Installing the 1296 MHz feed for Autumn Moon Bounce Communications

Text and photos by Gary Agranat.

A DSES team worked at the Plishner Radio Telescope site in Haswell on Sunday September 27, 2o2o. Team members were Ray Uberecken, Floyd Glick, and Gary Agranat. We accomplished the main objective, to install a new 1296 MHz feed at the focus of the 60 dish antenna. We also installed a mast in the ground, on which will later be added a Hughes Internet satellite antenna. Two friends of Ray’s came out and did an immense service by using metal detectors and magnetic rollers to clear nails and other metallic debris on the site. We changed out two of the locks. And we inspected the bunker.

Mast for Hughes Internet antenna

Ray and I met at the Plishner site at 0930 in the morning. 

We first installed a sturdy pipe mast behind the operations trailer, on which will be mounted a small satellite antenna to access the Hughes network geosynchronous satellite for Internet access.  Ray chose a spot that will not be blocked by the trailer or the 60-foot antenna.  We mixed cement and set the pole in its hole with the cement, using a level to check that the mast is vertical.

Moon Bounce (EME) Preparation

After that we manually rotated the 60-foot dish antenna to the service platform. I figured out, with Ray’s help and the checklists, how to use the software to monitor the antenna pointing. (Note: we might want to add a checklist just for this type of procedure, for using the software for just manual antenna pointing, as when we service the antenna.)

Floyd came out to the site by 1030. Ray and Floyd climbed the service platform. I worked on the ground to move feeds and tools up and down to them. We replaced the 408 MHz feed at the antenna focus with the newly built 1296 MHz feed. The 1296 MHz feed was built by KL6M, to specifications provided by Steve Plock (KL7IZW). The feed mount at the dish focus was designed by Ray, to enable the feed to more easily rotate out and be changed.

Conditions were somewhat windy, with a cold front coming, but still manageable. By the afternoon the winds had picked up enough that we postponed any further work at the feed. Work that still needs completion is installation of a 200 Watt amplifier at the feed. Since we are planning to operate at 1296 MHz from the Operations Trailer, which has a long coax hard line path to the pedestal and antenna feed, we expect significant power loss from the long path. We therefore need to boost the power again at the feed. We plan to install the amplifier the next weekend. We then also intend to test our setup by trying tropospheric scatter communications to the north.

We are planning to use this configuration to operate EME (Earth Moon Earth) Moon Bounce communications. And specifically we plan to participate in the ARRL EME contests on October 10-11, 2020 and on November 28-29, 2020 (UTC).

We discussed our plans for the upcoming contest in 2 weekends. The Moon then will be at last quarter phase. What that means is that it will rise on Friday night a little before midnight (about 1130 PM), and set Saturday a little after 2 PM. That means we will prepare to do overnight and morning operations. After the Moon rises we will try to pick up the ON0EME beacon in Belgium. We can try to contact across the Atlantic Ocean. The US East Coast will be in night time conditions, and so we anticipate less contacts to there. Daytime conditions, when more hams would be awake, are more favorable for the US West Coast, and across the Pacific Ocean to Oceana, Asia, and Australia.

Note that the 60-foot antenna will be configured with the 1296 MHz feed through the end of November. This will be an opportunity to try using it for other 1296 MHz communications, including troposphere scatter.  

Metal souring of the site

A friend of Ray’s who works at Planet Granite Ryan, and his brother, Rob, came out to the site also.  They have ground metal detectors and magnets on rollers, and systematically paced across the site to pick up nails and other small metallic debris.  They did pick up lots of nails, including along the roadway. They spent a few hours with us, and left after lunch. They did us a great service by helping remove a lot of this debris.

Combination Lock and Bunker Inspection

We attempted to open the combination locks at the gate, the bunker, and the generator shack. After still having difficulty, we replaced the locks at the gate and bunker, with the locks Myron Babcock obtained for us. These are similar model locks, and the combinations were kept the same.

We had a report that the bunker had been flooded by two successive rain storms in July. We opened and inspected the bunker. The bunker was dry, though the floor had more-than-normal dust and dirt, and some tiny debris was spread here and there. It will require a fresh cleanup before normal use. We saw no indication of mold from dampness.

