I'm in the cheapest motel in Richland, Washington. I'm driving an unmarked sedan with U.S. Government plates. I feel like Mr. Mulder.

My flight out was uneventful but pleasant. On Tuesday I left our house at 9 am, walked to the bank and then to the train station, catching the 9:30am metro for Los Angeles for $1.25. At Union Station I walked under the long-distance Amtrak trains to the bus depot, and at 10:00 I was on the "FlyAway" bus bound for the LAX airpot. Four dollars. Twenty minutes later, LAX. I drank a coffee and hacked away at my computer for an hour until my Alaska Airlines flight to Seattle boarded, at 11:30.

The flight out from Los Angeles was glorious. With my nose to the window my eyes searched out the geography of the Santa Monica mountains, the Carizzo Plain, the central valley. The peaks of the Sutter Buttes rose up and I thought that Mt. Shasta was strangely wimpy--but then the real Mr. Shasta rose up, snowbound and awesome in the clouds. (I've got to get a pilot's license!) Seattle looked snug and beautiful, pretty houses and trees scarlet and gold in the autumn. From Seattle the mountains are a jagged knife. We hopped over them in a short but turbulent flight in a turboprop airplane. Pasco.

Since then, long days at the LIGO Hanford Observatory. The well water on site is delicious. It comes from a superfund site. Day two: nine AM until midnight. Since then we've taken up a more reasonable noon-to-midnight. Tomorrow: laser intensity noise. Control room just called: my script has a bug.
IMG_1621
Tumbleweeds massed on the LIGO beamtube

Awesomely, theoretical physicist and old-school (usenet!) blogger John Baez describes a visit to LIGO Livingston Observatory in the latest posting of his "This Week's Finds in Mathematical Physics." This describes where I will be working for a year starting in August 2007, and is an apt description, too, of the LIGO observatory in Hanford, Washington where I spent the last week.

The place was pretty lonely. During the week lots of scientists work here, but this was Saturday, and on weekends there's just a skeleton crew of two. There's usually not much to do now that the experiment is up and running.

Yup. For the last couple days, one of those two was me.

As Joe Giaime later said, there have been no "Jodie Foster moments" like in the movie Contact, where the scientists on duty suddenly see a signal, turn on the suspenseful background music, and phone the President.

Hilariously, a email recently went out urging everyone to be careful about writing too explicitly about suspected gravitational wave detections in our log books, since those log books are readable by the public and any suspected discovery must be carefully checked, a process likely to take months. The idea that we would see a gravitational wave detection, in real time, from the control room—it seems ridiculously outlandish.

There's just too much data analysis required to see any signal in real time: data from both Livingston and Hanford is sent to Caltech, and then people grind away at it. So, about the most exciting thing that happens is when the occasional tiny earthquake throws the laser beam out of phase lock.

Too true! Earthquakes and storms cause much of the excitement. There are lots of seismometers at each LIGO observatory to monitor them, and I entertain myself processing data from the seismometers, as they are guaranteed to detect events every couple of minutes. I made a nifty contraption that shows where seismic waves are coming from:

Seismic beamforming to resolve a Mt St Helens event
See [livejournal.com profile] nibot_lab for an explanation

My arrival at LIGO Livingston is to coincide with the end of the current science run, this period of quiet listening and continuous recording. The place should become a hive of activitiy: the current LIGO will be partially disassembled, and during the year I'm there, a series of upgrades will make it much more sensitive. Instead of sitting in the dark listening for a faint signal from space, I'll be hacking on lasers and optics and all that jazz.

As for John Baez—he's a bit of a hero. I actually wrote to him when I was applying to grad school and he encouraged me to apply there at UC Riverside where he is a professor. In the end I didn't—it was late in the game, Riverside's not so appealing, and applying to a math department seemed a tad far-fetched. But I still read This Weeks Finds with a bit of a bittersweet sense of a path not taken.
Storm clouds over LIGO/Hanford.



Check out the full size version of that image too.


