Between May 29 and June 3rd we performed at 1500W noise characterization measurements of two ion pumps, which here we call simply small and big (info on the exact model will be added later on). These pumps consist of a large permanent magnet and the concern is the magnetic noise produced when this pump vibrates withing the static Earth field. A question concerning this noise and the consequent safe distance from the O5 test masses was asked by VAC reviewers. Answering it is the aim of this activities. Two activities have been performed.

1) Mapping. 
This activity was lead by Gilles who measured the ion pump static field on 3D grid of positions around each pump. For the small pump he used a 2D paper grid, for the big pump he used the plastic perforated frame that INGN-Genova made for the payload magnetic characterization and which the vacuum team moved from the CEB clean rooms to 1500W and reassambled in position. Gilles used his 3-axial magnetic probe, moved along the grid.

Attachments 1 and 2 show pictures of the setup of the big pump.

2) Shaking.
The big pump was excited using a little hammer tapping on the top flange of the ion pump, while one accelerometer (meggit) positioned vertically on top of the pump, and one 3-axial magnetic probe (Bartington MAG03_MC_100) were recording respectively the vibration of the pump body and the magnetic field. The magnetic probe was moved at a number of distances from the pump edge (approx 20cm to 120cm). Figure 3 is a sketch with coordinates of the measuring grid.
The attached txt file lists all measuring times and associated position of the magnetic probe. Attached are also spectrograms of the full measurement set. A magnetic field noise excess was measured in all locations. The last two show the probes spectrum when at approximately 30cm from the pump edge (mag probe position J13). The excess magnetic noise is evident and is also coherent with the vibration. 

Data frames have been saved in /data/procdata/envmon/MagneticNoise/ion_pump/shaking/saved_gwf/ion_pump_shaking_20260603_1464522918_8500.gwf

Analysis will follow.

ITF found DOWN in UPGRADING mode
No activities communicated to the control room

Today around 14:00 UTC, the WI PAM was moved back to its original reference position marked on the alignment plate (see 69208), since it was temporarily moved to allow the replacement of the damaged ZnSe viewport (see 69219).

ITF found DOWN in UPGRADING mode.
All times are UTC.
Below the list of activity comunicated to the control room:
09:03 - 09:56 Gouaty went in CEB Storage Room at 2nd floor, no access to any experimental areas required.
10:10 - 10:39 ZnSe WI viewport inspection (Pasqualetti, Nardecchia, Lumaca, Corubolo).
14:16 Zaza reported that NI payload has been cleaned and the ZnSe viewport has been replaced.

I have released a new version v10r3p4 of VirgoProcessMonitoring, that improves the browsing of the configuration file history. All instances have been restarted to use this new version.

The WI PAM activity has been finished yesterday, and the laser used for that activity was switched off yesterday (Tuesday) at 9:41 UTC as reported in https://logbook.virgo-gw.eu/virgo/?r=69194

ITF found DOWN in UPGRADING mode.
Planned activities communiucated to the control room.

• - Alignment GUI test Al9 (Boldrini, Fiori, Seder)
• - ENV: activitiy for NI instrumented baffle TF measurement (Tringali, Spinicelli, Fiori) in progress...
• - PAY: WI CP mount removal (Majorana, Naticchioni) in progress...
• - TCS: WI PAM actuator position reference and movement, plus viewport external inspection (Corubolo, Nardecchia, Lumaca, Pasqualetti, Gherardini, Francescon)
• - INF: Confined space safety training (Zaza, Gherardini, Fabozzi) in progress in CEB clean rooms
• - DAQ: 15:08 UTC - DMSserver restarted under request of Loic (for PCal flags)

This morning (09:00 - 10:00 LT), we went to the WI base tower to take reference pictures and measurements of the PAM actuator position (see Fig. 1).

Afterwards, we contacted the vacuum team to understand how much clearance is needed for the future replacement of the viewport. We agreed that moving the PAM actuator to a parking position on the base tower would provide sufficient clearance for the planned work. (see Fig. 2).

Finally, we took some pictures of the viewport to be replaced, as seen from the outside (Fig. 3). From the outside, the smaller viewport does not show the same signs of degradation as the viewport to be replaced. In particular, no sparkling/glittering features are visible, which would suggest dust or coating flaking, as observed on the damaged viewpor t (69192).

The OLTF of the BPL was measured after the bench was suspended. With the loop closed, a color noise was injected just before the control filter with a 0.01 V amplitude.

The measured UGF is 27 +/- 1 Hz, and the phase margin is 67 +/- 2 deg for all degree of freedom.

WE tested the newest version of the alignment GUI by sending commands to the WE mirror.

We tested the step movement, the ramp movement and the snail function, everything checks out.