Tumbleweeds were accumulated again at the ramp entrance.

We completed our activities by early afternoon, about 3 PM.

For the team, – Gary

We kept the antenna steering in manual configuration. We opened the System 1 steering software to monitor the position angles as we manually steered the antenna to the service platform.
We noted this radio interference at the site on our scope. This scan is from 0 to 1.8 GHz. The higher floor noise level at the left is from the sensitivity of our 408 MHz feed, which was still on the dish antenna, before we changed it out.
The 60-foot antenna is positioned for service.
Ray brought two feeds for the 60-foot antenna. This is Ray showing Floyd the 4 GHz feed, which we will use in the future, to calibrate the pointing position with geosynchronous satellites.
Floyd carrying the 1296 MHz feed to the antenna for installation.
The inside of the 1296 MHz feed. It is designed as a septum feed, with separate channels on each side for left and right circular polarization.
Rob with a metal detector, crisscrossing the site, picking up small metal debris.
Ray and Floyd on the 60-foot antenna service platform, starting work.
Removing the cover.
Ray is disconnecting the 408 MHz feed, so that it can rotate down and out for changeout.
The 408 MHz feed is now rotated down. It is connected simply by the shaft to the mount, for easier changeout.
Installing now the 1296 MHz feed. Its design doesn’t use a shaft, but instead will be securely fastened to the mounting frame.
Ryan using a metal detector on the west side of the site.
Our view towards the west. High clouds in the distance are an indication of a cold front gradually coming this way. We experienced steady windy conditions as the front approached..
Closing up.
Our view of Haswell in the distance. The clouds from the front were getting closer. By the time we left in mid-afternoon, the clouds were over us, but we had no precipitation.
The 1296 MHz feed installed.
We installed this ground mast. It will mount a small satellite antenna, to connect to the Hughes Internet network.

New work area in the science trailer, built by Bob Haggart

Bob Haggart (N0CTV) has been steadily improving the workspace of the science trailer at the Plishner radio telescope site. During the pulsar observation work on May 2, 2020, he completed building his latest enhancement: a partitioned work space at the east side of the science trailer. There is desktop space, which can be used for electronics building and testing. And there is additional shelf space, for better organization and storage.

Thank you Bob!

The new partitioned work area, seen from the middle of the science trailer.
New desktop workspace, with room for building and testing. There is also close access to test equipment, references, and technical documentation.
The work space in use during the pulsar observations on May 2, 2020.

Antenna Raising

Plishner Antenna Site Work Trip Report. By Gary Agranat. Photos by Steve Plock.

Ed Corn, Steve Plock, and Gary Agranat traveled to the Plishner antenna site in Haswell this past Saturday, October 19, 2019. The team completed erecting the 50-foot ham radio tower.

Completing the tower erection involved several tasks:

  • Installing the 3-band/3-element Yagi HF ham antenna,
  • Installing the 2-meter band vertical antenna on top of that mast. This will be our new antenna for our VHF talk-in radio system.
  • Installing two stand-off bracketed supports near the top of the tower on the sides, to raise and hold the 80 meter band and 160 meter band dipole wire antennas. This arrangement replaces the long pole that previously centrally supported those wire antennas. These bracket supports each have a pulley and rope, to raise and lower the wire antennas. The tower also supports a 6-meter band delta-loop antenna, which is simply tied from height.
  • Securing the coax cables for the Yagi and vertical antennas along the side of the tower.
  • Properly arranging the system of wires, coaxes, and support cables.
  • Raising the 50-foot tower, which involves turning the winch system that rotates the tower up from its pivot plate at its base. The 50-foot tower is raised from a pulley system on a second smaller adjacent tower.
  • Once the 50-foot tower is raised, securing 3 guy cables.
Steve took this photo of Ed and Gary at the completion of the tower raising.

Steve tested the SWR of the 3-band Yagi antenna with an analyzer. The antenna elements had been measured and assembled on a previous trip, to be optimized for the middle of each of the operating bands, of the 10, 15 and 20 meter bands. Steve measured an SWR ratio of 1:1 (perfect) at 28.51 MHz for the 10 meter band, and 1:1 at 21.19 MHz for the 15 meter band. The 20 meter band resonated with an SWR of 1:1.35 at 14.16 MHz. This is excellent, and as expected.

