Pierre
Auger Project
Progress
Report
Summary (photo album)
May was a particularly good month for surface
detector
deployment with 64 detector stations deployed and 63 filled with water. Because of bad weather and a shortage of
tanks, June will not be nearly as good.
The delay in tank delivery resulted from a (successful) effort
to
qualify a new vendor in
The new SD “cyclone” front end board from
The three fluorescence eyes are all operational. Some difficult to locate software bugs remain but data taking has otherwise been smooth. Corrector lenses are being added at a regular rate such that all telescopes should have lenses by October. We do not yet have access to the land for the Loma Amarilla FD building but expect it very soon. We expect construction to begin in September.
The DPA/offline structure is making steady progress. We hope to soon add more resources to that effort.
Although we have not yet identified all the funding that is needed to finish the Observatory, it now looks quite hopeful that we will complete the project as planned. Identification of funding of the last pieces of the array will be another reason to celebrate in November.
WBS 1.1 Fluorescence Detector (Jonny
Kleinfeller – Karlesruhe)
There are now at least 2 corrector ring lenses in operation at Los Morados.
Los Morados has been in operation during
the recent 2
dark periods.
All calibration systems have been installed at Los Morados.
Apart from corrector ring lenses, we can state 75% of FD is completed
and
operating with reasonable reliability.
WBS 1.1 Fluorescence
Detector cont. (Stefan Westerhoff –
During the May and June 2005 fluorescence runs,
the LIDAR
team completed and successfully operated its shoot-the-shower (StS) software. The programs are set up to
initiate
laser shots along the shower tracks of the largest hybrid and stereo
events, at
a rate of approximately one shot per LIDAR site per hour.
Starting one
week into the June run, we implemented the StS code and observed both
LIDAR's
properly shooting hybrid and stereo events in the FD fields of
view. Data
from the best events were presented at the
In addition to making progress on the StS, we have also completed
several
visualization and utility programs that allow users to easily monitor
the flow
of data. The webcams at both LIDAR sites are now operational,
enabling
runners to remotely observe the telescopes. We also cleaned up
and
organized the software environment on the PC Irene in CDAS, hopefully
easing
the task of runners on shift. During the next set of FD runs, we
would
like to address some lingering software and hardware problems,
including
instabilities in the T3 client software that runs on the FD PC's, and
drops in
the PMT high voltages that tend to appear after each StS.
Moreover, we
hope to refine the selection criteria for hybrid and stereo StS by
further
studying the hybrid and stereo T3 event rates.
WBS 2.1
SD (Ingo Allekote
–
Instituto Balseiro)
As of May 31, 2005, a total of 889 SD were
deployed in the
field, of which 855 contained water and 758 had electronics kits
installed. In
conclusion, over 50% of the surface detector tanks are deployed and
filled with
pure water. With 64 detectors deployed in May, the highest deployment
rate
since the beginning of the project has been achieved. However, due to a
series
of failures of the water transport trucks, the deployment rate for June
is
expected to be considerably lower.
One of the tanks filled with water was "Ayumi",
a tank that had been deployed long before and could not be accessed for
many
months, leaving a hole in the array. To fill this tank, a system for
using long
hoses (500 m) with additional pumps was developed by the local team in Malargue.
The fourth water transport tank, Tk-12-delta, was put in operations. It
required the construction of some extra support ribs to enhance its
rigidity
for the rough terrain in the field.
Solar panel brackets were produced and delivered satisfactorily by Equipos y Proyectos.
A new order for battery boxes has been placed at Formingplast
and Rotopol, who are producing 100 each.
After completion of liner production at UTN in
from UTN were designated as persons in charge for the liner testing in Malargue. The testing activity is expected to be
completed
by December 2005.
WBS 2.1 SD cont. (Peter Mazur - Fermilab)
In order to reduce the
cost of tank production in
The company has now made a mold for the production of our tanks and has begun producing tanks to develop and refine their production process.
Approximately eight tanks suitable for shipment to Malargüe have been produced, along with about five developmental tanks that were not suitable and were cut apart to study the internal structures in order to improve the molding process.
A new trucking company was located very near to the molding factory and an arrangement made for shipping a truckload of tanks in order to develop the shipping procedures for this company. Shipment of the first eight tanks is waiting only for the customs waiver.
With the funding
presently in hand,
The Juan Carlos
d’Olivo of UNAM has announced that the Mexican funding agency CONACyT
has just
awarded sufficient funding for 160 additional tanks. This number can be
added
to University funding from
With the funding
available from
Resin for all the tanks discussed above is provided by the US (Fermilab.) 169 tons of resin have just been ordered (which includes 9 tons of resin for the manufacture of battery boxes and enough resin for about 290 tanks) to be shipped to Argentina and Brazil.
WBS 2.2 Surface Detector Electronics (Tiina
Suomijarvi – IPN Orsay)
There are currently about 760 tanks with electronics on site.
