| ID |
Date |
Author |
Category |
Subject |
Text |
 |
|
3
|
Fri Jan 24 15:06:51 2025 |
Rodolfo | Detectors | Solar Blind PMTs | We (Danyal and Rodolfo) have installed two
"solar-blind" PMTs from "ET Enterprises"
Model 9423B to the "mirror chamber" at ESR |
|
|
21
|
Tue Feb 11 10:35:38 2025 |
Danyal | Detectors | XUV detector | Volker Hannen kommt am 19.2 (Mittags) und
dann machen wir Abends den XUV Detektor bereid.
|
|
|
35
|
Thu Feb 27 09:38:04 2025 |
Konstantin & Danyal | Detectors | Laufzeit Messungen | Gestern Abend haben wir die Signal Laufzeiten
im gemessen:
|
|
|
37
|
Thu Feb 27 10:52:32 2025 |
Rodolfo | Detectors | Taking PMTs into operation | [B]PMT Nord[/B] the power supply (CH0) is
giving an alarm already by an applied voltage
of -1707 V (operation voltage is -2450 V). |
|
|
44
|
Fri Feb 28 00:19:04 2025 |
Konstantin, Sebastian | Detectors | PMT power supply | We checked the PMT signal inside the cave
by using the local HV power supply. If one
needs to repeat the measurement at another |
|
|
51
|
Fri Feb 28 15:30:41 2025 |
Tamina, Rodolfo | Detectors | Fast PD Nord West | We had an issue with the PD NW. The signal
after the Rate Divider was not OK.
|
|
|
56
|
Fri Feb 28 19:33:03 2025 |
Volker | Detectors | Laser background | We measured the laser background rate in the
XUV detector.
The voltages applied were +300V at the MCP |
|
|
69
|
Sat Mar 1 13:34:30 2025 |
Tamina, Florian, Konstantin, Volker | Detectors | Erhoehter Untergrund XUV-Detektor | Erhoehter Hintergrund bei XUV-Detektor durch
das weiße Papier, welches zur Beobachtung
des Strahls über die Kamera verwendet wird. |
|
|
76
|
Sun Mar 2 03:23:46 2025 |
Danyal | Detectors | Schottky Bild 27_02_2025 | |
|
|
77
|
Sun Mar 2 03:24:42 2025 |
Danyal | Detectors | Schottky Bild 01_03_2025 | |
|
|
78
|
Sun Mar 2 03:25:23 2025 |
Danyal | Detectors | Schottky Bild 02_03_2025 | |
|
|
95
|
Mon Mar 3 16:35:43 2025 |
Danyal | Detectors | Schottky Bild 03.03.2025 - 2nd ion beam energy | The new Schottky frequency (137th observation
harmonic!) is at 244.62875 MHz |
|
|
100
|
Tue Mar 4 07:07:11 2025 |
Sebastian, Benedikt, Denise | Detectors | XUV Detektor Laseruntergrund | Laseruntergrund XUV Detektor krzpton0554.lmd
Schritte:
|
|
|
5
|
Mon Jan 27 10:59:22 2025 |
Sebastian | DAQ | RedPitaya | [B]Hostname: ext-91000370132.gsi.de
IP-Adresse: 10.100.3.106
[/B]
|
|
|
8
|
Mon Jan 27 16:57:07 2025 |
Sebastian | DAQ | COM Ports Gentec Messkopf NW und SW Tower @ ESR | COM 5 Südwest Tower --> Laser EXIT
COM 6 Nordwest Tower --> Laser ENTRANCE
|
|
|
9
|
Tue Jan 28 14:13:54 2025 |
Benedikt & Sebastian TEAMWORK DIGGA | DAQ | RedPitaya Adresse | SCPI Server:
http://169.254.204.79/
|
|
|
13
|
Fri Jan 31 16:37:39 2025 |
Sebastian | DAQ | PD Nord | PD Nord an ESR Panel PMT Süd verkabelt |
|
|
30
|
Thu Feb 20 13:37:30 2025 |
Denise, Sebastian | DAQ | CFD Schwellen DAQ | Schwellen fuer den CFD N842 (lascool)
Lasereinstellungen dabei waren: 0.5 Skalenteile
-> 115ps Pulse
|
|
|
31
|
Thu Feb 20 13:51:04 2025 |
Denise, Sebatian | DAQ | DAQ Channelliste | [TABLE border="1"]
TDC Channels |
|-
|
|
|
32
|
Tue Feb 25 13:12:01 2025 |
Sebastian | DAQ | Teilungsverhältnis Ohmlabs HVS250 | Hochspannung Maßstabsfaktoren
-140 kV >>> 248514
|
|