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http://hdl.handle.net/2248/2467
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DC Field | Value | Language |
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dc.contributor.author | Upadhya, S. S | - |
dc.contributor.author | Acharya, B. S | - |
dc.contributor.author | Bhat, P. N | - |
dc.contributor.author | Chitnis, V. R | - |
dc.contributor.author | D'Souza, A. I | - |
dc.contributor.author | Francis, P. J | - |
dc.contributor.author | Gothe, K. S | - |
dc.contributor.author | Joshi, S. R | - |
dc.contributor.author | Majumdar, P | - |
dc.contributor.author | Manogaran, M | - |
dc.contributor.author | Nagesh, B. K | - |
dc.contributor.author | Pose, M. S | - |
dc.contributor.author | Purohit, P. N | - |
dc.contributor.author | Rahman, M. A | - |
dc.contributor.author | Rao, K. K | - |
dc.contributor.author | Rao, S. K | - |
dc.contributor.author | Sharma, S. K | - |
dc.contributor.author | Singh, B. B | - |
dc.contributor.author | Stanislaus, A. J | - |
dc.contributor.author | Sudersanan, P. V | - |
dc.contributor.author | Venkatesh Murthy, B. L | - |
dc.contributor.author | Vishwanath, P. R | - |
dc.date.accessioned | 2008-06-20T07:12:53Z | - |
dc.date.available | 2008-06-20T07:12:53Z | - |
dc.date.issued | 2002 | - |
dc.identifier.citation | BASI, Vol. 30, No. 1, pp. 411 - 416 | en |
dc.identifier.uri | http://hdl.handle.net/2248/2467 | - |
dc.description.abstract | Pachmarhi Array of Cverenkov Telescopes consists of 25 Telescopes distributed within an area of 8000m2. The array was designed to detect and process faint Cverenkov light flashes that lasts for a few nanoseconds, produced in the atmosphere by celestial VHE ?-rays or cosmic rays. In this experiment, the arrival time and amplitude of fast tiny pulses have to be measured and recorded from each of 175 photo-tubes in a shortest possible time. In view of the complexity of the system, the entire array is divided into 4 sectors. A Distributed Data Acquisition System developed for the purpose consists of independent Sector Data Acquisition Systems and a Master Data Acquisition System. The distributed data acquisition and monitoring system are built using PC's which are networked through LAN. The entire software for DDAS was developed in-house in C language under LINUX environment. Also, most of the hardware barring a few fast digitization modules were designed and fabricated in-house. The design features, implementation strategy as well as the performance of the whole system are discussed. | en |
dc.format.extent | 601182 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Astronomical Society of India | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/2002BASI...30..411U | en |
dc.subject | Distributed Data Acquisition System | en |
dc.subject | Atmospheric Cverenkov Technique | en |
dc.subject | Distributed Cverenkov Telescopes | en |
dc.subject | PACT | en |
dc.title | Distributed data acquisition system for Pachmarhi array of Cverenkov telescopes | en |
dc.type | Article | en |
Appears in Collections: | BASI Publications |
Files in This Item:
File | Description | Size | Format | |
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Upadhya.pdf | 587.09 kB | Adobe PDF | View/Open |
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