For lunch, Steve treated us with smoked ribs from Broken Bones BBQ in Monument, with sauces, potato salad, and coleslaw. Gary brewed coffee. Also, the team met first at the firehouse in Ellicott. Gary baked orange-cranberry muffins. We ate our muffins at the firehouse, and shared the rest with the fire department crews there.

The team left the Plishner site by 4:30 pm.

The tower work began about a year ago. The work involved support and efforts by a number of team members. See our past posts from October 19-21, 2018 http://dses.science/plishner-site-report-for-the-weekend-of-october-19-21-2018, August 24, 2019 http://dses.science/plishner-work-trip-report-august-24-2019, and September 28, 2019 http://dses.science/work-site-trip-report-at-the-haswell-plishner-radio-telescope-site-september-28-2019.

The tower should significantly improve our capability to communicate long distances on the 10, 15, and 20 meter bands with the Yagi. The 2 meter band vertical should enable us to communicate on our talk-in VHF radio system to much further out.

Work Site Trip Report, at the Haswell Plishner Radio Telescope Site, September 28, 2019

by Gary Agranat

DSES Participants: Gary Agranat, Ed Corn, Bob Haggard, Bill Miller, Steve Plock.

Ed, Gary, and Bill met first at the Ellicott Fire Department, while Steve and Bob each traveled ahead solo. Ed encountered a problem with his truck and had to return home, but he passed the tower antenna mast and connector supplies to Bill. Steve and Bob arrived at the site by 9 AM, and Bill and Gary arrived by 10 AM.

We encountered light drizzling rain and low clouds on the route to the site, but the rain let up once we were on Highway 96 past Ordway. Steve called Ed to let us know the weather was good at the site. The weather completely cleared later, while the temperature remained comfortable.

Steve coordinated by phone with Skip Crilly and commenced a 48-hour long SETI drift scan at -7.5 degrees declination, run simultaneously with Skip’s antenna in New Hampshire. The 48 hour run will scan the -7.5 degree declination band twice, and therefore acquire a repeat set of data that can be compared with the first set.

Bob worked at the Communications Trailer, doing carpentry and painting work. He built a wood frame seal around one of the air conditioners, fabricated and painted a seal for the solar-powered fan, and painted the third work table he had added previously. Bob told me the trailer back door hadn’t been sealing — until recently — because it actually had not been closed properly. He closed the door properly and it is now sealed, without requiring further work.

Bob at work.

Bill, Steve, and Gary worked on preparing the 50-foot ham radio antenna tower.

Bill spliced the controller feed cable and wires for the antenna rotator, and verified proper operation, with some assistance from Gary. Bill used Steve’s crimping tools. The three of us then fed the controller cable through the dog house to the tower.

Bill first checked online for the correct color code standards for the control cable wiring. Then he matched the correct colored wires from the cable to the wires on the rotator. After the wiring was completed, the rotator and controller were tested for correct operation and correct meter calibration.

At the tower outside, the rotator was attached to its base plate, and that assembly was then attached to the tower.

When we tried to fit the mast in the holding tube at the top of the tower, we found that top opening was slightly damaged, and the mast wouldn’t fit in. We then took turns filing and grinding out the hole until the mast did fit properly. Steve applied a lubricating grease, to mitigate against the mast binding stuck when rotating. Eventually we successfully installed the mast to the rotator itself. We also retrieved a guy wire cable left at the communications trailer and attached it as the third guy wire connection for the top of the tower.

Bill with Steve, filing out the top opening for the mast. You can see two of the three guy cables already attached to the top of the tower.
Steve
Gary
Bill and Steve fitting the mast at the tower top. The mast was then securely fastened to the rotator.
The 60 foot antenna positions at 39.5 degrees elevation for the 48-hour SETI run, in progress.

Before we left for the day, we had two visitors from Eads come to look at the site. We all spent a little while talking about the site and the work.

Addendum

By Gary Agranat

Bob was the first to leave, then Steve. Steve said he would check on Ed on the way home. Bill and I (Gary) convoyed out last.

While Bill and I were driving back to Colorado Springs, about an hour and a half into the trip back, an auto accident happened right in front of us, with a vehicle overturning.