Adrian and me


Stefanos and me


More posts and pictures about LIGO: http://www.livejournal.com/users/nibot/tag/ligo
We (Adrian [professor], Stefanos [fellow grad student], and I) arrived here in the Pasco/Kennewick/Richland "Tri-Cities area" yesterday after something like fourteen hours of travel, hopping from Rochester to Chicago to Salt Lake City, and then finally to Pasco on a little Canadair Regionaljet. When I left Pasco last time, it was on the wings of an incoming blizzard; now it's hot and dry and the newspaper headline is, "Dust storm blackens Eastern Washington." Driving out through the sagebrush, it's good to be out West again. Our hotel room has an excellent view of the river. Yesterday afternoon when we arrived, Stefanos and I maintained illusions of going out to check on the hopping cafe scene (etc) of the Kennewick area, but what was originally declared a "short nap" at 5pm turned into the night's sleep, exhausted from the ridiculous travel that had commenced at 3:30am in Rochester.

Our location on Google Maps.
After several days of fighting with the peculiarities of the computer system at LHO (LIGO Hanford Observatory), my analysis program is good to go—and it is awesome indeed. All I need to do is type "make submit" and my program finds the data to be analysed, constructs a tree containing thousands of processing jobs that will perform the analysis, and then submits these jobs to the computing cluster at LHO. Working late at night on a Sunday when nobody else is using the cluster, I have all of the computing resources to myself: 276 processors, each running at several gigahertz, each one with a gigabyte of RAM, with a collective total of twenty seven terabytes of hard disk space, and access to a robotic magnetic tape system containing who knows how many terabytes more. Amazingly all of this sits in one room in a remote, desert corner of Washington State. Amusingly the data processing program consists of only 216 lines of Matlab, 100 lines of Python, 26 lines of Makefile, with a pinch of sed and dash of other unix goodness thrown in for good measure. Programs that write programs: that's what makes CS fun. As I said: type "make submit", wait, then results.mat will be sitting there, ready for ingestion by Matlab and consumption by the analysis phase.

Kent and I joked that a proper scientific analysis program should start with the raw data and ultimately typeset and mail the resulting publication. I wasn't really kidding. Read paragraph three of Background: Kepler. This time I might have it: type "make analysis" and that results.mat file will be picked up and churned through the analysis. Hypothesis testing is done. Figures are generated, in PNG and EPS. The LaTeX typesetter is run, producing both postscript and PDF. If I were properly awesome, the proper concluding text will be subbed in given the results of the hypothesis testing. Ultimately: Type "make all." Robots in Washington State awaken, transcribe signals from magnetic tape to disk. An army of machines grinds through the data. A program in New York State performs model fitting, hypothesis testing. LaTeX turns this into a beautiful manuscript, which the Laserjet 2300dn fuses to the page.

Pull the page out of the printer and read what you have discovered.


LIGO-Hanford Control Room


Beamline electronics cabinets (VME crates)


Testing circuit boards


My rental car on some Hanford road


Arrival back in Rochester (the plane didn't make it all the way to the gate, due to the snow -- or something)

Todd Matthews' Atomic Postcard is a great description of the place.

Back in Rochester now after a long but uneventful sequence of flights. The weather here in Rochester seems to be exactly the same as it was in Pasco when I left. The airplane didn't quite make it all the way to the jetway (on account of snow on the ground?) and so they had to wheel out the ladder contraption. Now to get back into school mode.. oh no! (I think Ryan's first words to me back here at the house were, "We need to go on a roadtrip!")

LIGO day 6

Jan. 15th, 2005 07:04 pm
IT's been a busy week at LIGO for me.. taking data, installing electronics, soldering, assembling, testing, spectrum-analysing, programming, etc. The LIGO electronics shop here has all the oscilloscopes, multimeters, spectrum analysers, function generators, power supplies, cables and connectors of every sort, etc etc, to make any reasonable person happy.

This morning I stopped at the Columbia River Exhibition of History, Science, and Technology museum here in Richland, where for $2.50 a retired Hanford worker gave me a two-hour tour of interpretive displays and models of the Hanford Works. I quizzed a guy at work on interesting places to go see around here, and he was full of ideas. I ended up just driving up around Hanford Site to a place where there's a view of the reactors.

I drove out to the farming town of Othello just to have a destination... it started to snow, which at first was novel, but then very quickly I realized that there was a strong possibility that I'd get stuck out in the middle of nowhere. Was quite relieved to get to a larger highway which is plowed. I stopped in at LIGO to take care of a few things... the two people there were gearing up to be snowed in.

