With the approach the Universities
Holiday Break it was necessary to shut down the SRT's development
effort until the beginning of the New Year. The
system was rolled from the development laboratory to a near by
storage facility. Figure 9 shows several members of the
team placing the system in the storage facility for a
well deserved rest.
Figure 9 - Placing the SRT System into Storage for the Holiday Season
On January 7th 2009 the SRT was
removed from storage and disassembled in the Embry-Riddle University
development laboratory. The disassembled SRT was moved from ERAU
to a private aircraft hanger at the Spruce Creek Fly-In Community
in Port Orange Florida. This move was made due to a space commitment at
the University and the lack of good sky visibility at the development
laboratory location. The new private hanger facility has
excellent sky visibility and is an ideal location for completing the
calibration and testing of the SRT. The radio telescope reassembled in
the Hanger Test Facility is shown in Figure 10.
Figure 10 - SRT System Reassembled in the Hanger Test Facility
In mid February an arrangement was made
to relocate the SRT from the hanger facility at Spruce Creek to the
Museum of Arts and Sciences in Daytona, Florida. As this will be
the permanent home for the telescope for some time it was decided to
brand the device with the IEEE logo. The logo was made large
enough to be seen from the ground with the antenna section mounted on
top of a twenty foot mast in the museum's courtyard. Figure 11,
shows the Section Secretary Al Jusko applying the logo to the azimuth
gearbox.
Figure 11 - Branding the Daytona IEEE Section's Radio Telescope
With the improved sky visibility at the
new hanger test facility complete testing of the radio telescopes
receiver could take place. Figure 12 shows the SRT on the hanger
apron
during receiver tracking testing. It should be noted that
height of the antenna pedestal was shortened so that the SRT could be
more easily moved in and out of the hanger space.
Figure 12 - SRT System on the Apron of
the Test Facility Hanger during
Initial Receiver Testing
On February 17th the SRT was
disassembled and loaded into a rental truck for the trip from the
aircraft hanger facility at Spruce Creek to the Daytona Museum of Arts
and Sciences. Figure 13 shows the Dayton IEEE Section moving team
unloading the disassembled small radio telescope into the courtyard
behind the planetarium at the Daytona Museum of Arts and Sciences
(MOAS). Dr Liu and Tracy Wichmann lift the parabolic reflector from
the truck while John Harris and Roger Grubic balance the dish above
their heads.
Figure 13 - Unloading the Disassembled SRT at the Daytona Museum of
Arts and Sciences
The Small Radio Telescope was then reassembled in the courtyard at the
Daytona Museum of Arts and Sciences. Figure 14 shows Dr. Liu
reattaching
the parabolic reflector to the azimuth drive assembly after its truck
journey from the Spruce Creek Hanger Facility. Roger Grubic operates in
the foreground with John Harris observing in the background.
<>
Figure 14 - Shows the Reassemble of the SRO at the Daytona Museum of
Arts and Sciences
The reassembled SRT was tested
and
found to have made the journey from Spruce Creek with no ill
effects. Figure 15 shows the SRT reassembled in the Courtyard at
the Daytona Museum of Arts and Sciences. Note the unused L Band
satellite Dish also shown in this photograph. After additional
testing of the SRO the L Band Satellite Dish is scheduled to be removed
from its 20 foot mast and the SRT will be lifted into its place.

Figure 15 - The Small
Radio Telescope Reassembled in the Courtyard at the
Daytona Museum of Arts and Sciences
On
February 21st, 2009 a reception was held at the Halifax River Yacht
Club in Daytona Beach for a representative group of the IEEE Life
Members Committee. These members, from throughout the United
States and a
number of foreign countries, had been holding their meeting in Orlando
Florida.
As this group was responsible for funding the SRT project they took
time from their meetings in Orlando to visit the Daytona Section to see
the the radio telescope. Figure 16 shows the gathering of the Life
Members Committee at the Halifax River Yacht Club prior to the
technical
presentations on the SRT and luncheon.

