As Dan mentioned, I had the pleasure of draining the water chiller last week. Few have worked with the water chiller and come away clean. The water pump has as much power as a small lawn mower and can move a gallon of water in 2 seconds up 100 feet, which led to a fantastic disaster scene the first time we tested it in the lab.
For the past couple months we've been refilling the water chiller at about 2 gallons per week. The system is closed, so we were sure there was a leak. We were never able to find it though because you can't open the access panel with the exposed 1.5HP finger eating fan running inside.
Once it was open for draining, I toggled the manual bypass valve to try to get some of the last liquid out of the maze of pipes inside, and found this gem:
The manual bypass valve has a 1" long 1/16"wide crack running down the length of the body, which vomits a vile mixture of antifreeze and fungus water when toggled.
The other user accessible valve I needed, naturally, is also broken:
This valve shuts off the flow to the water pump, so that you can disconnect the device you're cooling water for. It now only closes to the point of the chiller drooling like an old dog.
Monday, September 6, 2010
Saturday, September 4, 2010
Almost there
Since we stopped observation on August 22nd we've been reversing our work of the past year, taking pieces off the telescope and putting our gear back into boxes. It turns to be easier to take things apart than to put them together: in under two weeks we've gone from a fully operating instrument to a bare telescope with only mirrors and servos still attached. While Dave and I have been crawling all over the telescope, Ian and Tom have been going through the storage container, packing boxes and making sense of all the junk we've accumulated. Bryan was trying to work on data analysis so we made him drain the water and antifreeze from the chiller into jugs. Today we took apart the gantry, which was the last structure we're going to take apart ourselves.
To remove the various panels we had the telescope in birdbath position for a few days, and an overnight rain left this tree stump pattern on the primary. The Vertex guys are showing up in a little more than a week to handle the dis-assembly of the major pieces with the big crane as well as final preparations for shipping. We're in good shape for their arrival so we're taking a few days off this weekend.
Tuesday, July 20, 2010
HTT at JAO dedication
Thursday, June 10, 2010
Unwelcome Visitor
Wednesday, May 26, 2010
Observations
Things are winding down in the field a bit - tomorrow we'll be briefly down to 5 people for a few hours between Aubra leaving and Hans arriving. The receiver, telescope and readout are behaving well enough now to keep things running with only a few people. We've already achieved many of the instrument demonstrating astronomical observations we planned to in California, including:
- Jupiter - the brightest point source in the sky at 150GHz, for mapping our beams and calibrating throughput
- Tau A, the crab nebula - A bright polarized source in the sky, for demonstrating and calibrating polarization sensitivity. Humans saw the supernova progenitor 1000 years ago.
- The Galaxy - We're observing this one the same way we'll observe the cosmic microwave background, but it's much brighter, so it has a fast turnaround time and acts as a dry run for science.
- Saturn, Mars, 3C279, J1229+0203, etc - An assortment of sources across the sky, planets and the brighter quasars, whose positions have been measured to exquisite precision using optical telescopes and interferometer arrays like CARMA. We measure where they appear to be in our telescope, and check that against where we know they actually are.
Friday, May 21, 2010
Hair cut
Tuesday, April 27, 2010
Automated operation
The Polarbear receiver with operating bolometers ran continuously as the HTT scanned the sky all night last night. We all left it to get some sleep, but as of dawn, all systems appear to be working. As you can see from the dawn photograph, the weather was imperfect by morning. We'll have to look at the data to see how opaque the atmosphere was during the night. Jupiter will rise above an elevation angle of 20 degrees in 5 minutes, and the telescope will start observing it as soon as it does
Sunday, April 18, 2010
Days 12-16, Cooldown
The aftermath of assembling and
installing the receiver. Where's the broom?
Ian arrived along with Nate from UCSD
Chase and his stylish hat
Peter and Marius finished weatherproofing the electronics crate.
Dave and Adrian preparing for optics alignment measurements
from inside the telescope.
Measuring the position of the primary mirror
Monday, April 12, 2010
Day eleven: Mounting the Receiver
The receiver was lifted into the telescope and attached saturday
Ziggy and Bryan leak checking the receiver
The A-frame holds an I-beam with trolleys
and chain hoists.
to measure the relation of the focal plane to tooling balls
Almost there
Load straps and engine levelers.
temporarily on the ground.
Everyone watches the starting of the pulse tube cooler
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