Back in Richland now... I have a flight out of here at 9:00 tomorrow.. to Salt Lake City to Chicago to Rochester. Rochester! Yay! Looking forward to seeing people I know again.

LIGO Day 2

Jan. 11th, 2005 09:28 pm
Dear Taxpayers,

Thank you for the Swordfish dinner. I promise I will try to find some gravitational waves. I understand that you accept gravitational waves as payment for swordfish.

Tobin

* * *

Today Adrian and I came prepared to the LIGO site, with turkey sandwiches in lunchbags. The place is far enough out from town that it's not worthwhile to drive all the way back to eat. One of the LIGO offices has a kitchen, so one could really set up camp there. In fact, I've been scouting out tent locations in case I have to come back for a longer period of time. (I tried that at CERN and was quickly picked up by CERN security; I suppose it was a little brash to set up a tent right outside the main dormitory/cafeteria, but it does seem to me to be a reasonable and adventurous way to save the Government some money...)

* * *

In the morning we set out to drive the gravel road that follows the beamline, but the snowcover looked a bit much for the little Chevy rental car. There is a little "overpass," though, over one of the arms of the interferometer so that you can drive along the other arm in the inside of the "L". From there there's a nice view of the interferometer arms stretching off into the distance. It doesn't look quite as big as I expected, but I think I might have been looking at the midpoint stations.

We found ourselves a spectrum analyser, hooked up our little "whitening board," and measured the frequency response on each of its four channels. Everything checked out perfectly, so we went and installed it at the beamline, connected up signals from the interferometer's photodiodes (navigating around two bad channels), and took spectra on the output. Everything looks good. Tomorrow we'll hunt for signals!

We also transferred 5.6 GB of data onto Adrian's laptop. In the process I got to see the on-site computing center. Fairly impressive! Everything here is SUN (and all the test equipment is Stanford Research Systems; keep in mind that SUN originally was an acronym for Stanford University Network). There's something like 10 TB of online storage (fibre channel!), 100 TB in a tape robot system, a fast internet link to Caltech, and 280 xeon CPUs in a computing cluster.

Apparently some of the signal searches are actually limited by computational resources. To look for pulsars, for instance, you have to try all the doppler shifts and some other parameters. Therefore, in the tradition of SETI@Home, there's now Einstein@home which lets your computer help search for Gravitational Waves!

LIGO Day 1

Jan. 10th, 2005 11:39 pm
After a reasonably sumptuous breakfast at the hotel, Adrian and I drove out to the LIGO site. It's really closer than I had expected. The city of Richland, such as it is, peters out and quickly we're out on a straight stretch of 2-lane highway seemingly in the middle of nowhere. Steam is billowing up from somewhere a few miles off the road -- a reactor still running? The snow-covered desert is really quite pretty; the snowy hills blend right into the sky. At a bend in the Yakima river, we turn right onto the road that doesn't exist. A few miles later we're at the LIGO site, with a big sign out front with the LIGO logo.

There's a small collection of buildings at the "corner station" (the elbow of the "L"). One where we check in, where there are some offices too. Another has a tall roll-up door; this is some kind of assembly area. And the third building in the corner station itself. Inside everything is clean and well organised; it seems new.

The first half of the day was mostly the formalities (signing papers, reading safety information) and practicalities (getting keys, being shown around) of being introduced to LIGO, and the dozen-or-so people working on site. The Control Room is like Mission Control, with five projector displays on the wall (only the three forward ones currently in use), showing the current Interferometer status. Overhead, two large digital clocks display the time, one in UTC and one in local time. On two rows of desks there are numerous computer terminals, each with two large flatscreen displays. Almost all SUN Sparc machines. Closed-circuit TV displays show the area surrounding the LIGO center, and others show the LASER spots inside the interferometer. Most of the stations have the usual roller-chairs, but a few large inflated "fitness balls" are available too, lightening the atmosphere a bit.

At lunchtime we attended a meeting of the collaboration. Like at Big Physics labs everywhere, the meeting is done by teleconference on a sort of speaker phone system with PowerPoint slides projected onto the wall. The other LIGO observatory, in Livingston, Louisiana, is on the phone. As are, I think, the collaborators at MIT and Caltech. The meeting is, as meetings tend to be, very boring. They are planning when to do some big upgrades, planning for the next several years.