The accident happened while we were driving westbound on Colorado Highway 94. It was early evening by then, about 5:30 pm, and the sun appeared above in the western sky. Bill and I had been talking on the VHF ham radio during our 2 1/2 hour drive back from the site. Bill was driving ahead of me.

A couple of miles before Rush, I saw three vehicles approaching from a long distance behind, moving faster than Bill and me, while we were going at about the speed limit. I mentioned the vehicles to Bill, and we stopped talking, anticipating they would choose to pass us soon. They did soon pass us, all three staying close to each other. We could see they were some sort of laborers, with equipment filling their vehicles and with ladders on top. The third vehicle passed us as we were going up a hill, with the solid yellow line on our side. Bill commented that car was taking risks, although they all were driving in a risky manner. There was no visibility over that hill. And furthermore we were driving into the sun. A couple of miles later we reached the town of Rush, where the speed limit lowers from 65 to 50 mph. As those three vehicles ahead approached the town, I suddenly saw the last one veer to the left side of the road, and then roll over, with its front turned facing the opposite direction. Bill and I both stopped, as did a driver heading in the oncoming direction who almost got hit. And several more cars stopped briefly. We saw one occupant lie in the grass, but he eventually got up.

Bill had a better view of the accident ahead of me. It looked to him like one of the three vehicles ahead suddenly slowed as he reached the town with the lower speed limit. The sun was right above and ahead of us, which created a greater visibility challenge. The sudden slowing apparently caught the last driver off guard, as he swerved to the right to avoid the vehicle ahead of him. But that put his right side of his car in the grass there, which caused a tire blowout and a swerve then to the left. And he overturned.

The volunteer fire department nearby responded relatively quickly. But we waited about 2 hours for a sheriff’s deputy to arrive, and then another hour for a State Patrol officer to arrive. The State Patrol was who we had to give our witness statements to. We didn’t finish with that until 8:30 pm, and I didn’t get home until 9:30.

The driver of the overturned vehicle eventually got up, but he refused medical help, although we wondered if he nonetheless might have been hurt.

Meanwhile the communities there are small, and everyone there knows everyone else. The other driver who stayed was a local woman school teacher. We chatted with her and also the volunteer firefighters, and with some of the neighbors who stopped to see if everyone was OK.

The State Patrol officer later explained to us that there were 6 accidents in the region called in within a period of 5 minutes, when our accident happened. One happened just about 9 miles further west from us on Highway 94, in the town of Yoder. That accident had injuries, and some of the firefighters who were with us then had to leave to respond to the other accident.

At a minimum, this is a reminder to take care to drive safely, especially with limiting conditions like the sun setting ahead.

Haswell Site Trip Report for December 14-16, 2018

Personnel present – Bill Miller, Ed Johnson, Steve Plock, Ed Corn, Myron Babcock, Bob Haggard, Glenn Davis, Phil Gage, Hans Gaensbauer, Rich Russel.
Rich Russel and Bob Haggard showed up Friday, joined later that day by Hans Gaensbauer. All three spent the night and Rich did radio astronomy observations. Bob  Haggard finished the new front stairs for the communications trailer. Thanks Bob they look great! Everyone else came the next day. Glenn Davis and Phil Gage upgraded the software on pointing System 1, and Glenn installed the NTP server as well. Bill Miller and Ed Johnson were able to demonstrate go-to functionality on System 2 and the PID algorithm employed operated flawlessly. A milestone has been achieved and Ed plans to attempt sidereal tracking as his next step. Congratulations to all members of both pointing teams!
 The fireproof door for the bunker hallway was cut to size by Steve Plock, Myron Babcock and Hans Gaensbauer. Ed Corn continued with electrical buildout in the bunker.
 Again many thanks to all who participated and worked in the spirit of friendship and cooperation.
submitted by: Steve Plock, President DSES

Bob Haggart’s work building a new porch and stairway for the communications trailer

Bob Haggart N0CTV is working on building a new stairway and porch to the communications trailer at the radio telescope site.  He started the work at home after taking measurements. Today he traveled to the site to continue the work.  With him were his grandson Allen and Allen’s friend Ben. Bob writes:

“We arrived at 11 AM. Worked on the porch and covered the fan with 24″ X 24″ plywood. Ran out of time but did get the porch assembled and painted inside and out. The hand railing is only temporary and will finish next work day on the 17th.”

