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Testing the glass bars from Desert Glass Works. The green light scattered at multiple points along the surface of the bar, giving it this glow.
Ryan's waveform plotter in JupyterLab workspace for the Centauri Stars. You can see everyone practicing their data analysis in their own waveform plotter copies.
Saturday and Sunday are the last two days of beam time, so we are up against the clock to get useful data and analyze it before our final presentation on Monday. We'll be working all weekend, but can take different shifts and fit in breaks for everyone. Today started with our morning check-in as usual. Once we were at the test beam, Vibeke gave a data analysis tutorial to the rest of our team. Now everyone knows how to access new data runs through the JupyterLab system, plot waveforms, and identify signals. Some support scientists (grad students and post docs) volunteered their weekend time to help us create visuals that quantify and show the SiPM pulses, and they assisted with signal to noise waveform analysis. Ivo (looking sharp in his purple parachute jacket) was particularly helpful in guiding us to make the heat maps of SiPM signals. Ivo has been a huge asset for our team in discussing and analyzing our data, and troubleshooting our system.
We had 3 glass bars donated to us for our project by Desert Glass Works in Colorado Springs, but they got held up in customs, misplaced in a warehouse, then delivered to an office without any notice. We finally found them this morning and got to test them for our detector. They don't have the level of polish and flatness necessary to determine the angle of Cherenkov radiation, but they would work to detect Cherenkov light. When we're done, we will use them to create a display of our project back at Centaurus.
We took several more data runs throughout the day, but we had some midday excitement when the whole beam and accelerator stopped working. The "Machine State" on the display screen just said "Problems." However, the "Problems" were quickly remedied and we were back online. Jack, Liam, and Ocean took turns as beam coordinator to optimize the angle between the particle beam and the glass radiator bar such that we would get the best signal while still having a predicted distribution of light that could help us backtrack to a Cherenkov angle. Our SiPM's have still not been perfectly reliable, so we continue to have gaps in data. We are getting some projection patterns that are consistent with what we would expect to see.
Many of us worked on assignments from classes back home during down time, but we also got some rest/recharge/wellness breaks. At 6:30 PM, we gathered at the DESY entrance to take a bus to the nearest shopping mall. We had a variety of food for dinner, provided by Antoine as always. We got smashburgers, kabab, Indian food, and Korean food. We appreciated the comfort food at the end of a long day of work.
Heat map of maximum signals to active SiPM channels
Photon Heat Map on Sensors
Broadcom Silicon Photomultiplier AFBR-S4N44P014M: our single-channel SiPM that is used for ultra-sensitive precision measurements of single photons.
Signal pulses on a silicon photomultiplier channel
Visualizing signal and noise on channel 7
Final labeled setup of our experiment
Relaxing and socializing after dinner at the mall
Stairs down to the test beam area, past the high voltage lines
Entering the HERA particle accelerator tunnel
Quadrupole magnets for focusing or defocusing the electron beam in the tunnel
This is an old photomulitplier tube (not like our tiny 4mm x 4mm SiPM's)
After our regular morning meeting checking in with the teams at ELSA and CERN, we split into 2 groups. Some of us worked in the test beam area, and the others went on a visit with Sven to an underground particle accelerator tunnel. This is from the HERA (Hadron Electron Ring Accelerator) project, and we also got some time up close with HERA's old detectors. The groups traded off with each other so that everyone would have a chance to see HERA and get some beam time before lunch.
We collected more test beam data with a range of positions of our silicon photomultiplier array using the vertical and horizontal translation stages. We have tried a few different beam energies, beam rates, and offset angles of our glass bar to the particle beam. We also have been working extensively on analyzing the data we already have, learning how to use the waveform plotter in JupyterLab through the DESY data network. We've made histograms of average maximum SiPM signal for each channel so that we can tell which photomultipliers are still working, and which ones have on average a larger signal. Some photomultipliers have stopped working, but then sometimes they start working again. It is still a mystery why there is irregular reliability of some of the photomultipliers.
The tunnel for HERA was so cool! We got to take the classic particle accelerator tunnel photos, see some impressive magnetic containment and focusing systems, and learn about liquid helium cooling systems and superconductors. We saw a spark chamber for detecting cosmic rays, an old wire chamber, and the biggest magnet I've ever seen (even bigger than the Big Red Magnet in our test beam area). We also saw a RICH (Ring Imaging Cherenkov) detector, which was massive. It would be cool to design a compact RICH detector, but that is harder than our compact DIRC (Detection of Internally Reflected Cherenkov radiation) detector we've been working on. While we have gone over the basics for how a particle accelerator works multiple times with experts from CERN, ELSA, and DESY, it is much more meaningful to see it all in person and understand the scale and dimensions first hand. We also got to see some of the machinery used to quickly assemble the beam components in the tunnel.
