Progress through Photos

This webpage is devoted to Progress through Photos; as the construction of the LWDA test station at the VLA develops and sites for other LWA stations are explored, we will replace older photos with newer ones. Additional photos may be found on the LWA Wiki

Long Wavelength Array

Second summer Work Party at the LWA-1 site. (July 25, 2009 )

The second LWA-1 work party was held on a Saturday. The day was spent putting conduit into the trenches.
Taking a lunch break to eat barbequed ribs in the shade of the trailer!

Construction continues at the LWA-1 site. (July 10, 2009 update)

Here are some more photos from the on-going construction this summer.
Astrophysics graduate student, Steven Tremblay, is feeding the fiber-optic cable (yellow-orange) for the internet connect to the hut into flexible conduit (black). The trenching continues.
Another view of the trenching, cables, and conduit.

First of the summer Work Parties at the LWA-1 site. (June 24, 2009 )

The first summer work party at the LWA-1 construction site was held on Wednesday June 24. Adam Martinez, UNM Graduate Research Assistant in Construction Management is the Manager of the summer construction crew which consists of undergraduate and graduate students from Civil Engineering. Among the senior LWA staff participating in the work day were Lee J Rickard, Executive Project Director, and Walter Gerstle, Civil Engineering Professor. Three UNM undergraduate majors in Astrophysics did most of the heavy work.
Photos courtesy of Hélène (Lanie) Dickel , UNM Adjunct Professor.

LWA summer crew members:
Adam Martinez, LWA Construction Manager and graduate student in Construction Management
AJ Gallardo, undergraduate student in Construction Management
Sunil Danthului, graduate student in Construction Engineering
Sudipta Ghorai, graduate student in Construction Engineering
Volunteer undergraduates, majoring in Astrophysics, who participated in the 1st Work Party
Matthew Koppa, Dave Martin, and Anthony Ortiz
Trenching and preparing junction boxes. Short trenches spoke to where blade antennas will be located.
Lee J shows how to put the connectors onto the short conduit pieces which will connect from the ground to the top of each blade antenna.. Walter in back left and students take over from Lee J and complete the outfitting of the conduits with connectors.
(Above) Lanie joins in the conduit connector task. The done pile at lower left is now much larger than the small pile of conduit pieces awaiting connectors. Adam Martinez and John Dickel (UNM Adjunct Prof) successfully test inserting an extra cable through a conduit already filled with 28 cables - from one junction box to another.

Construction begins at LWA site 1 (June 2009 )

Construction of the first station of the LWA began on June 2nd and is progressing well. Surveying has been completed and the current focus is on trenching for the conduits. As of June 16th, one full branch has been trenched and laden with conduit. The shelter has been ordered. Photos courtesy of Adam Martinez.
A load of conduit pipes. Trench ready to be filled with conduit.
Connecting everything up in the junction box. Covering up the filled trench with dirt.

LWA Review for Long Lead Items (June 01 2009 )

A meeting of LWA staff, Review Committee members, UNM officials, professors, and graduate students was held June 1, 2009 on the UNM campus to present and discuss the current status and upcoming plans regarding the construction of the first station of the Long Wavelength Array.
Photos courtesy of Lanie Dickel.
Some of the participants chat over coffee before the meeting begins.

Fencing installed at LWA site 2 (May 27 - 28 2009 )

UNM graduate students in civil engineering return in May to install the fencing around the 120m x120m LWA site 2 (near the end of the north arm of the VLA) . Photos courtesy of Joe Craig.
Details of the construction of a corner for the fencing around the LWA site 2. The gate can be seen at the upper right of the photo. Looking along the fence with a couple of graduate students barely visible in the distance.
 
Putting in the separators which keep the horizontal wires apart. Looking back towards the VLA (in a compact configuration) in the distance.