We restored the original position of the mirror after the test.

For the record: the new steering mirror was clean when packed LAPP, and was still clean when unpacked at NE building. However, after the installation (of the mirror, tuning the angle, and of the sphere), there was some dust deposited on the mirror. Despite that we Paul and myself were wearing head cover, face mask, glasses, gloves and clean white garnment. Paul  has cleaned the mirror, with a tissue. 

This morning we went at NE to install the new steering mirror and the Rx sphere. The NE PCal is finally on again since 14H UTC. See the last figure with the VIM plot showing the relative calibration of the three power sensors of the NE Pcal.

Note that the responsivity (gain) of the Rx sphere has not been changed, and the gains of the Tx photodiodes neither. They are kept to be the same as during O4. If the NE PCal mis-calibration by 0.9% during O4 was due to optical losses in the M4 mirror, we were expecting that the power seen by Rx would increase by 0.9% compared to the other two photodiodes.

As a first remark, it seems that the relative calibration of Rx sphere and Tx_PD2 is similar than during O5, at better than 0.1%, while the relative calibration of Tx_PD1 has changed by ~0.5%. However, it is difficult to disantangle which sensor calibration has varied. A full recalibration based on WSV or a comparison with the NCal will be necessary to get useful information.

**********************************

Pictures 1 to 5 show the NE PCal Rx bench with:

• the new mirror (Thorlabs BB1-E03), put with aoi of about 20-25°. The reflectivity of this mirror has been characterized vs aoi at LAPP, as shown in the pre-last figure.
• the Rx sphere, moved to another position than before (since the aoi was 18-19° during O4)
• the temperature and humidity sensor moved behind the sphere.
• the sphere cap and a beam dump to be used during interventions on the bench, also put behind/on the side of the sphere.

Before enabling the power supply (Hameg29) to switch on the sphere, I have switch it off to recover the Ethernet monitoring. Unfortunately, after switch on, the channel 1 was dead (-12 V for the NE_Tx_PD photodiodes), no more providing any voltage. Note that this power supply for NE PCal has already been changed already twice because of similar issue, but on channel 3 instead.

In the afternoon, we have replaced the power supply Hameg29 by the Hameg32. Following an advice from Nicolas Letendre, we have added a cable to connect the grounds of the two pairs of channels: 1 and 2 (providing the -12 V and +12 V for the photodiodes) and 3 and 4 (providing the -15 V and +15 V for the sphere).

Another change, the maximum current setup is now the same as at WE : 0.3 A for channels 1 and 2, and 0.5 A for channels 3 and 4 (while until today it was 0.3 A for the four channels).

Figures 7 to 10  show the NE PCal electronics in the rack, with some vision of the cabling, and the power supply panel information when the laser is off and when the laser is set to 1.3 W. Figure 11 shows the id of the follower-circuit used for the NE Rx sphere (before the ADC).

Figure 6 shows the rear panel of the laser driver: I noticed that the leftmost fan is not working (and another fan seems to be a bit noisy). 

**********************************

Figures 12, 13, 14 and 15 are pictures of the WE Pcal rack, id of the WE Rx follower circuit, rear panel of the laser driver, with all fans working, and power supply panel with the laser set at 1.3 W.

**********************************

Figures 10 and 15 show the information about the setup of the NE and WE PCal Hameg power supplies, as well as the current values delivered when the laser is set to 1.3 W.

This afternoon, the status of the HWS-DET SLED and of the flip mirror installed to block the beam on EDB was checked.

It was found that the flip mirror could not be moved either via the VPM or using the local remote control.

The local remote control is normally powered by its dedicated power supply. However, since the corresponding power connection was difficult to identify, the discharged battery was  replaced with a new one.

After the battery replacement, the flip mirror became operational again and can now be controlled both remotely and locally.

The nominal power supply of the local remote control still needs to be identified and verified. For the time being, the system is operating correctly using the new battery.

The morning was dedicated to weekly maintenance started at 6:00UTC, here a list of the activity reported to the control room:

- standard vacuum refill from 6:00UTC to 10:00UTC (VAC Team);
- cleaning of central building (Ciardelli with external firm: from 6:00UTC to 10:00UTC);
- TCS: PAM actuator alignment on WI (#69194);
- CAL: north end PCAL switch on and checks;
- PAY: WI payload removal, in progress;
- ENV: Preparation activities for NI instrumented baffle TF measurement;

Air Conditioning
at around 13:30UTC I put back the detection area air conditioning system in "portata ridotta".

SBE
recovery of SDB2 vertical position with F1 step motors from 13:35UTC to 13:45UTC.

We are going to enter the NI tower (Irene, Piernicola, Maria).