Figure 16 - A
gathering of Life Members Committee at the Halifax River Yacht Club
to discuss the Small Radio Telescope Program
The first item on the agenda was a
welcome to the Dayton Section from Roger Grubby current Section
Chairman. A presentation by Charlie Husbands, the SRT Project
Leader, consisted of a brief lecture on Radio Astronomy, the
development and characteristics of the SRT system, and a history of the
acquisition and construction of the Daytona's SRT device. Tracy
Whitman, the Section
Treasurer, then gave an accounting of the funds spent on the project to
date. Dr. Hugh Ward the Education Director on the
project then explained the proposed steps necessary to integrate the
SRT into the museum's planetarium program and in the future to permit
remote access to the telescope for education and research applications.

Figure 16 - A
Presentation on the SRT given to the Life Members Committee at the
Halifax River
Yacht Club
After
the series of presentations, a luncheon buffet was set up at the
Halifax
River Yacht Club for the attending Life Members. During the
luncheon a
simulation of the operation of the SRT was presented, demonstrating the
displays and controls necessary to select a radio sources, calibrate
the telescope, track an object, record the received data and reduce
the data into useable form.

Figure 16 - Luncheon
Buffet for the Life Members Committee at the Halifax River Yacht Club
After
the luncheon the Life Members Committee group was transported to the
Daytona
Museum of Arts and Sciences. Figure 17 shows the Life Members
gathering in the courtyard behind the museum where the SRT is
temporarily housed.

Figure 17 - Gathering
of the Life Members Committee in the courtyard behind the
Daytona Museum of Arts and Sciences
As a
demonstration the operation of the SRT, the Sun was selected as
the
object to be tracked. Figure 18 shows the Life Members Committee
gathered
in the courtyard of the Daytona Museum of Arts and Sciences watching
the radio telescope track the Sun.

Figure 17 - The Life
Members Committee in the courtyard behind the
Daytona Museum of Arts and Sciences watching the SRT track the Sun
At
the conclusion of the demonstration a number of the members had
specific questions on the construction and operation of the Small Radio
Telescope. Figure 18 shows Dr. Ward in the dark hat, who is the
Educational Director, on the SRT Project answer specific
questions about the telescope.

Figure 18 - Dr. Ward
answering questions on the operation and construction
of the SRT with a group of visiting Life Members
On
March 19th, 2009 a work party was put together to change out the
parabolic reflector on the SRT. Dr. Hugh Ward had provided the
Daytona Section with a 10 foot parabolic dish, in wonderful condition,
to allow us to improve the sensitivity of the existing SRT.
Figure 19 shows Al Jusko assembling, in the background, the
four segments of the new 10 foot dish. The existing 7.5 foot
dish, with the subreflector electronics still attached, is shown
in the foreground. The change out of the parabolic reflectors was done
in the courtyard of the Daytona Museum of Arts and Sciences.

Figure
19 - The Removal of the 7.5 Foot Parabolic Reflector and the Assembly
of the 10 Foot Parabolic Reflector
The 10 foot parabolic reflector was
assembled and then lifted into the halo assembly ring on the SRT.
The new reflector fit exactly into the the brackets on the halo ring
and all of the bolt holes used to hold the 7.5 foot reflector could be
used without any modifications. Figure 20 shows the SRT with the
new 10 foot parabolic reflector securely mounted in the halo assembly
of the SRT. The 7.5 foot parabolic dish with the subreflector still
attached is shown in the background.
Figure
20 - The SRT with the new 10 foot parabolic dish bolted into the halo
ring.
After
securing the new 10 foot parabolic dish onto the SRT the subreflector
assembly was removed from the old configuration and mounted, with new
stand-off rods to the new parabolic reflector. Figure 21 shows Dr. Liu
and Al Jusko adjusting the subreflector assembly on the new SRT
configuration. Part of the alignment process requires carefully
adjusting the subreflector focus point for the new reflector
configuration.

Figure 21 - Al Jusko
and Dr. Liu adjusting the focal distance from the subreflector
to the main reflector in the new configuration
With
the installation of the new 10 foot parabolic reflector completed the
SRT was run through as series of test to determine its operational
capability. Figure 22 shows the initial Sun tracking test
required to adjust for antenna alignment and determine the systems
mechanical performance. The installation of the new reflector
will markedly increase the sensitivity of the SRT system.