Spring Break Work Week (March 16 - 19, 2009)

UNM students surveyed, trenched, pulled cables through conduit, and conducted various tests on the new Oz-post under the direction of Joe Craig, LWA Programs Operations Director with the assistance of Adam Matrinez, graduate student assistant in Civil Engineering (working under Prof. Walter Gerstle). All the photos are available in a power-point file and the associated document describes the daily schedule and accomplishments.
Monday March 16 - tasks included - clean up ground screens, secure RV, reposition weather station, survey 5 locations.
Tuesday March 17 - more surveying and preparation begun on the junction boxes.
Wednesday March 18 - lots of trenching, modifications to junction boxes, and discovery that hard flexible conduit will work better than the straight conduit sold in sticks.
Measuring the forces required to deviate the posts by some angle. The Oz-Post performed so well that one was installed in an actual antenna location; torsional testing was conducted and determined to be no threat. The mast did not budge.
Thursday March 19 - morning and afternoon spent filling in the trenches with shovels. It was extremely easy to pull cables through the junction box system. The only concern left in the conduit design is whether 28 cables can be pulled easily in the 3" conduit.

More trenching experiments (January 10, 2009)

On January 10, 2009, a new trencher was rented and brought to the LWDA site to make more tests. This trencher is more efficient and able to get through more difficult areas better than the smaller, hand pushed one that we tried during our first attempt in November 2008.

View of the trencher and the first trench made with it.
The trencher can make curved trenches (radius of 32 feet) and intersecting trenches. For the latter, it is necessary to back up to the original trench; one can not cross a trench when making an intersection.

Mobile Workstation (November 2008)

The new mobile workstation is being fitted up for operation at the sites. Thanks to support from the Department of Physics and Astronomy at UNM, there is now a truck available to tow the workstation.

Outside and inside the new LWA Mobile Workstation.
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Trenching (November 2008)

Trenching between the LWDA site and the RTA site (300m away) was carried out on November 22. The previous, above-ground cable had been damaged. The LWDA-RTA interferometer is in continuous use, so replacement of the cable was necessary. But this work also enables us to do some measurements of the effects of dispersion in the cable under the varying environmental conditions, and gives us experience with the equipment and procedures for burying cables.

Making the trench with the trencher; cables from one of the blade antennas goes into the trench.
The trench goes 1,000 feet from the shelter which is seen in the distance to the LWDA Rapid Test Array (RTA). The junction box with its cover plate is shown in the foreground; it is located at 500 feet from the shelter.
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"Brassboard" analog receiver built and tested (September 2008)

The "Brassboard" Analog Receiver for the LWA was designed at UNM by Joe Craig, LWA Systems Engineer. Each receiver board/module contains four independent receive channels. Each channel provides a maximum gain of 80dB, with 60dB of gain control in 2dB steps, spread out over two digital step attenuators which balance the receiver's noise figure against linearity performance. The receiver has a reconfigurable filter bank with three selectable filters; 20 MHz-80 MHz "Full Bandwidth" filter, 28 MHz-54 MHz "Reduced Bandwidth" filter, and a "Split Bandwidth" filter to provide additional independent gain control over the low-frequency portion of the spectrum (diplexer split at 32 MHz). Along with these filters, there is also an "FM Notch" filter to attenuate the FM band. In addition to gain and filtering, the receiver also has an integrated Bias-T for powering the Front-End Electronics (FEE) and control logic for switching on and off the FEE power. The logic interface is standard TTL/CMOS static I/O interfaced over a ribbon cable.

The spectrum shown is 100ms integration of 200MSPS time data, FFT'd with a RBW of 30kHz in the "Full Bandwidth" filter configuration. This data was acquired with the current LWA receive chain at the LWDA/VLA site on Sept. 6th, 2008.
Joe Craig's brassboard analog receiver and the test spectrum.
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5 LWA sites approved (September 3, 2008)

The FEMA CATegorical EXclusion (CATEX) has been signed and filed. This brings the number of LWA sites which have satisfied the Federal environmental permit process to 5 (LWDA + 4 with this action). The completion of the CATEX is a major step forward in the site acquisition.

The accompanying photos shows all 5 sites (as yellow squares) on a partial map of New Mexico and then photos of the individual sites.
 
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LWA Programs Operation Director hired.

Dr. Joe Craig was hired at UNM in February 2008 in the position of Programs Operation Director for the Long Wavelength Array (LWA). Joe is a RF Systems Engineer.
craig We welcome Joe Craig, the new Programs Operation Director, to the LWA Project Team. Joe received his BS in Electrical Engineering from New Mexico Institute of Mining and Technology.
 

