Fast and flexible CCD-driver system using fast DAC and FPGA

被引:31
作者
Miyata, E
Natsukari, C
Akutsu, D
Kamazuka, T
Nomachi, M
Ozaki, M
机构
[1] Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Toyonaka, Osaka 5600043, Japan
[2] Osaka Univ, Grad Sch Sci, Dept Phys, Toyonaka, Osaka 5600043, Japan
关键词
D O I
10.1016/S0168-9002(00)01015-9
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
We have developed a completely new type of general-purpose CCD-data acquisition system which enables one to drive any type of CCD using any type of clocking mode. A CCD driver system widely used before consisted of an analog multiplexer (MPX), a digital-to-analog converter (DAC), and an operational amplifier. A DAC is used to determine high- and low-voltage levels and the MPX selects each voltage level using a TTL clock. In this kind of driver board, it is difficult to reduce the noise caused by an electrical short between high and low levels in MPX and also to select many kinds of different voltage levels. Recent developments in semiconductor IC enable us to use a very fast sampling(similar to 10 MKz) DAC with low cost, We thus develop the new driver system using a fast DAC in order to determine both the voltage level of the clock and the clocking timing. We use Field Programmable Gate Array (FPGA) to control the DAC. We have constructed the data acquisition system and found that the CCD functions well with our new system. The energy resolution of Mn K-alpha has a full-width at half-maximum of similar or equal to 150 eV and the readout noise of our system is similar or equal to 8e(-). (C) 2001 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:157 / 164
页数:8
相关论文
共 11 条
[1]  
*ALT CORP, 1998, MAX PLUS PLUS 2 PROG
[2]  
[Anonymous], 1988, VHDL LANG REF MAN IE, P1076
[3]  
BARR P, 1988, ESA SP
[4]   SCIENTIFIC CHARGE-COUPLED-DEVICES [J].
JANESICK, JR ;
ELLIOTT, T ;
COLLINS, S ;
BLOUKE, MM ;
FREEMAN, J .
OPTICAL ENGINEERING, 1987, 26 (08) :692-714
[5]   Verification of the Astro-E Hard X-ray Detector based on newly developed Ground Support Equipment [J].
Kataoka, J ;
Nomachi, M ;
Takahashi, T ;
Kawaguchi, G ;
Terada, Y ;
Murakami, T ;
Tanihata, C ;
Uchiyama, Y ;
Yamaoka, K ;
Fukazawa, Y ;
Kamae, T ;
Makishima, K ;
Tashiro, M ;
Kubo, H .
EUV, X-RAY, AND GAMMA-RAY INSTRUMENTATION FOR ASTRONOMY IX, 1998, 3445 :143-154
[6]   MAXI (monitor of all-sky X-ray image) for JEM on the Space Station [J].
Matsuoka, M ;
Kawai, N ;
Mihara, T ;
Yoshida, A ;
Kubo, H ;
Kotani, T ;
Negoro, H ;
Rubin, BC ;
Shimizu, HM ;
Tsunemi, H ;
Hayashida, K ;
Kitamoto, S ;
Miyata, E ;
Yamauchi, M .
EUX, X-RAY, AND GAMMA-RAY INSTRUMENTATION FOR ASTRONOMY VIII, 1997, 3114 :414-421
[7]  
RICKER GR, 1998, P ALL SKY XRAY OBSER, P366
[8]  
TANAKA Y, 1994, PUBL ASTRON SOC JPN, V46, pL37
[9]  
THOMAS DE, 1991, VERILOG HARDWARE DES
[10]  
WEISSKOPF MC, 1995, P SOC PHOTO-OPT INS, V2515, P312, DOI 10.1117/12.212599