Bob’s work is replacing a small simple set of metal steps that has given us access to the communications trailer.

The original set of steps to the communications trailer. Bob’s new porch and stairway is replacing this.

The new porch and stairway provide a great improvement.

Bobs has built this new porch and stairway. It is larger, sturdier, and gives much better support. The handrail is temporary. The permanent handrail is planned to be installed on the next group work trip on Nov. 17.

Bob Haggard N0CTV, standing with his work.

Thanks to Bob for all this work, and for improving the access to the communications trailer.

DSES Science Meeting, October 22, 2018

DSES Science Meeting 10-22-2018                   Meeting Notes by Bill Miller

Location Rich Russel’s Residence, Colorado Springs

Attendance:   Gary Agranat, Ed Corn, Floyd Glick, Glenn Davis, Steve Plock, Rich Russel, Tony Bigbee, Ray Uberecken, Dave Molter, Jon Richardson, Bill Miller

Attending Remotely via TeamViewer:   Skip Crilly, Dayton Jones, Jamie Riggs

Last Trips: Oct 19 Observation Trip. Oct 20 Work trip for ED. Steve, Hans, Gary, Paul

Next Trips to site:  The regularly scheduled 3rd Saturday of the month, Saturday Nov 17th.  Observation the night before on Nov 16th

Meeting Schedule: 

  • DSES Technical and Operations Meeting- 2nd Monday of Every Month
  • DSES Science Meeting – 4th Monday of Every Month

Accuracy:  The notes for this meeting may be out of order.  This was done to group the discussion into subjects for better clarity and continuity, so they are not true chronological minutes.  As always if I have misstated, omitted or misrepresented anyone please feel free to correct me WKM.

Agenda and Notes

Ray Uberecken has his mount ready to install a 12 ft dish with capability up thru the KU band. He needs to move the dish from the KCME radio station to his site in Payton.  The dish F/D ratio is the same as the 60 ft Haswell dish, so the 12 ft dish could be used to prototype feeds and receivers for the Plishner site.  Ray would like some volunteers from the DSES to help move it next Sunday the 28th at 10AM.  (Note: Recent change of plans.  Ray will hire a crane to pick the dish out of the KCME yard enclosure before disassembly.  This is currently scheduled for 7 AM Saturday, November 10th.) He could use some volunteers,  power drills with sockets and a trailer.  KCME is at Fontanero and 1921 N. Weber in.  Bill will send an EMAIL out to the group.

Once the dish is in place the first thing that Ray will install is a Dicke Switch.

Ray also wants to know if we want to use the 8 channel UHF remote at the site for reset and control of the systems.  We have not been using it, but that is available and installed in the communications trailer rack and can be commanded remotely from Ray’s residence.

Ray has also started his optical observatory with 8 inch Celestron and a good refractor at his residence.

 

Dr. Rich Russel reviewed his new Radio Astronomy Guide Rev. 3.

The RA/Dec of many of the objects are from both celestial coordinate year 1950 epoch and year 2000 epoch, so needs updating.

The output of the SpectraCyber is in volts and a translation to Jansky is needed. 

Rich and Gary observed a number of sources on the Oct. 19th observation trip.

Some source positions were very good.  Others were not.  This may indicate a pointing error or other system issue.

They were getting a lot of clear source signatures but don’t know what many of them were.  Rich would like to do cross galactic scans while changing declination to map the whole area in the future.

Cassiopeia A, Cas-A, was thought to be seen, but at a relatively low amplitude. Cas-A, being a 2200 Jy source it should have been clearly seen but they weren’t sure they had it.

Sagittarius A was strong and had the instrument setup with too high of gain, resulting in scale saturation.

Special sources 1 and 2 were studied.

The special source 2, a contact binary star is getting close to a supernova event in a few years, and we want to baseline it and get ready to observe the supernova emission.

To find objects Gary used the tables in Rich’s observing guide and in the Data Book  “Astrophysical Data: Planets and Stars” by Kenneth R. Lang.