After lunch, some of us went out to Hamburg for shopping or sightseeing, some played soccer, and some worked or rested until we all met near the Elbphilharmonie at 6:30 PM. Antoine planned a surprise outing to the Miniatur Wunderland. There are miniature models of cities, landscapes, and scenes from around the world, including a mini airport, a mini car race through Monaco with camera tracking, a mini amusement park, and so many more. It was quite impressive. We got home late (almost midnight), but we had a great day.
This big, blue-gray structure shields radiation (BONUS: find the golden idol from Raiders of the Lost Ark)
A spark chamber for detecting cosmic ray showers - look very carefully for the zaps; even though this is 6 floors below ground, we still get cosmic radiation
Ryan and Vibeke take in the scale of Miniatur Wunderland's Swiss Alps
The real Elbphilharmonie
Vibeke and Ocean happened upon this sweet ride in the streets of Hamburg
Miniatur Wunderland's Elbphilharmonie
Minatur Wunderland rocket launch (I'm guessing it's meant to be Cape Canavral, FL ?)
The Millenium Falcon takes off from the Hamburg Airport at Miniatur Wunderland
Rio Carnaval Samba Parade in the Miniatur Wunderland
The Monaco Grand Prix roars by and Miniatur Wunderland
Getting ready for more test beam runs
The Centauri Stars show Michael Sullivan from the US Department of State our experiment in the test beam area for our VIP Day
A double rainbow at the end of the day - view from the DESY Guest House courtyard.
Today was more test beam time and data collection, this time moving the translation stage for our light sensors up and down and farther back to try to find a full picture of the light projection pattern. The difficult part is that the signal drops significantly when going farther away from the end of the glass bar, so at some point it will be lost in the noise. Vibeke created a plot of distance vs. average signal maximum in volts to evaluate how much light intensity we lose as we get farther away. We learned about background signal and waveform baselines so that we could better extract the signal.
We also presented for our VIP Sponsor's Day, along with the other 4 teams, meeting diplomats from around the world, sponsors of Beamline for Schools, and directors of the various facilities. We presented our work up until now during a live in-person and Zoom call event. Thanks to everyone who tuned in and supported us from the US!
We had a barbecue banquet reception afterwards with excellent roasted vegetables, cheese, breads, and meats and time to meet with all of the VIP's. There was a massive downpour right at the start of the barbecue, so tables were moved inside to keep everyone dry, and the grill was under a tent. This weather allowed for a beautiful double rainbow on the way back to our guest rooms for the evening.
Green light bouncing inside our glass bar
Our setup then...
Our setup now.
Dylan, Vibeke, and Liam run the test beam
Ryan shares his simulation results, with Vibeke processing our first real test beam data
Look at the bottom blue line on the oscilloscope reading during this video - those pulses are actually light on a silicon photomultiplier during a test beam run.
Today we had many beam tests and collected a significant amount of data. While confirming our detection of Cherenkov radiation with an oscilliscope, we switched a majority of our working photosensor channels to attach to our digitizer so that we can read out more sensors simultaneously. Our silicon photomultipliers are down to 60% that are actually functioning, so we will have some gaps in our data but can still get an overall picture. Ryan updated his simulation to predict the light pattern projected out at the end of our glass bar, and Vibeke worked extensively on data analysis.
Achtung – Strahlbetrieb an Strahl 21 wird gestartet. Attention - Beam 21 is going to be switched on. Getting ready for test beam runs.
Signals on our central silicon photomultiplier during a test beam
One example of Ryan's simulated light projection out the end of the glass bar
Natalie and Dylan working with Marcel and another scientist to test our SiPMs and get the go-ahead to turn on the beam.
Ryan has been working relentlessly to provide our team with a simulation of what results we theoretically expect to get once our setup is up and running. He built it from scratch in Python.
Today was a busy but fruitful day of troubleshooting, productive struggle, and at long last some beam time!
In the morning, the group tackled several tasks. Some of our team worked to prepare the aluminum tube with new 3D printed supports and foam so that we can safely insert the fused Silica glass bar. Ryan continued working on the simulation. Vibeke and others continued to work to understand the data acquisition system.