Figure
22 - The SRT shown during Initial Sun Tracking Tests with the
newly installed 10 foot Parabolic Reflector
On
1 April 2009 the SRT was moved from the courtyard of the Daytona Museum
of Art and Science to a 20 foot mast. The mast was currently
occupied by a 10 foot "L" band satellite dish. Figure 23 shows
two workman from Advanced Cable removing the "L" band parabolic dish
from the antenna mast.

Figure
23 - Removing the "L" Band Satellite Dish from the Antenna Mast
A
bucket truck, provided by Advanced Cable, was used to move the SRT from
the ground to the mast. Figure 24 shows the lifting arm of the
bucket truck positioned over the center of gravity of the SRT. In this
photo it can be seen that the bucket truck has just lifted the
SRT free of the ground pedestal.

Figure
24 - Lifting the SRT free of the Ground Pedestal
The
SRT was then moved from the courtyard toward the mast.
Figure 25 shows the SRT being transported to the antenna mast end of
the courtyard using the bucket truck.

Figure
25 - Moving the SRT from the Pedestal toward the Roof Mast
With
the help of the bucket truck the SRT is lifted to the roof the the
Daytona Museum of Arts and Sciences. Figure 26 shows the SRT
being guided onto the satellite mast.
Figure 26 - The SRT is being guided to the mast on the roof of the
Daytona Museum of Arts and Sciences
With the Small Radio Telescope on the
mast, it was aligned and secured. The cables were then dressed
and strapped down to permit proper operation from the ground.
Figure 27 shows the SRT after the installation process on the roof had
been completed.
Figure 27 - The Small Radio Telescope Installed on the roof of the
Daytona Museum of Arts and Sciences.
With the SRT Antenna Installed on the
roof the Daytona Museum of Arts and Sciences it was necessary to
connect it to the SRT controller and control computer in the
Planetarium. Figure 28 shows Al Jusko installing PVC conduit in
the overhang between the SRT antenna and the Planetarium at the Daytona
Museum of Arts and Sciences.
Figure 28 - Installing Conduit to carry the SRT Control and Data Cables
under the Overhang at the Daytona Museum of Arts and Science
Figure 29 shows Al Jusko connecting
the final segments of the conduit on the rear wall of the Daytona
Museum of Arts and Sciences. The nine conductor control cable and
the coaxial cable required to interface with the SRT is shown extending
for the conduit under construction.
Figure 29 - Al Jusko working on the final segment of the Outside
Conduit and SRT Control and Data Cables
The final segments of the control
conduit are shown in Figure 30. At this point the control cable
and coaxial cable pass through the exterior wall of the
planetarium at the Daytona Museum of Arts and Sciences.

Figure
30 - The Control Cable Conduits where they enter the wall of the
Planetarium
Because
of limitations on the length of the cabling between the SRT Antenna and
SRT Control Box it was necessary to install the Control Box at site
just inside the rear wall of the planetarium. Figure 31 shows the
SRT Control Box on the extreme right of the hardware on the
shelf. In this configuration the laptop computer is connected to
the SRT Control Box with a short piece of RS 232 cable. With this
configuration we were able to run a series of test with the radio
telescope to confirm that the installation to this point was working
correctly.

Figure
31 - Final Position of the SRT Controller and Temporary
Laptop Computer Test Station
In the final configuration a desktop
computer will be used to control the SRT system from the Control
Console position of the Planetarium. To interconnect the
Control Box to the Control Console position it was necessary to run
approximately 100 feet of RS 232 cabling through the access space in
the ceiling of the planetarium. Figure 32 shows Al Jusko and Dr.
Hugh Ward working the cable through the ceiling access space around the
planetarium's projection equipment.

Figure
32 - Installing the final cabling in the ceiling of the MOAS
Planetarium
from the SRT Controller to the Computer Control Station
With
the RS 232 link connecting the SRT controller to the SRT Computer
Facility the Planetarium installation was completed. Figure 33
shows the SRT Computer System integrated into the Planetariums display
racks. From this point the computer can control the SRT antenna
system and display the graphical results on the planetariums overhead
projection system.

