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 |