The V notch object that Tony studied was not tried in Rich and Gary’s session.

Galaxy Observations:

Rich and Gary also did an experiment to measure the hydrogen (HI) Line Doppler shift and therefor the velocity along the galactic plane. They were able to get reasonable hydrogen measurements of the galaxy’s rotational velocity at multiple points from the center out to the radius of the sun.

Rich plotted these observations and got a curve that is in the ballpark but a little different than the published data on similar measurements.  This is the first time that the Galactic angular velocity measurement has been attempted with the 60 ft. dish.

 

See Dr. Rich Russel’s attached Science Meeting presentation for more detail on the site trip and the observations mentioned above.

DSES Science Meeting Presentation October 22, 2018 [Please click to view.]

 

Tony Bigbee also went to the site for the observing session last week.  Tony installed onto the system after Rich and Gary had finished.  He did not get the expected results on the RASDR 4 receiver when attached to the 60 ft. dish over the weekend.  He thought that the issue may be with the pointing accuracy of the System 1 controller.  We used System 2 at the open house when Tony had very good results but did not get the same on this last weekend’s observation session using System 1.  Tony looked for the V notch absorption object and is using a new code to calculate the source amplitude.  He did not get good results on this and suspects pointing error.

He  calculated the curves for the open house and last weekend’s observations showing time and discovered that these are different indicating that something is wrong between the two.

Tony did a Mollweide projection plot like the one below.  In Tony’s plot the green line is the meridian,  the blue line is the galactic plane.  The black X is the position of the telescope. See Tony Bigbee’s actual plot when he posts or sends it out.

Figure 1 Example of a Mollweide Projection

Rich suggests that anyone going down to observe should measure some of these same sources and get data to compare their results.

 

Skip Crilly says we have aligned NRAO 5690 at Greenbank and Haswell sites three times using the System 1 controller and it seems to be positioning correctly. Steve can do an additional observation next week, Tuesday and Wed and verify the alignment.

Another difference from the open house observation was that Steve Plock added the alternate cavity filter configuration.

As mentioned previously the coordinates of some of the sources are from celestial coordinate year 1950 epoch and year 2000 epoch so may be different positions now due to precession and galactic movement.  A mathematical correction to the coordinates may be required to make an accurate set of coordinates for the current date. However, the small difference afforded by this is probably within the capture angle of the dish.

 Glenn Davis says that his NTP time sever may be useful to improve the accuracy of the pointing systems. 

Bill Miller said that the System 1 controller may still have a discontinuous elevation reading error.  This was seen previously this summer and has not been fixed.  This could contribute to a pointing error and inaccuracy on some coordinates.

 

Additional Considerations:

Anyone going to do observations at the site should try to replicate the studies of the observation guide and use the Observation Checklist to make their session useful and comparative.

Currently the LMST is close to local time, and so one needs to consider this and observe in the evening instead of afternoon.

See the back of Rich Russel’s observing guide for dish rules and limits. An observation data sheet and suggestions are available in the back of the guide as well.

We need a list of some calibration sources to start all observing session with, to be sure that the pointing system is working properly and that it isn’t broken with new SW drops.  Also, we hope the voltages we measure from calibration sources (with known Jansky levels), will enable us to derive the Janskies of other objects we wish to observe.  Janskies are the measure of the flux density that the antenna receives.

Three papers have been accepted in the next SARA journal.

“The Deep Space Exploration Society 2018 Perseid Meteor Shower Open House”. By Bill Miller, Gary Agranat. Deep Space Exploration Society.

SpectraCyber Neutral Hydrogen Measurements using the Deep Space Exploration Society 60 – foot Antenna System“. By Richard Russel D.Cs., Ae.E.; Gary Agranat. Deep Space Exploration Society.

Dark HI Cloud Observation using the Deep Space Exploration Society Plishner 18 – Meter Dish with the RASDR4“. By Tony Bigbee, Richard Russel, Steve Plock. Deep Space Exploration Society.

 

Skip Crilly discussed his new 28 ft. antenna that has a 5 pixel or 5 separate antenna segment feed and is mounted on a cargo trailer but will be used mostly for SETI.  The antenna may not be large enough to observe the strange signals we have seen.  File size is one challenge since it is inversely proportional to the gain and noise ratio.

