Readout electronics of a prototype spectrometer for measuring low-energy ions in solar wind plasma
Abstract Readout electronics is developed for a prototype spectrometer for in situ measurement of low-energy ions of 30 eV/e–20 keV/e in the solar wind plasma. A low-noise preamplifier/discriminator (A111F) is employed for each channel to process the signal from micro-channel plate (MCP) detectors....
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Yang, Di [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2016 |
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| Schlagwörter: |
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| Anmerkung: |
© Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Chinese Nuclear Society, Science Press China and Springer Science+Business Media Singapore 2016 |
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| Übergeordnetes Werk: |
Enthalten in: Nuclear science and techniques - Singapore : Springer, 2006, 27(2016), 6 vom: 12. Okt. |
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| Übergeordnetes Werk: |
volume:27 ; year:2016 ; number:6 ; day:12 ; month:10 |
| Links: |
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| DOI / URN: |
10.1007/s41365-016-0136-0 |
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| Katalog-ID: |
SPR038194384 |
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| 100 | 1 | |a Yang, Di |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Readout electronics of a prototype spectrometer for measuring low-energy ions in solar wind plasma |
| 264 | 1 | |c 2016 | |
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| 500 | |a © Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Chinese Nuclear Society, Science Press China and Springer Science+Business Media Singapore 2016 | ||
| 520 | |a Abstract Readout electronics is developed for a prototype spectrometer for in situ measurement of low-energy ions of 30 eV/e–20 keV/e in the solar wind plasma. A low-noise preamplifier/discriminator (A111F) is employed for each channel to process the signal from micro-channel plate (MCP) detectors. A high-voltage (HV) supply solution based on a HV module and a HV optocoupler is adopted to generate a fast sweeping HV and a fixed HV. Due to limitation of telemetry bandwidth in space communication, an algorithm is implemented in an FPGA (field programmable gate array) to compress the raw data. Test results show that the electronics achieves a 1 MHz event rate and a large input dynamic range of 95 pC. A slew rate of 0.8 V/μs and an integral nonlinearity of 0.7-LSB for the sweeping HV, and a precision of less than 0.8 % for the fixed HV are obtained. A vacuum beam test shows an energy resolution of 12 ± 0.7 % full width at half maximum (FWHM) is achieved, and noise counts are less than 10/sec, indicating that the performance meets the physical requirement. | ||
| 650 | 4 | |a Solar wind plasma |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Energy spectrometer |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Readout electronics |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a A111F |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Data compression |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Cao, Zhe |4 aut | |
| 700 | 1 | |a Qin, Xi |4 aut | |
| 700 | 1 | |a Hao, Xin-Jun |4 aut | |
| 700 | 1 | |a Liu, Shu-Bin |4 aut | |
| 700 | 1 | |a Feng, Chang-Qing |4 aut | |
| 700 | 1 | |a An, Qi |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Nuclear science and techniques |d Singapore : Springer, 2006 |g 27(2016), 6 vom: 12. Okt. |w (DE-627)513219439 |w (DE-600)2238719-5 |x 2210-3147 |7 nnns |
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| 856 | 4 | 0 | |u https://dx.doi.org/10.1007/s41365-016-0136-0 |z lizenzpflichtig |3 Volltext |
