The Telescope Array in Millard County

Latest TA News

December 20, 2005: A new web site for the TA Environmental Assessment.

February 10, 2005: The Plan of Development is submitted to the Fillmore BLM Office.

February 2, 2005: BLM Deputy Director Jim Hughes from Washington DC visits the TA (my presentation).

January 19, 2005: Fillmore BLM visits the surface detector sites (some of my pictures).

December 21, 2004: Helicopters deploy the first 18 surface detectors on SITLA lands (some of my colleages' pictures). And their picture of our first fluorescence detector building on Black Rock Mesa.

August 2004: Newest pictures from the county fair (you can see a scitillator station!).
8/28/04: (Belated) Ground Breaking at Black Rock Mesa! Pictures say more than a thousand words...

Under the leadership of the ICRR at the University of Tokyo Japanese physicists have obtained funding to build the Telescope Array an array of 576 scintillation detectors on the ground. A PDF version of the layout as shown above with the water features and another version with mountains shown in shaded relief are also available: Water and Mountains.

On the US side the collaboration is led by researchers at the University of Utah, Department of Physics. The Utah HiRes group has a proud tradition in the air fluorescence measurement of extensive air showers produced by high energy Cosmic Rays. From the first successful use of this technique by the Utah group under the leadership of the late Professor Keuffel it developed it in an ongoing series of experiments on the Army Dugway Proving Grounds.

In the summer of 2002 a single HiRes mirror was deployed on the Black Rock Mesa south of Deseret to compare the local atmosphere around Delta to Dugway. It recorded laser shots fired straight up into the night sky from the TV hill above Oak City - much in the same manner as we do on Dugway to monitor the atmospheric conditions during our data taking. The experiment on the Black Rock Mesa was conducted with the help of students from Delta High School, who took shifts with us during the moon-less nights that made up our observation time. The results from that experiment verified that the atmospheric conditions around Delta are very similar to those found on Dugway.

Our Japanese colleagues are the experts in scintillator based ground observation of highest energy cosmic rays. For ten years they observed cosmic rays with the AGASA experiment, coming to conclusions that seem somewhat different from what we see in our HiRes data. The AGASA experiment is finished now, and the next step for our Japanese colleagues is to build TA here in Utah with us. Like the bigger Auger observatory TA is a hybrid experiment, integrating both the HiRes and the AGASA observation technique in an effort to resolve any apparent discrepancy. Auger is a hybrid between fluorescence detectors and water Cerenkov counters on the ground as opposed to fluorescence and scintillators in TA. Since water Cerenkov detectors and scintillators each have their characteristic responses that emphasize different aspects of an extensive air shower, it should be particularly interesting and powerful to combine these two ground array techniques by interleaving them to measure the same showers. This is one important way in which co-siting Northern Auger and TA could generate synergy. Northern Auger is the necessary complement to its southern site, achieving all-sky coverage for the first time in the history of highest energy cosmic ray observation. TA is funded and will be built in Millard County, Utah - a site consciously chosen at a time when Millard County also was the designated site for northern Auger.

Below I have links to the transparencies I used in some recent talks of mine. The talks were directed to the general public and discuss TA in particular:
1.) talk given at the College of Science Day 2003
2.) talk given in Delta January 9, 2004
3.) talk talk given in Delta January 21, 2004
4.) Public Hearing presentation given in Fillmore March 3 and in Delta March 4, 2004.
5.) Presentation to the Air Force given at Hill Air Force Base on March 10, 2004
6.) Range Program Planning Board Meeting at Hill Air Force Base on April 8, 2004
7.) Presentation to BLM given at the BLM Utah State offices on May 10, 2004

Caution: The originally planned High School Contest alluded to in some of the earlier presentations is cancelled. VERY sorry about that!

During the public hearings it emerged that BLM will not be willing to process our application until a final design for the scintillation counter support is presented. BLM suggested that we ask an engineering firm to produce a viable design much before the contest would yield one...

Update (March 30, 2004):

The High School Contest is abandoned at this point and replaced by a process where an engineering firm hopefully with local expertise from Millard County will be charged with designing this structure. An add soliciting show of interest from qualified companies is in this weeks (week of March 30, 2004) Chronicle Progress. The add asks that interested companies contact me via e-mail giving their contact information and with a subject line reading "support structure" by April 6, 2004. A rough sketch of my conceptual design for the structure is shown here, with the blue box representing a thin walled stainless steel box the contains the plastic scintillator material that needs to be held horizontally by the structure. The stainless steel box and the enclosed scintillator material weigh about 350 lb, to which the weight of batteries, solar panels, and a light electronics box will have to be added. The dark gray box sitting on top of the blue scintillator in the view from the short side (upper left of the white panel in the viewgraph) represents this electronics box. A roof should provide shelter from solar radiation as well as rain and snow and be painted as to blend in with the surrounding sagebrush as well as to prevent reflection that might irritate pilots during exercises in the UTTR. The design has to be simple and affordable for mass production, with more detailed design goals to be supplied by us at a later stage. Deployment considerations will also have to play a role in the design and engineering of this support structure.

We keep looking into how to meaningfully involve the local High Schools in our work. The decision to abandon the contest was forced upon us through constraints imposed by agencies involved in the permitting process for our project. Other opportunities will arise as the project unfolds. Press releases concerning TA:
1.) January 12, 2004

Here is the original list of scintillation counter coordinates. The coordinates were calculated by a computer program that I wrote and are not yet adapted to the local geography. Individual counters will have to be moved from their ideal computed position by hopefully not more than 50m absolute to respect the local terrain. Some locations have already been visited and preliminary adjustments have already been made where it was found necessary. Below you will find an updated list for the part of the array that is on public lands.

Ground Array Site Staking on Public Lands:
June 14-25, 2004

In the two weeks indicated we are aiming to stake all the ground array counter positions that are on public lands. BLM has requested us to do this so they can review our R/W application. In preparation for this effort we put up beacons at the five communications tower positions: these visual beacons will allow us to verify the communication paths between detector locations and the communication towers as we do the staking. For more pictures of the beacons themselves please follow this link. The beacons are made from fiber column forms for concrete and painted with a highly reflective paint. The one on Black Rock Mesa has a red stripe around its middle.

Well, time has moved on, and another job is done: The staking was was done in a wonderful team effort with our Japanese colleagues! Everybody was working together to keep the schedule, and despite one and a half days lost to rain and subsequently muddy terrain we finished by 11am on Friday, June 25. The result of this effort is a new and final list of detector locations for all sites on public lands. For the moment it still contains five locations where we have two sites staked each. Before the middle of July we will have these ambiguities resolved. The preliminary list with the five ambiguous sites can be found here. All coordinates are WGS84.

Food for thought: Many communities and counties have recognized the value offered by the beautiful desert night sky and adopted a dark sky ordinance. As discussed in the link there are good and bad ways to design such an ordinance, but little doubt seems to exist that it helps - if you like the stars, that is.

Please come again: Updates are certain.


Kai Martens
Last modified: Sun Feb 6 22:44:44 MDT 2005