 

Meeting was adjourned after much secondary discussions not captured here.

 

 

Old 9/24/2018 Agenda and Notes from last science meeting:

  • Glenn Davis proposes a graphical user interface called Astro Guide that would allow better guiding and tracking of radio sources.
  • Rich’s presentation and overview of the radio astronomy guide
    1. Started with Floyd’s list
    2. Added the 1420 MHz sources from the book “Tools of Radio Astronomy” by K Rohlfs and T Wilson.
    3. Added the hydrogen measurements from K5SO, Dr. Joe Martin who has provided signature images of the objects.
  • Gary, Jay Wilson, Rich and Steve all went to the site on 9/22 and did observations using the 60 foot dish.
    1. Used Spectra Cyber
    2. Used system 1 pointing
    3. Used the new setup with the cavity filter
    4. Limit switches are set at +/-15 ether way of north. CCW to 345.  CW to 015.
    5. Gary got great pictures of the event.
    6. Need screen print capability to capture the Spectra Cyber parameters display.
    7. The Spectra Cyber SW is easy to take the data and use it.
    8. Need a Lap Top with a com 2 serial port to attach the spectra cyber. This is difficult because most of the Serial to USB port adapters don’t want to set for Com1 or Com2.
    9. Need to do calibration sources before and after observation of an observed object and keep all settings on the Spectra Cyber the same.
  • From Tony, “To avoid problems of solar interference all observations were made between sunset and sunrise. Most scans were taken with the telescope on the meridian.” Galt and Kennedy, 1968,  ‘Survey of Radio Sources Observed in the Continuum near 1420 MHz, Declinations —5° to +70°’ http://adsabs.harvard.edu/abs/1968AJ…..73..135G
  • Rich presented a number of plots from their observations. See Rich’s report.
  • The scan across the galaxy were at one RA. The radio hot area was offset from the optical.
  • The galactic rotation rate was also observed.
  • Got a lot of raw data, learned how to catalog it and analyze it.
  • The calibration sources did not show any signal above the noise.
  • Got good data for Sagittarius A, SAG A.
  • 3 Papers have been submitted for the SARA Journal.
  • The Western SARA conference is in Boulder in March.
  • Next Observation Trip. Need a couple of nights.

Plishner Site Report for the Weekend of October 19-21, 2018

This is a summary of our activities at the Plishner radio telescope site during the third week of October 2018.  Steve Plock, Ed Corn, and Gary Agranat contributed to this report.

Participants this weekend were Gary Agranat, Paul Berge, Tony Bigbee, Ed Corn, Hans Gaensbauer, Dave Molter, Steve Plock, and Rich Russel.

Our plan for the rest of the year is to work at the site during the third weekend of each month.  The Friday evening is devoted to astronomical observing, and the rest of the weekend is then devoted primarily to infrastructure and equipment work.

60-foot Antenna Observing, by Gary Agranat, WA2JQZ

On Friday afternoon and evening Rich, Gary, and Paul did 1420 MHz neutral hydrogen observing with the 60-foot antenna.  The primary observing goal was to take regular measurements of the hydrogen signal along the Milky Way galactic plane at 10 degree intervals, from the galactic center to about 110 degrees (a little more than the first quadrant).  The Doppler shift of the hydrogen was measured at each 10 degree point. From that, Rich later used some basic geometry to derive a velocity and distance from the galactic center for each measurement.  A second goal was to observe several known, strong galactic radio sources that could be used in the future for calibration of our observations, and also to see if we are capable of observing those sources in a consistent way (without unknown biases).  A third goal was to observe additional galactic sources as targets of opportunity, to see how well we do, and to also see what problems we hit.

Galactic plane observing started at about 5 pm local time, when the galactic center in Sagitarius had risen high enough in the sky for us to observe. The galactic plane and most of the other observing were done with the 60 foot antenna pointed along the meridian (180 degrees azimuth to the south and zero degrees to the north), in order to eliminate the Earth’s rotational motion in the Doppler shift measurements.  We observed until about 10:30 pm, when the team was then quite tired. To warm us up during the evening, we made a batch of hot apple cider.