Virgina Tech and University of Iowa join the LWA Project in July 2007.

LWA Executive Project Director hired.

Dr. Lee J. Rickard was hired at UNM in April 2007 in the position of Executive Project Director for the Long Wavelength Array (LWA). Lee J. was formerly at the Naval Research Lab, and is a well respected scientist who has published in both ionospheric and astronomical journals. Lee J. will be establishing the LWA Project Office on South Campus at UNM.
The two LWA Directors - Left: Lee J. Rickard, Executive Project Director and Right: Greg Taylor, Scientific Director - at a party celebrating Lee J.'s arrival.
 
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Site Testing for LWA Stations

First overnight RFI testing

The first overnight RFI testing at potential LWA stations took place at the VLA North Arm and Magdelena sites during June 25-27, 2007.
"Campsite" just off the North Arm of the VLA includes a tent, one of the Big Blade antennas plus the new trailer - June 25, 2007.
 
As a member of the team to select sites for the LWA stations, UNM graduate student Frank Schinzel is reviewing maps while data on Radio Frequency Interference are being recorded by computer inside the trailer at a location in the northern part of the Plains of St.Augustine in Socorro County. The signals are picked up by the blade antenna in the front right of the picture.
 
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First RFI Testing of potential sites

Testing for radio interference at potential sites for other LWA stations began in December 2006.
Testing at the Twin Peaks site - located north of US 60 and west of the North arm of the VLA. U-Haul truck with test equipment, big blade antenna infront and power supply equal red item in field to the right. December 15, 2006
 
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Long Wavelength Demonstrator Array LWDA

Welcome to the Construction site

The LWDA is a test bed for the development of the LWA - it is located on the VLA site.

LWDA Interferometer

During the week of May 14, 2007 an LWA team working with Bill Erickson set up an outlier antenna to work with the LWDA as an interferometer. The outlier is the second of the Big Blade antennas currently at the LWDA site (aka BB2) and is located approximately 300 meters due East of the 16 element LWDA. The interferometer allows us to achieve high Signal-to-Noise measurements on many known discrete radio sources. In turn, that allows us to constrain technical characteristics of the LWDA more accurately than previously possible, including accurate flux and phase calibration. The interferometer also brings a new operational mode for targeted source observations, in addition to the current all-sky monitoring and phased array beam-forming modes of the LWDA alone. The LWDA and outlier are remotely configurable between various modes, including with multiple beams, and a number of innovative science programs are being considered to take advantage of these capabilities.
Landscape photo showing the approximate 300 m separation between Big Blade 2 (BB2 - on the left) and the 16 element LWDA (on the right).
SINE and COSINE interferometer fringes on the bright radio source Cas A at 74 MHz. The operational mode employed was a tracking two element interferometer between the outlier Big Blade antenna (BB2) and the phased array LWDA. Each point represents 1 second of data at 1.6 MHz instantaneous bandwidth.

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The Specmaster Data website lets you view Daily Dynamic Spectra and learn about special events from Big Blade at the LWDA site.
Commissioning observations made in October 2006 by the Long Wavelength Demonstrator Array (LWDA) highlight its all sky imaging capability. This 24 hour movie (also available in mpg format) is made at a frequency of 73.8 MHz and shows the full sky as visible from the LWDA site in New Mexico. As the sky rotates, emission from the bright sources Cassiopeia A, Cygnus A, and the Sun, as well as the bright regions of the Galactic Plane, are all clearly visible. The Galactic Center region is marked by the position of the Sagittarius A complex. This movie was made by Tracy Clarke (NRL/Interferometrics Inc) using AIPS to process the observations from the LWDA.
During second half of October 2006 all the hardware was installed at the site, including both polarizations and digital receivers for all the dipoles. Careful phase calibrations were performed and these movies demonstrate how successful they were. Congratulations to all who made this possible.
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Constructing the LWDA

LWDA site - 16 dipoles and electronics trailer (right back) with VLA antennas in the background as photographed in early August 2006.
New large blade antenna for testing (photo - August 2006).
The first results are displayed in power point presentations at URSI and AAS in January 2006.
Construction of the LWDA began at the VLA site during the Autumn 2005.
 
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