Figure 33 - The SRT Control Facility integrated into the Planetariums
display facility
In Mid May 2009 a tropical depression
dumped up to 24 inches of rain on the Daytona Area. One of wings
of the museum of the Daytona Museum of Arts and Science suffered
flooding which resulted in extensive water damage. The entire
museum was closed for a month and 60 percent of the facility was able
to reopen on 15 June 2009. The wing of the museum that was not
able to reopen was the one containing the planetarium. Figure 34
shows the state of planetarium following the flooding. The seats
have been removed and the planetarium machine stands watch in the empty
wing of the museum.

Figure
34 - The Planetarium Machine stands in an empty Planetarium
after the May flooding destroyed that wing of the Museum
When the museum reopened a decision
was made to operate a version of the planetarium show in the
auditorium.
until the planetarium could be restored to its former condition.
The Daytona IEEE Section decided to approach the museum about
installing a wireless Ethernet Link between the SRT Control Computer in
the the planetarium and a remote computer in the projection booth of
the
auditorium. To remotely control the SRT computer in the
planetarium UVNC software was obtained, installed and tested in a
pair
of computers to demonstrate this remote control and display
capability. Figure 35 shows Dr. Liu running a series of test on
the remote software system, chosen for this application, using
two computers interconnected over an Ethernet link.
Figure
35 - Dr. Liu testing the remote control computer software for remoting
control of the SRT from the Museum's Auditorium
To interconnect the SRT Computer and
the Remote Control Computer in the MOAS Auditorium required the
installation of a special wireless Ethernet link. A Memorandum of
Understanding was formulated and signed by the responsible MOAS
and Daytona IEEE personnel to permit the installation of this
link. The first portion of the link's installation involved
pulling a 100 foot
terminated CAT5 Ethernet cable from the control console position in the
planetarium to a wiring closet in the office space of the damaged
museum wing. Figure 36 shows Al Jusko examining the Ethernet
cable at the wiring closet end of the cabled portion of the link.
Figure 36 - Al Jusko examining the Ethernet Link from the Planetarium
Console Position to the wiring closet in the damaged museum wing.
A high gain router was then installed
in the wiring closet and connected to the SRT Control Computer through
the cabled portion of
Ethernet link. Because of the thickness of the walls and
the number of galleries in the Planetarium Wing of the museum the
output power of the selected router was unable to reach the Museum
Auditorium without signal regeneration.
Figure 37 - The Hawkings 300N Router installed in the
wiring closet in the damaged wing of the museum
To
close the wireless Ethernet link from the planetarium to the auditorium
required a
regeneration facility. Figure 38 shows a portion of the
information desk in the mail lobby of the Daytona Museum of Arts and
Sciences. Installed under this desk is a 16 dB gain corner reflector to
communicate with the router in the wiring closet in the planetarium
wing. The high gain antenna is interfaced to a wireless Ethernet
range extender
unit. This unit increased the signal gain sufficiently to close
the wireless link
between the planetarium's wiring closet and the auditorium's
projection booth.

Figure
38 - A portion of the Information Desk in the Daytona Museum of
Arts and Science
containing the range extender unit and corner reflector necessary to
close the wireless Ethernet link
The
auditorium end of the wireless Ethernet link was installed in the
auditorium's projection booth. This end of the link is supported
by a desktop computer operating with UVNC software. With
this software the operator can view the display on the SRT control
computer in the planetarium and remotely operate the SRT hardware and
software. From this station the computer display can be patched into
the auditorium's digital projector system. Figure 39 shows the
SRT remote computer hardware installed in the auditorium's projection
booth.