Daniel took Adrian and I into the clean-room environment that houses the corner station to get us acquainted. There's an automatic boot scrubber before we enter the 'garb' room, and then we put on booties and LASER safety goggles. Earlier Adrian had drawn for me a schematic of the LIGO observatory. The input laser is only a few watts, but the arms of the interferometer form resonant cavities, which build up a laser power on the order of kilowatts. The laser is infrared. We have proximity cards to enter the cleanroom area. We enter one-by-one, and the computer notes that we're now each "inside". Entering an area without using the proximity cards activates interlocks and automatically shuts down the lasers. The safety system is to protect people from lasers, and the cleanroom system is to protect the ultra-high-vacuum system and the clean optics from the dirt that rides in on people.

Once inside the clean area, the vacuum system of the corner station is visible. The beamlines are housed in a vacuum pipe about 1m in diameter. The optics systems are housed in large metal cylinders along the beamline that look like giant tin cans welded into the system. Beside the beamline are the usual rackmount systems familiar to any physics installation: crates containing VMW-bus backplanes, with cards sprouting patch cables. Analog signals are routed into digitizers. The digital signals are eventually stored in a sort of distributed shared memory, which is reflected between machines using gigabit ethernet over optical fiber. The air is clean and it's easy to breathe.

Daniel showed us around the electronics and we set about our mission. For various reasons, there is an interest in looking at a signal at 37.5 kHz -- noise tends to cancel out at this frequency, so it might be a good place to hunt for a signal. To gain access to this signal, software digital signal processing is used to shift this signal down to baseband, so that it can be stored at a reasonable sample rate. Our task is to verify the frequency response of some "whitening" (equalizer) boards, connect signals from the interferometer output photodiodes to this board, make sure the data acquisition (DAQ) is working properly, record data from this frequency range, and then look at it. The DAQ system seems to run on VxWorks (I believe the same OS that ran on the Mars rover).

I really have to brush up on my signal processing... FIR and IIR filters, Butterworth filter design, complex baseband signal representations / quadrature, control systems design. LIGO is really all about control loops: The main operating mode of the interferometer is to keep the interferometer output locked at a "dark fringe" (no light output; total destructive interference) by using actuators to move the mirrors; and the feedback signals to these actuators becomes the output signal of the detector. There are several resonant cavities, most of which are kept resonant by active control systems.

In between times, Adrian explains all about how LIGO works, and what we will be doing. ("And tomorrow, Dark Energy," he says. I don't know what Dark Energy has to do with anything...)
LIGO, sitting out here in the desert, staring up into space, listening carefully for a signal -- it reminds me of SETI a little bit, the project that is listening for radio transmissions from other civilizations. Like with SETI, it is unlikely that the current LIGO installation will detect anything; but it will be a big deal if it does. It's actually quite a poor comparison, because we're very sure that Gravitational Waves -- what LIGO is listening for -- exist, and it's merely a manner of building a sufficiently sensitive listening device. Hearing from an honest-to-god ET would be a Much Bigger Deal indeed. Maybe what makes me relate the two projects is the degree to which both are inherently peaceful.

Big Physics has historically been all about accelerators -- machines that you might call "atom smashers" even though they don't smash atoms anymore (they've moved on to much smaller things to smash), and today there are huge accelerator projects (Fermilab near Chicago, CERN near Geneva, SLAC at Stanford) and they are entirely peaceful operations. But the history of accelerator physics is not quite so peaceful. The first big accelerators were invented and built at Berkeley, and with them came the ability to smash atoms together, forming exotic new elements and the field of nuclear science. A young Glenn Seaborg stumbled across Plutonium there, some others stumbled across Fission, and suddenly everyone involved was booking train tickets for Los Alamos and Chicago.

In the American nuclear archipelago, Hanford Site may or may not be the Big Island, but it's certainly the biggest mess.