After lunch, we had a very educational discussion with Antoine around communication and making sure that all members have at least a basic understanding of what is going on with all the different moving pieces of our experiment. Then we worked to ensure that we could read a trigger from our PCB board. All of our team made accounts and connected to DESY's remote data base. We learned of an issue with our PCB where the high resistance resistors were resulting in no output signal from our SiPMs, and so a kind scientist quickly burned those off for us. We delicately inserted the glass bar into our aluminium tube, set the tube into the blackbox, and were finally able to turn the beam on. Unfortunately, we did not see anything on the oscilliscope. Tomorrow we have the big task of figuring out how to make our SiPMs work, or if not, change our set up and use SiPMs that DESY can provide. Fingers crossed!
An extremely kind scientist volunteering his time to help us burn off all of the unecessary resistors from our PCB. Ryan and Mr. E watch intently.
Liam, Dylan, and Natalie quickly working to reconnect our PCB so that we can turn on the beam. BEAM TIME!
A spike on the oscilloscope, showing that an SiPM has measured a photon. *Sigh of relief*
Walking to XFEL visitor center through the XFEL campus
Learning about how XFEL works
Our tour guide, Lars, sharing about Small Quantum Systems
This morning, we took the bus and walked through a lovely park to visit European XFEL, the X-ray Free-Electron Laser facility. They partner with DESY to create X-ray lasers, which can explore the structure of matter at incredibly small scales, as well as dynamics of biological molecules.
There are several different projects happening at XFEL, in fields varying from quantum science to high pressure and temperature environments, and they will even begin to research fusion. We were there until lunch time, when we returned to DESY (after finding some delicious wild blackberries growing along the fence). Today was the first rainy day, with more to come.
Following lunch, we returned to work on various aspects of the experiment. We prepared our black box for the experiment, verified the control system for the translation stages, worked on the simulation, re-designed the holding system for the glass bar within the aluminum tube portion of the black box, connected all the cables from the SiPM board to our digitizer in the black box, connected the power supply, and attempted our first round of data collection of background noise with just the black box and no light signal.
We discovered our power supply, when set to 40 volts then turned on and connected to our circuit board, dropped voltage to about 15-16 volts. We'll begin tomorrow morning by trouble-shooting the power supply/circuit board setup, but we might know what the problem is already!
In the meantime, the new 3D prints are going overnight (this is a 13-hour job). We've definitely made a habit of re-printing our designs at the end of every day. But we know these ones will be the best so far to effectively hold our glass bar.
Descending into the main hall at XCEL
Ocean and Vibeke look into a clean room area
Testing in progress when the lights are on - can't enter!
XFEL Gollum (Samweis to the right, spelled the German way)
XFEL test area with marble floors we can't walk on
Dylan, Noah, Vibeke attaching cables to the board back at DESY
Antoine making sure the digitizer is properly connected
Ross, Ryan, Jack, Dylan, Isaac, Liam, and Ocean take in the view of the Elbe from Altona Balkon
Boats passing on the Elbe
All of us on a boat on the Elbe
Today is our outing day! We went into the city of Hamburg, with Antoine as our wonderful tour guide, and Oliver accompanied us. We also slept in for the first time all week, leaving at 10:30 AM for a bus to Altona, south of DESY.
We saw beautiful views of the water while waiting for a water taxi ride towards the Elbphilharmonie Hamburg, where we got to do a 360-tour of the upper terrace with views across the water and into the city.
We then walked through that part of town towards a modern shopping mall, where Antoine bought us all lunch at a variety of food court restaurants (kebab, Indian food, burgers, etc.). Our friend Henry from the UK team made a Starbucks stop for the Unicorn drink (only available for a very limited time).
Afterwards, we walked north to get to the St. Nikolai Memorial, where only the tower and a few walls remain from the church that was there until Operation Gomorrah in August 1943, when a large portion of Hamburg was destroyed during air raids. We went midway up the tower, and some of us visited the museum while others rested on a low wall in the courtyard that was once the nave of the church. The memorial is meant to educate visitors on the causes and consequences of WWII, and it serves as an anti-war monument and a place of remembrance.
Next, we walked towards City Hall, and had free time in small groups around that central part of town. Ms. Becker walked around the small lake with a central fountain, swans, and beautiful views of Hamburg.
Then we gathered back together in front of City Hall, ordered food, and took the train and bus back to DESY for a pizza party in the cafeteria with just the Beamline for Schools groups. Some of us relaxed outside on the patio while others played pool or darts, basketball, or played piano and sang.
An old U-boat submarine along the shores of the Elbe
This ferry has an airplane, it's a Lufthansa ferry. Elbphilharmonie is on the right, the building that looks like waves.