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10.1007/s41365-016-0136-0 doi (DE-627)SPR038194384 (SPR)s41365-016-0136-0-e DE-627 ger DE-627 rakwb eng Yang, Di verfasserin aut Readout electronics of a prototype spectrometer for measuring low-energy ions in solar wind plasma 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Chinese Nuclear Society, Science Press China and Springer Science+Business Media Singapore 2016 Abstract Readout electronics is developed for a prototype spectrometer for in situ measurement of low-energy ions of 30 eV/e–20 keV/e in the solar wind plasma. A low-noise preamplifier/discriminator (A111F) is employed for each channel to process the signal from micro-channel plate (MCP) detectors. A high-voltage (HV) supply solution based on a HV module and a HV optocoupler is adopted to generate a fast sweeping HV and a fixed HV. Due to limitation of telemetry bandwidth in space communication, an algorithm is implemented in an FPGA (field programmable gate array) to compress the raw data. Test results show that the electronics achieves a 1 MHz event rate and a large input dynamic range of 95 pC. A slew rate of 0.8 V/μs and an integral nonlinearity of 0.7-LSB for the sweeping HV, and a precision of less than 0.8 % for the fixed HV are obtained. A vacuum beam test shows an energy resolution of 12 ± 0.7 % full width at half maximum (FWHM) is achieved, and noise counts are less than 10/sec, indicating that the performance meets the physical requirement. Solar wind plasma (dpeaa)DE-He213 Energy spectrometer (dpeaa)DE-He213 Readout electronics (dpeaa)DE-He213 A111F (dpeaa)DE-He213 Data compression (dpeaa)DE-He213 Cao, Zhe aut Qin, Xi aut Hao, Xin-Jun aut Liu, Shu-Bin aut Feng, Chang-Qing aut An, Qi aut Enthalten in Nuclear science and techniques Singapore : Springer, 2006 27(2016), 6 vom: 12. Okt. (DE-627)513219439 (DE-600)2238719-5 2210-3147 nnns volume:27 year:2016 number:6 day:12 month:10 https://dx.doi.org/10.1007/s41365-016-0136-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 27 2016 6 12 10 |
| spelling |
10.1007/s41365-016-0136-0 doi (DE-627)SPR038194384 (SPR)s41365-016-0136-0-e DE-627 ger DE-627 rakwb eng Yang, Di verfasserin aut Readout electronics of a prototype spectrometer for measuring low-energy ions in solar wind plasma 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Chinese Nuclear Society, Science Press China and Springer Science+Business Media Singapore 2016 Abstract Readout electronics is developed for a prototype spectrometer for in situ measurement of low-energy ions of 30 eV/e–20 keV/e in the solar wind plasma. A low-noise preamplifier/discriminator (A111F) is employed for each channel to process the signal from micro-channel plate (MCP) detectors. A high-voltage (HV) supply solution based on a HV module and a HV optocoupler is adopted to generate a fast sweeping HV and a fixed HV. Due to limitation of telemetry bandwidth in space communication, an algorithm is implemented in an FPGA (field programmable gate array) to compress the raw data. Test results show that the electronics achieves a 1 MHz event rate and a large input dynamic range of 95 pC. A slew rate of 0.8 V/μs and an integral nonlinearity of 0.7-LSB for the sweeping HV, and a precision of less than 0.8 % for the fixed HV are obtained. A vacuum beam test shows an energy resolution of 12 ± 0.7 % full width at half maximum (FWHM) is achieved, and noise counts are less than 10/sec, indicating that the performance meets the physical requirement. Solar wind plasma (dpeaa)DE-He213 Energy spectrometer (dpeaa)DE-He213 Readout electronics (dpeaa)DE-He213 A111F (dpeaa)DE-He213 Data compression (dpeaa)DE-He213 Cao, Zhe aut Qin, Xi aut Hao, Xin-Jun aut Liu, Shu-Bin aut Feng, Chang-Qing aut An, Qi aut Enthalten in Nuclear science and techniques Singapore : Springer, 2006 27(2016), 6 vom: 12. Okt. (DE-627)513219439 (DE-600)2238719-5 2210-3147 nnns volume:27 year:2016 number:6 day:12 month:10 https://dx.doi.org/10.1007/s41365-016-0136-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 27 2016 6 12 10 |
