6 December, 2002
6 December, 2002
Bai & I went out to the SPASE (South Pole Air Shower Experiment) shack and put in a full day's work. SPASE is designed to detect muons from above, and consists of about 4 acres of 100 or so widely spaced scintillator detectors. When a charged parcticle enters the Earth's atmosphere, it interacts, usually with a nitrogen atom, and creates a cascade of millions or billions of secondary parcticles. Many of these secondaries are muons, a sort of heavy electron with a very finite lifetime. The more energy the original parcticle had, the more secondaries are created. You need a big detector area to image extensive air showers, and that's what SPASE is.
That's also what WALTA (Washington Area Large-Scale Time Coincidence Array) is. WALTA's the cosmic ray experiment I'm involved with in collaboration with many Seattle area high schools and the University of Washington. Our WALTA array will cover a much larger area than SPASE but with many fewer detectors. The ultimate difference is in the energies of the primary parcticles each can detect.
Part of SPASE is an experimental ice tank. Muons entering the dense ice of the tank interact with water molecules and create faint Cerenkov light. This light can be detected by PMTs (photomultiplier tubes) which sit frozen in the top of the ice. The ICECUBE neutrino detector will incorporate many surface tanks like this one in a surface array called ICETOP as a way to get information about the muons from the atmosphere entering the ICECUBE neutrino detector. Ultimately, ICECUBE is not interested in these atmospheric muons. Rather, they represent noise in the data, and ICETOP will provide a sort of data filter to subtract atmospheric muons from the data.
The tank was finished last summer, and sealed up, and there's lots of questions. To answer them, we have to dig out the tank. The South Pole is flatter than Kansas. Anything that dares stick out above the horizon quickly aquires drifting show. That's what all the bulldozers are up to: just moving snow downwind of the station. The tank? Last year, the top was at snow level. This year, a meter and a half under.
Fortunately for me, during the long holdover at McMurdo, Bai dug most of it out. We finished the job (this snow is easy to dig, sort of like styrofoam), and cut the tyvek covering and the black light-tight shroud, and opened up the tank. The tank didn't freeze very clear, and some new cracks appeared around one the PMTs. Anything less than clear ice ultimately changes, and not for the better, the ability of light to reach the PMT. But a crack that was present at freezing last year had nearly disappeared. This is surprisingly dynamic process in this tank of ice. We repaired a couple of cables, and drilled some very narrow deep holes to install some temperature sensors (Bai is curious about the winter temperatures of the PMTs, which are only rated to -55 C, but of course the air gets much colder here) At the end of drilling, Bang! A new pressure crack appeared, 30 degrees off horizontal, not reaching the surface. Ice is weird. While we were standing around, it gave a couple of low moans.
Note: untangling extension cords at - 30 C is not easy. The plastic insulation makes the wire like spaghetti: dry spaghetti, that is.
We also ran some experiments with my portable detector (more on that in a future journal)
AMANDA meeting after dinner. I was so tired. Bob Morse from the University of Wisconsin is leaving tomorrow, and wanted to do a go around and get tasks lined up.
Contact the TEA in the field at .
If you cannot connect through your browser, copy the TEA's e-mail address in the "To:" line of your favorite e-mail package.