From http://www.columbiariverkeeper.org/history.htm: In January 1943, Hanford was chosen as a site for the government's top-secret Manhattan Project. The mission was to produce plutonium for the nuclear bomb. It was selected because of it's remoteness, its abundant water for reactor cooling, and its plentiful electricity from hydroelectric dams. In the spring of 1943, 1,200 residents were evacuated from the towns of Hanford, White Bluffs, and Richland. Access was denied to Native Americans who had historically used the lands for hunting, food gathering and religious purposes. The world's first three plutonium production reactors were quickly built with a work force of 51,000. Just 27 months after construction started Hanford-produced plutonium provided the explosive charge for the worlds first nuclear detonation in Alamogordo, New Mexico. Not long after, the Nagasaki bomb was powered by concentrated plutonium manufactured at Hanford.

Weapons-production activities at Hanford came to an end with the end of the Cold War in the 1980's (so recent!). Now the big project at Hanford Site is cleaning up the mess, to the extent that it can be cleaned up, at a monetary cost of ~ $100 billion.

* * *

LIGO has nothing to do with all of this, however, except that it was built here at Hanford. LIGO is a big L-shaped contraption, with each arm of the "L" four kilometers (2.5 miles) in length. Laser beams travel through the L, bouncing off of mirrors at each end. The whole thing is a giant — and very complicated — interferometer, identical in principle to (but vastly larger and more sensitive than) the interferometer that Michelson used to disprove the existence of the Ether. In LIGO the idea is that a passing gravitational wave (coming from a galaxy far, far away) will stretch space, changing the path lengths in the arms of interferometer, resulting in a measurable signal.

The whole thing becomes very complicated because Gravitational Waves are very weak: a 4km arm of LIGO is expected to change in length by 1/1000th of the diameter of a proton!

Why is LIGO built way out here at Hanford? Largely for the same reason the Government chose to put a plutonium factory here: remoteness. With the extreme sensitivity of the LIGO machine, it would be completely overwhelmed by the vibrations from city traffic in a big city. The other reason is just that there is space here to build such a large machine. [I also wonder whether it's important that the other LIGO observatory, at Livingston, LA, be as far away as possible, or have some other relative positioning requirements.]

Driving directions to LIGO: "The key turn-off along this route is unsigned, so we cannot recommend it unless you know the surrounding area well. There is a jog in SR-240 at the North end of Richland. Coming from Richland, you can jog to the left and follow SR-240 about 10 miles out into the countryside. Eventually you will see the Yakima River along the left side of the road, which is your signal that you are getting close. You will see a weir in the river, near where the river takes a sharp bend. This is Horn Rapids. Look for a big green sign just before a four-way intersection. The sign will indicate that SR-240, to Vantage is straight ahead and SR-225 to Benton City is to your left. The sign gives no indication whatsoever that there is a two-lane highway, SR-10 that goes to the right. (This is probably an intentional oversight harking back to the days when Hanford was a secret and very secure site. We recently have gotten assurances from the Washington State Department of Transportation that this road does not exist, although many of our employees drive it every day!)

* * *

Adrian pointed me to a nice anecdote about Wilson, a Director of the Fermilab accelerator. He was asked by Congress how Fermilab would contribute to national defense, so as to justify its cost:

[I]n 1969, when Wilson was in the hot seat testifying before the Congressional Joint Committee on Atomic Energy, Sen. John Pastore demanded to know how a multimillion-dollar particle accelerator improved the security of the country. Wilson said the experimental physics machine had "nothing at all" to do with security, and the senator persisted.

"It has only to do," Wilson told the lawmakers, "with the respect with which we regard one another, the dignity of men, our love of culture. It has to do with: Are we good painters, good sculptors, great poets? I mean all the things we really venerate in our country and are patriotic about. It has nothing to do directly with defending our country except to make it worth defending." (http://www.news.cornell.edu/releases/Jan00/RRWilson_obit.hrs.html)
Hampton Inn - Richland, WA
On the banks of the Columbia river
Washington State, East of the Cascades

64 km from Oregon, 120 km from Idaho
352 km from Seattle

30 minutes from Hanford Site

-3.8°C with light snowcover, crunchy ice

I'm on some kind of mission here, but I'm not sure what entirely. They gave me plane tickets to Pasco. A rental car was ready at the airport. I met Adrian at the hotel for dinner. He'd arrived an hour before.

In the morning we'll drive out to LIGO's Hanford Observatory and I'll find out for real why I'm here.

March 2020

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