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10.1007/s41365-016-0136-0 doi (DE-627)SPR038194384 (SPR)s41365-016-0136-0-e DE-627 ger DE-627 rakwb eng Yang, Di verfasserin aut Readout electronics of a prototype spectrometer for measuring low-energy ions in solar wind plasma 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Chinese Nuclear Society, Science Press China and Springer Science+Business Media Singapore 2016 Abstract Readout electronics is developed for a prototype spectrometer for in situ measurement of low-energy ions of 30 eV/e–20 keV/e in the solar wind plasma. A low-noise preamplifier/discriminator (A111F) is employed for each channel to process the signal from micro-channel plate (MCP) detectors. A high-voltage (HV) supply solution based on a HV module and a HV optocoupler is adopted to generate a fast sweeping HV and a fixed HV. Due to limitation of telemetry bandwidth in space communication, an algorithm is implemented in an FPGA (field programmable gate array) to compress the raw data. Test results show that the electronics achieves a 1 MHz event rate and a large input dynamic range of 95 pC. A slew rate of 0.8 V/μs and an integral nonlinearity of 0.7-LSB for the sweeping HV, and a precision of less than 0.8 % for the fixed HV are obtained. A vacuum beam test shows an energy resolution of 12 ± 0.7 % full width at half maximum (FWHM) is achieved, and noise counts are less than 10/sec, indicating that the performance meets the physical requirement. Solar wind plasma (dpeaa)DE-He213 Energy spectrometer (dpeaa)DE-He213 Readout electronics (dpeaa)DE-He213 A111F (dpeaa)DE-He213 Data compression (dpeaa)DE-He213 Cao, Zhe aut Qin, Xi aut Hao, Xin-Jun aut Liu, Shu-Bin aut Feng, Chang-Qing aut An, Qi aut Enthalten in Nuclear science and techniques Singapore : Springer, 2006 27(2016), 6 vom: 12. Okt. (DE-627)513219439 (DE-600)2238719-5 2210-3147 nnns volume:27 year:2016 number:6 day:12 month:10 https://dx.doi.org/10.1007/s41365-016-0136-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 27 2016 6 12 10 |
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10.1007/s41365-016-0136-0 doi (DE-627)SPR038194384 (SPR)s41365-016-0136-0-e DE-627 ger DE-627 rakwb eng Yang, Di verfasserin aut Readout electronics of a prototype spectrometer for measuring low-energy ions in solar wind plasma 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Chinese Nuclear Society, Science Press China and Springer Science+Business Media Singapore 2016 Abstract Readout electronics is developed for a prototype spectrometer for in situ measurement of low-energy ions of 30 eV/e–20 keV/e in the solar wind plasma. A low-noise preamplifier/discriminator (A111F) is employed for each channel to process the signal from micro-channel plate (MCP) detectors. A high-voltage (HV) supply solution based on a HV module and a HV optocoupler is adopted to generate a fast sweeping HV and a fixed HV. Due to limitation of telemetry bandwidth in space communication, an algorithm is implemented in an FPGA (field programmable gate array) to compress the raw data. Test results show that the electronics achieves a 1 MHz event rate and a large input dynamic range of 95 pC. A slew rate of 0.8 V/μs and an integral nonlinearity of 0.7-LSB for the sweeping HV, and a precision of less than 0.8 % for the fixed HV are obtained. A vacuum beam test shows an energy resolution of 12 ± 0.7 % full width at half maximum (FWHM) is achieved, and noise counts are less than 10/sec, indicating that the performance meets the physical requirement. Solar wind plasma (dpeaa)DE-He213 Energy spectrometer (dpeaa)DE-He213 Readout electronics (dpeaa)DE-He213 A111F (dpeaa)DE-He213 Data compression (dpeaa)DE-He213 Cao, Zhe aut Qin, Xi aut Hao, Xin-Jun aut Liu, Shu-Bin aut Feng, Chang-Qing aut An, Qi aut Enthalten in Nuclear science and techniques Singapore : Springer, 2006 27(2016), 6 vom: 12. Okt. (DE-627)513219439 (DE-600)2238719-5 2210-3147 nnns volume:27 year:2016 number:6 day:12 month:10 https://dx.doi.org/10.1007/s41365-016-0136-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 27 2016 6 12 10 |