Figure
39 - The remote control station in the Museum's Auditorium's projection
booth
for operating the SRT in the Planetarium.
In early 2010 the Executive Committee of
the Daytona Section requested that work begin on providing remote
connectivity so that the SRT can be operated over the World Wide
Web. This capability would allow the SRT to made available to a
number of schools and educational institutions for instructional and
research purposes. The diagram in Figure 40 shows the components
and connectivity required to implement the remoting capability.
Figure
39 - A diagram of the components and connectivity required
to provide remote connectivity to the SRT
In Figure 40 the dark yellow boxes
are
components that were added to the Planetarium configuration of the SRT
to allow remote operation. It was decided to set up a Wireless
Ethernet Link to the SRT system as an alternative to using the museum's
existing internet
network. This was done to isolate the two system for
administrative
purposes and provide a designated Static IP for the exclusive use of
the SRT system. We chose to use the Clearwire provider for this
purpose. The SRT system does not require high uplink and downlink data
rate connectivity for remoting purposes. Figure 41 shows the
Clearwire modem mounted in a transparent frame installed high in a
window of the office area of the Planetarium Wing of the museum.
Figure 41 - The Clearwire Ethernet Modem installed in a window of the
Planetarium Wing of the museum
The Clearwire modem is interconnected to
the SRT computer through a ethernet router. The router acts as a
major mode in the network configuration allowing the SRT computer to
communicate with the outside world by way of the wireless modem,
provide remote control power control to the SRT's receiver and antenna
controller, and provides connectivity to the Ethernet webcam mounted on
the roof of the planetarium. Figure 42 shows the router used in
the SRT system layout.
Figure 42 - The network router installed in the SRT equipment rack
In order to provide remote power control
an "iboot" remote power controller was procured. The "iboot"
operates
under computer control from the SRT computer by way of the router,
through Cat5 cabling. The power controllers task is to power on
or off the SRT receiver and antenna control motors under computer
control. When the remote viewer gains control of the SRT computer he
uses an icon on the desktop to switch "on" power to the SRT receiver
and antenna electronics. At the end of the remote session the
user returns to the desktop and turns "off" power to the SRT receiver
and antenna electronics. Figure 43 shows the "iboot" interfaced
to the SRT receiver.
Figure 43 - The "iboot" Remote Power Controller supporting the
SRT Antenna
Driver System and Receiver.
The last piece of hardware controlled by the SRT computer via the
router is the web cam mounted on the roof of the Planetarium
building. The Webcam is used to monitor the movements of the
antenna structure during movements of the SRT antenna structure.
The Webcam is mounted on the outside wall of the Planetarium and
receives
control signal and transmits digitized video over a Cat5 cable that
interconnects it to the SRT
router. Power is furnished to the Webcam through the Cat5
cable. Because the SRT antenna structure can not been seen from
the Control Rack
in the Planetarium or by a remote operator over the internet the Webcam
permits the user to visually verify the commanded movements of
the SRT dish. Figure 44 shows the camera in its protected
shield mounted on the exterior wall of the Planetarium.
Figure 44 - Webcam Mounted on the Exterior to Monitor Physical
Position of the SRT Antenna Structure
To support the SRT operations during
periods of darkness it became necessary to light the SRT antenna
structure. Adequate lighting is necessary to monitor the movements of
the antenna
structure through the web camera to avoid potential mechanical
problems. With the antenna structure illuminated the SRT can be
operated remotely around the clock. To
accomplish this task a 400 watt halide floodlight was installed on the
exterior wall of the planetarium. Figure 45 shows the electrical
contractor boring a hole in the exterior wall of the planetarium prior
to installing the flood lamp.
Figure 45 - The Electrical Contractor boring the hole for the
floodlight wiring
through the exterior wall of the Planetarium
Cabling was run from the newly installed
electrical box on
the roof , through the exterior wall of the planetarium, to an
electrical control box in the planetarium. Figure 46
shows the electrical contractors mounting the halide floodlight fixture
on the exterior wall of the planetarium aimed, across the roof,
at the SRT antenna
structure.
Figure 46 - Mounting the Floodlight fixture on the Exterior Wall of the
Planetarium
A picture of the halide
flood lamp installed to light the SRT structure, during hours of
darkness, is
shown in Figure 47. The flood lamp installation is shown on the
left, connected through the electrical box in the center, to the
lighting control position in the planetarium. Also shown, to the
right, on this photograph is webcam in its associated rain shield.
Figure 47 - The completed Halide Flood lamp installation on the
exterior wall of the Planetarium