3253 PMTs have been received on site. Currently no particular problems are found in the PMT tests prior to deployment. The field failures of ensemble PMT, base and cables are 6%. Half of the failures are due to cables and can be repaired on site. Some of the failures are due to large temperature coefficient. For the moment no specifications have been set for the temperature coefficients. As a corrective action, a more strict connector test has been installed in the AB. It will also be studied whether the failures are infant failures occurring during the first year of operation (after summer – winter temperature cycling).
The most UB failures are due to fuses. The fuses will now be systematically changed to bigger ones which should correct for the failure.
The Cyclone board passed a critical design review during the Orsay analysis meeting. Until the Cyclone production will get online, a minimum rate of 50 boards per month will be ensured with the current design.
A preproduction batch of 30 TPCBs are expected
from the
The SDE commissioning studies are still in progress. Figure below shows the ToT rate. A stabilization time of a few months is typically required before the trigger rate reaches the nominal value of about 1.5 Hz.

This period has seen us dealing with increasing load at the ‘back-end’ of the comms system as more detectors are added. Deployment of antennas and preparation of antenna kits has continued, with some important milestones passed.
· Surface Detector Antenna System preparation and deployment – Jorge Abraham
· 59 Kits were mounted during April 2005. 63 during May 2005 ** The best month !!!.
· There are 166 ready to install. Total made: 1025 ** 1000 reached in May !!!
· Antennas for more than 100 Kits were tested antenna feeders for more than 50 Kits were tested too.
· The 855 antennas mounted were reached.
· During June-July will arrive “the last” batch with 160 Antennas.
·
During 2004 and 2005 we placed the
ultraviolet
protection. From 275 Unprotected Kits we protected 116 in 4 trips to
the
Comms Upgrades
A number of important upgrades were made to the comms radio racks in all the comms shelters;
Interface rationalisation – In order to reduce system loading, the Base-stations were reconfigured so that the supporting TCP/IP interface units now service a maximum of 3 base-stations each (reduced from 4).
TCP/IP interface processor upgrade – again, to reduce loading, all the embedded Linux processors inside these interfaces were upgraded from 48 to 66MHz.
A new Comms System control PC (the ‘MetMon’ PC) has been ordered and will be deployed at the site during the next period. This is a good performance ‘server-type’ rack PC that will be able to support management of the full 1600 node array.
Last
Shipment of Radios Arrives in Malargue
This occurred
around the middle of
June so strictly speaking should be in the next report; however it’s
still nice
news.
WBS 5.0 DPA/Offline-
(Bruce Dawson, Markus Roth and Tom Paul)
A new beta release of the offline software
(version 1.2) was
produced in May, providing a number of enhancements and bug fixes.
A few serious bugs in the SD simulation codes were corrected, including
errors
in resampling routines which seemed to account for at least some part
of the
constant intensity problem.
Some optimization of the SD simulation modules has been performed,
resulting in
an increase in simulation speed by nearly a factor of 2.
Version 1.2 is compatible with the latest CDAS code (4.2). Filling of
the raw
SD event has been moved to a dedicated module in order to make it
possible to
read
The SD reconstruction modules underwent a complete rewrite since the
PRR in
November 2004. The aim was to simplify the code and to make it more
stable and
robust, while keeping the same methodical approach. A detailed
description of
the reconstruction algorithms is given in a
recent internal note (GAP-2005-035). The SD reconstruction example is
revised
and some more information is reported on for showcase purposes. The
SdRecPlotter, a module for displaying events, is rewritten as
well. There
are lots of eye-catching additions displaying more
detailed information. The rewritten SdEventSelector module performs the
latest
official event selection (GAP 2005-023; a conservative T5 trigger with
at least
6 non-dead stations as neighbors).
A first set of high level interfaces to the molecular database have
been
prepared, making it straightforward to access monthly average profiles
as well
as data from radios on launches. Similar interfaces for the aerosol
database
are in preparation.
A Tutorials section is now included with the offline
distribution. It
contains a few very simple example programs demonstrating how to use
the
offline framework to perform common tasks. We plan to populate
this area
with examples to help answer the most frequent questions from users.
WBS 9.0
Observatory Operations – (Julio Rodriquez Martino - INFN)
Data taking with the FD continued normally during April and May. Some hardware and software problems still show up each night. Specially problematic is the fact that the mirrorPCs disconnect from the DAQ, forcing the operators to power cycle both the PCs and the electronic crates and to restart the data taking run each time. The whole procedure takes several minutes, contributing a large fraction to the telescope dead time.
This problem is especially important in Los
Morados, where it
happens quite often. The responsible people (
enough human resources. The ideal situation would be that some knowledgeable person spends a whole FD shift in Malargue, analyzing the problem.
Good news is that the weather was nice most of the time, meaning that the data taking was smooth from this point of view.
LIDAR-FD interaction was fine-tuned in LL and CO sites. There is no interference in the FD data taking coming from the LIDAR any more. The "shoot-the-shower" firing mode
was successfully tested in both sites.
The FD calibration was checked by mounting a nitrogen laser on a truck and firing it in front of different bays. The method is similar to the one used when analyzing CLF data, with the added flexibility of changing the position of the laser. Results will be made public soon.