Mr. E, Jack, Dylan, and Levi enjoy the view from the Elbphilharmonie terrace looking towards the St. Nikolai tower
The whole DESY crew pproaching the St. Nikolai tower
Isaac, Henry, Merlina, and Amy at the fountain across from St. Nikolai. Ryan photographs the tower in the background.
Ms. Becker saw a rainbow in the fountain as some canoes passed by during her walk through Hamburg.
Swan couple in Hamburg
Sunday evening stroll beneath the paper lanterns
Trees along the shoreline
Hamburg City Hall (Hamburger Rathaus)
Attached motorized translation stages for vertical and horizontal movement of our detector
Digitizer with cables on top of the computer for test runs of our data acquisition system
One of the tunnels in Building 1 leading towards the test beam area
Today was a long work day at the test beam area. We started by organizing a list of all of the different parts of the experiment we needed to work on, who would do what, and how long we expected it to take. We had so much to do that we were all busy throughout the day without very many breaks, other than for food.
We got help from Oliver in soldering a super tiny resistor to our circuit board (it is about the size of a small grain of salt). Ryan, Liam, Jack, and Ocean took care of several new 3D prints for stands, holders, and mounts for our various pieces of equipment.
We switched over to a new dark box design with a much, much larger box to allow us to remotely control the position of our detector using 2 motorized translation stages attached together, which were too big to fit in our original dark box for the detector. Instead of our Team USA-themed small ammunition can that was painted inside with "Musou Black"), we now have a giant plastic storage bin with an even bigger, thick black blanket to drape over the whole thing. We'll cut a small, round hole in the back for cables and a larger, square hole in the front for the aluminum square tube that is the black box around our glass radiator bar.
Natalie ran some introductory tests on the SiPM (Silicon Photomultiplier) circuit board with the power supply, and figured out how to correct a ground wiring issue.
Noah, Levi, and Merlina investigated the cable system with a sample circuit board and made good use of a label maker to number all of the cables that would be connected to the back of our circuit board and to our digitizer to transmit the data from the SiPMs. Jack figured out how the circuit board would need to be spaced from the translation stages and how to arrange the cables so that everything would fit. Ryan has been an MVP, consulting on most aspects of the project and helping out in multiple ways.
Vibeke and Dylan learned how to work with data readout to the computer using the digitizer and how to set up the triggering system.
Ryan continued working on his own python code to model the transmission of the light inside our glass bar, and how it would project out the end.
We also saw the UK team making significant progress on their experiment, so we will hopefully both be ready to test with the beam around the same time. Below are some before/after pictures of their setup. We'll do some before/after of ours once everything is ready!
It gets very hot and stuffy inside Hut 23, so the tunnels from Building 1 are a nice place to cool down, and they provide a quick short cut when going from the cafeteria or meeting room to the test beam hall, useful in the heat or in the rain.
The cafeteria doesn't serve dinner on weekends, so Antoine ordered us all our preferred meals from burger and pizza takeout around 7:30 PM, and we had a picnic dinner outside the beamline while putting one last 3D print job in. We can't emphasize enough how supportive and phenomenal Antoine is for this project and our experience here.
Initial computer simulation rendering of light in glass
Our metal stage set on a rotating platform, set on a mechanical lift
The UK team's setup now
The UK team's OLD setup (before making improvements)
Demonstrating our setup and getting materials ready
De-noising the power supply in the test beam hut 23
We started again at 9:00 AM with a quick meeting checking in with our 2 teams at DESY (USA + UK), and the team at ELSA (Bangladesh). The UK team has a very cool experiment using old cell phones as a beam telescope, and their set-up and adjustments are looking good. The Bangladeshi team is testing a new material as a scintillator, which is something that lights up when hit with charged particles. They have already had a beam test with a great image as of this morning! It's also Ms. Becker's birthday. She was surprised with flowers, fresh strawberries, a card from the team, and the happy birthday song.
We got to work right away at the test beam to move things along with our machinery, circuit board, power supply, and data acquisition system. Antoine, Oliver, and Marcel were all incredibly helpful in troubleshooting whatever issues came up throughout the day. Antoine is putting in a superhuman effort across our 2 teams - he is truly excellent at this work, and we all appreciate him greatly.
The time flew by, but by 7 PM we were all feeling the impact of working long hours.
After dinner, some of us went to bed early, but a group of us from both teams played basketball together at the court near our guest house.
