANSMISSION, AND REFLECTION AT E=50-30,000 EV, Z=1-92 [J].
HENKE, BL ;
GULLIKSON, EM ;
DAVIS, JC .
ATOMIC DATA AND NUCLEAR DATA TABLES, 1993, 54 (02) :181-342