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10.1007/s41365-016-0136-0 doi (DE-627)SPR038194384 (SPR)s41365-016-0136-0-e DE-627 ger DE-627 rakwb eng Yang, Di verfasserin aut Readout electronics of a prototype spectrometer for measuring low-energy ions in solar wind plasma 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Chinese Nuclear Society, Science Press China and Springer Science+Business Media Singapore 2016 Abstract Readout electronics is developed for a prototype spectrometer for in situ measurement of low-energy ions of 30 eV/e–20 keV/e in the solar wind plasma. A low-noise preamplifier/discriminator (A111F) is employed for each channel to process the signal from micro-channel plate (MCP) detectors. A high-voltage (HV) supply solution based on a HV module and a HV optocoupler is adopted to generate a fast sweeping HV and a fixed HV. Due to limitation of telemetry bandwidth in space communication, an algorithm is implemented in an FPGA (field programmable gate array) to compress the raw data. Test results show that the electronics achieves a 1 MHz event rate and a large input dynamic range of 95 pC. A slew rate of 0.8 V/μs and an integral nonlinearity of 0.7-LSB for the sweeping HV, and a precision of less than 0.8 % for the fixed HV are obtained. A vacuum beam test shows an energy resolution of 12 ± 0.7 % full width at half maximum (FWHM) is achieved, and noise counts are less than 10/sec, indicating that the performance meets the physical requirement. Solar wind plasma (dpeaa)DE-He213 Energy spectrometer (dpeaa)DE-He213 Readout electronics (dpeaa)DE-He213 A111F (dpeaa)DE-He213 Data compression (dpeaa)DE-He213 Cao, Zhe aut Qin, Xi aut Hao, Xin-Jun aut Liu, Shu-Bin aut Feng, Chang-Qing aut An, Qi aut Enthalten in Nuclear science and techniques Singapore : Springer, 2006 27(2016), 6 vom: 12. Okt. (DE-627)513219439 (DE-600)2238719-5 2210-3147 nnns volume:27 year:2016 number:6 day:12 month:10 https://dx.doi.org/10.1007/s41365-016-0136-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 27 2016 6 12 10 |
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Yang, Di @@aut@@ Cao, Zhe @@aut@@ Qin, Xi @@aut@@ Hao, Xin-Jun @@aut@@ Liu, Shu-Bin @@aut@@ Feng, Chang-Qing @@aut@@ An, Qi @@aut@@ |
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Yang, Di |
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Yang, Di misc Solar wind plasma misc Energy spectrometer misc Readout electronics misc A111F misc Data compression Readout electronics of a prototype spectrometer for measuring low-energy ions in solar wind plasma |
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Readout electronics of a prototype spectrometer for measuring low-energy ions in solar wind plasma Solar wind plasma (dpeaa)DE-He213 Energy spectrometer (dpeaa)DE-He213 Readout electronics (dpeaa)DE-He213 A111F (dpeaa)DE-He213 Data compression (dpeaa)DE-He213 |
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misc Solar wind plasma misc Energy spectrometer misc Readout electronics misc A111F misc Data compression |
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Readout electronics of a prototype spectrometer for measuring low-energy ions in solar wind plasma |
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Readout electronics of a prototype spectrometer for measuring low-energy ions in solar wind plasma |
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Yang, Di |
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Nuclear science and techniques |
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Yang, Di Cao, Zhe Qin, Xi Hao, Xin-Jun Liu, Shu-Bin Feng, Chang-Qing An, Qi |
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10.1007/s41365-016-0136-0 |
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readout electronics of a prototype spectrometer for measuring low-energy ions in solar wind plasma |
| title_auth |
Readout electronics of a prototype spectrometer for measuring low-energy ions in solar wind plasma |
| abstract |