Details of the observations and results were discussed at the science meeting on Monday October 22nd, and those will be covered in a separate post.

– Gary WA2JQZ

60 foot dish antenna on Friday late afternoon, as the galactic plane observations started.

 

We’ll continue with the discussion of the weekend infrastructure work.

Saturday Infrastructure Work by Ed Corn, KC0TBE

Our first order of business was to re-service the toilet and spare in the outhouse. They now both have RV antifreeze for winter. Next installed was a portable heater for winter operations and I labeled all the breakers in the out house. I then labeled the doors with instructions for emergency exit and the safety pin for privacy at the main door.

With the help of Gary, Hans, and Paul we have the first 3 tower sections in place at the bunker, along with the first set of guy wires. [More about the tower below.]

-73’s Ed KC0TBE

DSES Site Work Report by Steve Plock KL7IZW, DSES President

Paul Berge worked on Friday, Saturday and Sunday. Because he travels  from Lyons, Co. he prefers to maximize his efforts each visit. Also the weather window for the year is closing. I attempt to support his efforts as best as I can. Paul provided support for Rich Russel’s data acquisition which included galactic Doppler measurements. The team  knocked  off before midnight.  Results have already been detailed in the  Science meeting on 22nd of October.

On Saturday Ed installed a heater in the outhouse, winterized the RV toilets, and labeled the outhouse breakers.

During Saturday afternoon Hans, Ed, Paul, Steve and Gary all worked together to erect the new communications tower. The first set of guys were finished  at 23 ft. by Ed Corn doing all the climbing.   The majority of the rest of Saturday myself  and Paul spent evaluating the elevation limit switch operation, including testing complete functionality with fault clearing via the built in override capability.

Later that day, Tony Bigbee showed up, and Paul and Steve supported subsequent  hydrogen observations using the RASDR4 receiver.

The majority of Sunday was consumed by lubrication of the dish and adjustment of the azimuth drive chain. I also installed the conduit in the elevation bulkhead so that Bill Miller can complete his synchro  wiring project.

Sunday Dave Molter worked into the night using the 500W floodlights and mixed over 1000lbs of concrete to try to prevent continued erosion in the ramp area.  A big thanks to all who participated in  this cooperative effort.

– Submitted by:  Steve Plock,   President DSES

Photos by Gary, from Friday and Saturday:

Position of the 60-foot antenna as it is pointed due south, at 180 degrees azimuth along the meridian.

The Moon with the 60-foot antenna.

View from the base of the dish antenna, looking towards Haswell.

Haswell as the sun set Friday evening.

Pikes Peak and Cheyenne Mountain were visible on the horizon, about a hundred miles to the west-northwest.

Work Saturday morning at the outhouse.

Work at the outhouse, including labeling.

Hans helping Ed unload tower sections and a jin-pole, for building up the ham radio communications tower at the bunker.

The first section of the tower had already been installed during the last work trip. Here Ed is safely secured to the tower after the second section has been hoisted with the jin-pole, which is also temporarily securely attached to the tower. He is fastening the bolts of the second section on to the top ends of the first section. He did this again with the third section.

Ed fastening the bolts of the second tower section on to the top of the first.

The team standing ready as Ed works on the tower. Hans is standing by the third tower section.

The tower at left with the third section up. A 6-meter delta loop antenna was hung from the tower to the doghouse. Stainless steel guy wires were also extended from the third section, per tower specifications.

Hans, Paul, and Gary installed supports for the guy cables, at one-third intervals around the tower.

Hans and Paul securing one of the guy wires at the ground support.

Configuration of the tower with 3 sections, until work resumes next time. The current plan is to install one more section with a rotator. The rotator shaft will have at least a triband HF yagi antenna and a 6 meter directional antenna for meteor scatter. Also, small horizonal supports will be added to support the 80 and 160 meter dipoles, currently supported at that position with a pole.

 

DSES Plishner Site Work Trip Report September 14-16, 2018

Here is our report of our work trip at the Plishner radio telescope site in Haswell, on the weekend of September 14-16, 2018. Opens as a PDF file. Illustrated with photos.

DSES Plishner Site Work Trip Report September 14-16, 2018

By Bill Miller and Gary Agranat.