| ID |
Date |
Author |
Category |
Subject |
Text |
 |
|
220
|
Fri Jul 2 20:33:44 2021 |
Yuri | Accelerator | 70Se setting with closed scrapers | We tune back to 70Se.
The scrapers stay closed at EEXDS2HA=0 mm,
EEXDS1HG=+5 mm
|
|
|
21
|
Fri May 7 01:07:27 2021 |
Helmut Weick | Analysis | maybe frequency ID | We think we see the frequency range of A/q=2.25
at 243.1 MHz.
This would correspond to L=108.2m and E=386.4 |
|
|
29
|
Fri May 7 03:51:56 2021 |
Shahab | Analysis | peak frequencies | a reference schematic of the peaks on 410
MHz (211th harmonic) and 245 MHz (126th harmonic) |
|
|
33
|
Fri May 7 06:53:56 2021 |
Akash, Liliana | Analysis | Some plots | Some plots of statistics up to now |
6x |
|
34
|
Fri May 7 07:02:33 2021 |
Guy Leckenby | Analysis | Online Monitoring Plots | In compliment to Liliana's plots, this is
the summed spectra I calculated from 0338
to 0507. |
|
|
36
|
Fri May 7 08:04:22 2021 |
Carlo Bruno, Desislava Kalaydjieva | Analysis | 7:00 - 14:00 analysis shift | (See
https://triumfoffice365-my.sharepoint.com/:w:/g/personal/dillmann_triumf_ca/Eb_LCp7yTx5Bgc8TO8khJmEBWeS-ycdPRnG02wQout-fgQ?rtime=3n3A3xMR2Ug
for remote shifter instructions. To be updated/corrected |
15x |
|
57
|
Fri May 7 20:28:32 2021 |
Kanika, Michael, Shahab | Analysis | Some pictures from the 410 detector | some pics. |
9x |
|
71
|
Sat May 8 08:16:08 2021 |
Akash, Nic, Jelena, Zsolt | Analysis | Night shift analysis | (Jelena has analysed these data files)
E143_245MHz_2021.05.08.00* (-s 5.0 -t 0.5) |
16x |
|
94
|
Sun May 9 05:38:29 2021 |
Iris, Chris G. | Analysis | offset btw png and tiq files from server? | This might have been answered before but I
looked at one png file and one tiq file from
the same run that was stored on the server. |
|
|
95
|
Sun May 9 05:54:11 2021 |
Ragan | Analysis | offset btw png and tiq files from server? | This is due to the 50% trigger setting in
the spectrum analyzers )) |
|
|
96
|
Sun May 9 05:56:29 2021 |
Iris, Chris G., Jacobus, Michele | Analysis | Not_52Mn spectra added up | Attached is a summed spectra of all files
taken between 1:17am and 1:59am (on the 245
MHz detector).
|
|
|
99
|
Sun May 9 06:34:37 2021 |
Iris, Chris G., Jacobus, Michele | Analysis | Runs 2-3am Not_Mn52 | Summed up runs on the 245 MHz detector between
2-3am (computer time).
One has -s 0.1 -t 8.0
|
|
|
101
|
Sun May 9 07:16:47 2021 |
Iris, Chris G., Jacobus, Michele | Analysis | Runs 3-4am Not_Mn52 | Summed up runs on the 245 MHz detector between
3-4am (computer time).
-s 0.1 -t 8.0 |
|
|
103
|
Sun May 9 12:53:01 2021 |
Desislava Kalaydjieva, Taka Yamaguchi | Analysis | Analysis, Morning shift, 9 May | For the whole morning shift there were no
significant changes in the spectra.
|
9x |
|
108
|
Sun May 9 17:39:21 2021 |
Guy | Analysis | Comparison between 72Ge: 7th 19h vs 8th 21h | Following Xiangcheng Chen's analysis, I analysed
11 ms time slices separated by 25 ms to see
the evolution of the potential isomer across |
|
|
112
|
Sun May 9 20:34:47 2021 |
Rui-Jiu Chen | Analysis | Comparison of frequency spectrum between 72Ge and other isotope | This some preliminary analysis results by
using NTCAP data. The IQ rate of NTCAP
is 20 MSamples/seconds. I analyzed data files |
6x |
|
126
|
Mon May 10 03:37:53 2021 |
Chris C | Analysis | isomer? or wishful thinking? | They are not easy to find, but we do occasionally
see what might be the isomer. |
|
|
127
|
Mon May 10 04:08:13 2021 |
Iris (Chris C., Jeff C.) | Analysis | Comparison between 72Ge: 10th 1-2am on 245 MHz | > Following Xiangcheng Chen's analysis, I
analysed 11 ms time slices separated by 25
ms to see the evolution of the potential |
|
|
128
|
Mon May 10 05:25:29 2021 |
Iris (Chris C., Jeff C.) | Analysis | Comparison between 72Ge: 10th 1-2am on 410 MHz | Same as before, but for 410 MHz detectors.
Peaks visible in the 3rd-5th slice.
|
8x |
|
130
|
Mon May 10 06:22:15 2021 |
Iris (Chris C., Jeff C.) | Analysis | Comparison between 72Ge: 10th 1-2am on 410 MHz | Same as before but for 4-5am on 410 MHz detector.
Peak visible.
|
9x |