A retired detector (ARGUS) on display at DESY across the road from the DESY Guest House
Liam, Vibeke, and Antoine working in Hut 21
Levi, Noah, and Dylan with the oscilloscope
Youssef and Isaac from the UK show Mr. E their system for the test beam
Evening basketball fun with both teams
Map of winning teams and host Beamlines
Beam telescope in the test beam area, with a trigger mechanism
At 9:00 AM, we had our first BL4S Whole Group Morning Zoom Meeting with CERN, ELSA, DESY, and all the support staff. Each of the 5 teams from the USA, UK, Türkiye, India, and Bangladesh presented their team and their experimental setup (see the Initial Centauri Stars Presentation Slides), with time for questions. We then received the technical presentations on the beamlines at all 3 facilities.
After lunch, we visited the test beam hall and had our first work session to prepare for our experiment and get to know the facilities.
We have been making many 3D prints for parts, testing different components, and getting help from the electronics experts at DESY to assemble the silicon photomultipliers on our circuit board. We also have been working with additional equipment, like a new power supply, oscilloscope, 16-channel digitizer for data acquisition, and connecting cables.
We have our whole dark box setup ready (and decorated), but we are considering building a bigger one that can house a remote motorized system to adjust the position of our detector.
We tested our custom manufactured quartz bar in the holders we designed, and made sure that light from a laser beam totally internally reflects along the bar.
We worked until about 6:00 PM, returned to the dining hall to play some pool/billiards and to throw darts with the UK team, then we were surprised with a welcome reception and dinner at 6:30 PM hosted by the scientists at DESY, including the assistant director.
The Big Red Magnet up close
Intro to the Test Beam 21 area
The Big Red Magnet
This is where the particle beam comes into the Test Beam 21 area
Custom manufactured quartz bar
Our Centauri Stars / Team USA dark box set-up, detector mount/rail system, + glass holders
Liquid Nitrogen ice cream at our cryogenic safety training
Most of the day was safety training, including fire safety and extinguisher practice with a real fire simulator, cybersecurity, cryogenics, and particle accelerator test beam safety. During cryogenic safety training, we also did several classic liquid nitrogen demonstrations, such as shattering roses, shrinking metal pieces and balloons, and making strawberry liquid nitrogen ice cream.
We also received our official Test Beam User badges and had a tour of the facilities.
After dinner, we got to go to the top of a new DESY building to view the solar eclipse from the roof. Jorge Andres Villa Velez, the BL4S coordinator from CERN, sent us eclipse glasses. Oliver Schaefer, another excellent support scientist at DESY, set up a projection telescope for everyone to view the eclipse more clearly.
Some of us got to see some meteors once it was dark, due to the Perseids meteor shower. We successfully survived the first full day with many exciting moments!
Fire safety training
Jack's first run of saline water fire extinguisher practice
DESY Test Beam User Badge
Building 1 Entry Hall
3D model of DESY facilities, synchrotrons, and test beams
Eclipse photo from our BL4S group chat
Projection telescope of the solar eclipse with Antoine and Oliver
Merlina and Amy (from UK) + Hamburg view from DESY
Eclipse projection with clouds
Eclipse projection near maximum
Sunset eclipse from the rooftop
Exploring campus with the UK team
Looking at the map of DESY
We travelled all day, arriving in Hamburg mid-afternoon and taking public transportation to DESY with our amazing host and coordinator research scientist, Antoine Laudrain. We met up with the team from the UK - they are from Liverpool and their experiment involves using cell phone cameras as particle detectors. We got settled in the DESY Guest House, had dinner in the cafeteria, explored the campus, and prepared for the next day of safety training and getting our official badges.
View from DESY Guest House
Ocean and Noah in flight
Local cola drink in the cafeteria
Arrival in the Hamburg airport - jetlagged but happy!
Centauri Stars BL4S Team
We leave for Hamburg, Germany today on Lufthansa. We have carefully packed all of our key equipment pieces for our DIRC (Detection of Internally Reflected Cherenkov radiation) detector in our luggage. This includes a very fragile $1000 custom manufactured quartz bar (50 cm x 1 cm x 1 cm), our custom printed circuit boards for data collection, a dark box, and some extra glass bars for demonstration (and possibly additional experiments if we get time). We have prepared a presentation for when we arrive and meet another team from the UK. Many thanks go to everyone who helped us get our experiment ready: Jochen Schwiening, Antoine Laudrain, Marcel Stanitzki, Oliver Shaefer, John Cumalat and the CU Boulder Physics Department, Luverre Glass, Desert Glass Works, JLC PCB, Mouser Electronics and Broadcom, David Summers and the group at LASP, and all of our donors and educators. We are representing the US (and all the Americas) for this opportunity... no pressure!