Abstract Readout electronics is developed for a prototype spectrometer for in situ measurement of low-energy ions of 30 eV/e–20 keV/e in the solar wind plasma. A low-noise preamplifier/discriminator (A111F) is employed for each channel to process the signal from micro-channel plate (MCP) detectors. A high-voltage (HV) supply solution based on a HV module and a HV optocoupler is adopted to generate a fast sweeping HV and a fixed HV. Due to limitation of telemetry bandwidth in space communication, an algorithm is implemented in an FPGA (field programmable gate array) to compress the raw data. Test results show that the electronics achieves a 1 MHz event rate and a large input dynamic range of 95 pC. A slew rate of 0.8 V/μs and an integral nonlinearity of 0.7-LSB for the sweeping HV, and a precision of less than 0.8 % for the fixed HV are obtained. A vacuum beam test shows an energy resolution of 12 ± 0.7 % full width at half maximum (FWHM) is achieved, and noise counts are less than 10/sec, indicating that the performance meets the physical requirement. © Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Chinese Nuclear Society, Science Press China and Springer Science+Business Media Singapore 2016 |
| abstractGer |
Abstract Readout electronics is developed for a prototype spectrometer for in situ measurement of low-energy ions of 30 eV/e–20 keV/e in the solar wind plasma. A low-noise preamplifier/discriminator (A111F) is employed for each channel to process the signal from micro-channel plate (MCP) detectors. A high-voltage (HV) supply solution based on a HV module and a HV optocoupler is adopted to generate a fast sweeping HV and a fixed HV. Due to limitation of telemetry bandwidth in space communication, an algorithm is implemented in an FPGA (field programmable gate array) to compress the raw data. Test results show that the electronics achieves a 1 MHz event rate and a large input dynamic range of 95 pC. A slew rate of 0.8 V/μs and an integral nonlinearity of 0.7-LSB for the sweeping HV, and a precision of less than 0.8 % for the fixed HV are obtained. A vacuum beam test shows an energy resolution of 12 ± 0.7 % full width at half maximum (FWHM) is achieved, and noise counts are less than 10/sec, indicating that the performance meets the physical requirement. © Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Chinese Nuclear Society, Science Press China and Springer Science+Business Media Singapore 2016 |
| abstract_unstemmed |
Abstract Readout electronics is developed for a prototype spectrometer for in situ measurement of low-energy ions of 30 eV/e–20 keV/e in the solar wind plasma. A low-noise preamplifier/discriminator (A111F) is employed for each channel to process the signal from micro-channel plate (MCP) detectors. A high-voltage (HV) supply solution based on a HV module and a HV optocoupler is adopted to generate a fast sweeping HV and a fixed HV. Due to limitation of telemetry bandwidth in space communication, an algorithm is implemented in an FPGA (field programmable gate array) to compress the raw data. Test results show that the electronics achieves a 1 MHz event rate and a large input dynamic range of 95 pC. A slew rate of 0.8 V/μs and an integral nonlinearity of 0.7-LSB for the sweeping HV, and a precision of less than 0.8 % for the fixed HV are obtained. A vacuum beam test shows an energy resolution of 12 ± 0.7 % full width at half maximum (FWHM) is achieved, and noise counts are less than 10/sec, indicating that the performance meets the physical requirement. © Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Chinese Nuclear Society, Science Press China and Springer Science+Business Media Singapore 2016 |
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Readout electronics of a prototype spectrometer for measuring low-energy ions in solar wind plasma |
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https://dx.doi.org/10.1007/s41365-016-0136-0 |
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Cao, Zhe Qin, Xi Hao, Xin-Jun Liu, Shu-Bin Feng, Chang-Qing An, Qi |
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Cao, Zhe Qin, Xi Hao, Xin-Jun Liu, Shu-Bin Feng, Chang-Qing An, Qi |
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10.1007/s41365-016-0136-0 |
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2024-07-03T16:41:39.350Z |
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