The time-space structure of pulses in Cherenkov light detectors
Here the results of calculations of pulses in Cherenkov light detectors for the Yakutsk array are presented. As long as the Vavilov-Cherenkov light is used to calibrate signals in scintillation detectors at the Yakutsk array it is vital for these measurements to be precise. The validity of measureme...
| Main Authors: | , , , |
|---|---|
| Format: | Report |
| Language: | unknown |
| Published: |
arXiv
2009
|
| Subjects: | |
| Online Access: | https://dx.doi.org/10.48550/arxiv.0912.1487 https://arxiv.org/abs/0912.1487 |
| id |
ftdatacite:10.48550/arxiv.0912.1487 |
|---|---|
| record_format |
openpolar |
| spelling |
ftdatacite:10.48550/arxiv.0912.1487 2023-05-15T18:45:19+02:00 The time-space structure of pulses in Cherenkov light detectors Podgrudkov, D. A. Dedenko, L. G. Roganova, T. M. Fedorova, G. F. 2009 https://dx.doi.org/10.48550/arxiv.0912.1487 https://arxiv.org/abs/0912.1487 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences Preprint Article article CreativeWork 2009 ftdatacite https://doi.org/10.48550/arxiv.0912.1487 2022-04-01T14:49:41Z Here the results of calculations of pulses in Cherenkov light detectors for the Yakutsk array are presented. As long as the Vavilov-Cherenkov light is used to calibrate signals in scintillation detectors at the Yakutsk array it is vital for these measurements to be precise. The validity of measurements of the signal Q(400) used as the estimation parameter at the Yakutsk array has been confirmed. Our calculations show that the width of time pulses increases from nearly 50 ns at a distance of 100 m from the shower axis up to 700 ns at 1000 m. : 4 pages, 5 figures, 31 ICRC Report Yakutsk DataCite Metadata Store (German National Library of Science and Technology) Yakutsk |
| institution |
Open Polar |
| collection |
DataCite Metadata Store (German National Library of Science and Technology) |
| op_collection_id |
ftdatacite |
| language |
unknown |
| topic |
High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
| spellingShingle |
High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences Podgrudkov, D. A. Dedenko, L. G. Roganova, T. M. Fedorova, G. F. The time-space structure of pulses in Cherenkov light detectors |
| topic_facet |
High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
| description |
Here the results of calculations of pulses in Cherenkov light detectors for the Yakutsk array are presented. As long as the Vavilov-Cherenkov light is used to calibrate signals in scintillation detectors at the Yakutsk array it is vital for these measurements to be precise. The validity of measurements of the signal Q(400) used as the estimation parameter at the Yakutsk array has been confirmed. Our calculations show that the width of time pulses increases from nearly 50 ns at a distance of 100 m from the shower axis up to 700 ns at 1000 m. : 4 pages, 5 figures, 31 ICRC |
| format |
Report |
| author |
Podgrudkov, D. A. Dedenko, L. G. Roganova, T. M. Fedorova, G. F. |
| author_facet |
Podgrudkov, D. A. Dedenko, L. G. Roganova, T. M. Fedorova, G. F. |
| author_sort |
Podgrudkov, D. A. |
| title |
The time-space structure of pulses in Cherenkov light detectors |
| title_short |
The time-space structure of pulses in Cherenkov light detectors |
| title_full |
The time-space structure of pulses in Cherenkov light detectors |
| title_fullStr |
The time-space structure of pulses in Cherenkov light detectors |
| title_full_unstemmed |
The time-space structure of pulses in Cherenkov light detectors |
| title_sort |
time-space structure of pulses in cherenkov light detectors |
| publisher |
arXiv |
| publishDate |
2009 |
| url |
https://dx.doi.org/10.48550/arxiv.0912.1487 https://arxiv.org/abs/0912.1487 |
| geographic |
Yakutsk |
| geographic_facet |
Yakutsk |
| genre |
Yakutsk |
| genre_facet |
Yakutsk |
| op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
| op_doi |
https://doi.org/10.48550/arxiv.0912.1487 |
| _version_ |
1766236360788672512 |