Friday, September 1, 2017

Radio-Sky Spectrograph works with Radio-Jupiter Pro,

There are a number of ways that Radio-Sky programs can interact with one another.  For example, RTL Bridge can send signal strength from a RTL dongle receiver to Radio-Sky Spectrograph  (RSS) and to the Radio-SkyPipe (RSP) strip chart program.Radio Eyes can start a RSP chart. Radio Jupiter Pro (RJP) can send calculated Jupiter or Solar information to RSS.  Since more people use RSS for Jupiter and solar studies than anything else that I am aware of, it makes sense that RSS can draw this information from RJP when desired.



A new update for RJP facilitates the new Slope Note Pad tool.  With this tool you can easily
run through SPS files and take the slope of a feature (modulation lane, N burst etc.) and
it will grab the corresponding CML IoPhase from RJP and will add it to a list that is exportable
to a spreadsheet.  You just click at the beginning and end of each feature you want the slope
of and your data is compiled for you.

Also be reminded that if you have RJP running along side RSS, and you have the option
set under Options / Network / Radio Jupiter Pro Information Server / Connect to RJP
You can then right click anywhere on your chart and select  Get RJP Charts, which will
produce CMLIo charts, SkyMaps, and AltAz views for that given time. You don't have to
type a time into RJP to do this. Each of these RJP displays has a camera button which
places the image in the clipboard for easy pasting into all of these nice reports you have
been creating. All of these displays popping up in addition to your RSS display takes a lot of screen real estate. Probably would be easiest on a multi-monitor system.

There is a new version of RSS 2.8.45 that you can get to through Help/Check for Updates.

If you have never installed RSS you can get it here:

http://radiosky.com/spec/Spectrograph.exe

For this to work correctly do the following update to RJP:

http://radiosky.com/rjp3/rjp_update_3_8_2.exe

In RJP you want to make sure the Information Server (JIS) is running on start up.
This is found under Tools / Jupiter Information Server.



Finally, you could use the JIS feature to grab the info for any program by making a TCP connection to the IP and Port shown.  In the Jupiter Info Server Options you can push out the selected info (in string format)  by using the Push option or by Sending a "J" to the server from your client you can get the JIS to send you the string.  Try it using a terminal program.

Added September 2. 2017
Larry Dodd, K4LED, used the features described above to make the nice solar observation report below;




Have Fun.

Jim

Wednesday, August 16, 2017

RTL RFI Interference Sniffer

RTL RFI Interference Sniffer



 A useful RFI finder tool is a software defined radio (SDR) such as a $20 dongle receiver (and $40 up-converter if you want to cover HF).   You might also be able to find frequency ranges that are free from interference!  You can actually use a portable setup like this for hunting down interference.


This system can be improved by mounting the antenna on the end of a wooden or plastic stick,( a paint stirrer works well).  The choke helps to keep you from becoming part of the antenna, which while not resonant, works well when probed close to suspected radiators. (Not hot power lines !)  As a matter of fact, you should wear some electrically insulated gloves when doing this.

This project requires an Android device that has OTG USB support so that the device can be used to operate a RTL style dongle radio.  The tablet itself is an RFI radiator, or at least the one I have tried is. It possible insulate yourself from the tablet by using gloves, placing it in a cover, or mounting it on a piece of sturdy cardboard that can be used to handle the tablet without touching it.  When you touch the tablet you become an antenna for its own RFI.  Normally that isn't a problem because your antenna is far from your tablet, but in this case you are carrying them both. 

You need two programs from the Google app store.
  • RF Analyzer (Free) or SDRTouch (I bought the paid version for $10).
  • RTL-SDR driver.
Just search for RTL SDR in Google Play. You may even find a program you like better. It works well for me on this rather modest 7" LG tablet that came "free" with a phone plan.

I am using the small whip antenna that came with one of RTL dongles (everyone has at least 8, right?) You can also construct a small dipole or loop if you wish.  Unless you know that you are going to be working in a relatively small part of the spectrum, the antenna is not going to be resonant anyway.  In most situations it is going to act like a near-field voltage probe, which is probably the preferable mode for sniffing interference sources around the house. If it is too sensitive it is going to be harder to home in a RFI source.

Read my post about RFI basics.






Pre-Eclipse Checklist for Radio Jove Observers


Radio Jove observers from Canada to Mexico will be watching the great 2017 eclipse at at 20.1 MHz.  We will be looking for changes in the galactic background radio emissions.  This is different from most other eclipse/radio experiments that will be occurring. Those efforts mostly will be looking at artificial radio signals (transmitters) reflecting from the ionosphere.  Not us.  We picked a target made harder by the fact that we will be looking at a quiet part of the sky.

The sky at 408 MHz during the eclipse of August 21, 2017 as seen from KY.  The circle represents a dipole antenna beam aimed at the zenith.  The Sun and Moon (neither to scale) are shown to coincide. Virgo A will also be near the beam.
Andrea and I will be on the road looking for a place in the line of totality to set up our dipole. Roads are expected to be clogged with people.  Good luck to everyone observing.  Be safe out there


Radio Jove – Solar Eclipse Instructions Checklist


1. Observing Plan – coordinated practice sessions with Radio Jove Team
     a. Call during a Help Session
     b. Upload a 24-hr test record to the Data Archive to check data quality            http://radiojove.org/archive.html

2. Equipment
     a. Receiver tuned to a clear frequency (near 20.1 MHz) and working properly
     b. Antenna Setup – Dual Dipole (No phasing cable) or Single Dipole
     c. Calibrator (optional but encouraged for better scientific results)
     d. Windows Computer with Sound Card
     e. Check the audio cable input to the computer – choose Line or Mic input
     f. Software – Update Radio-Skypipe Pro (to version 2.7.28 or later)
          i. Set ALL Identity Info (under Options menu)
              1. Give a useful Local Name (this is your Station ID name; e.g. MTSU or HNRAO)
              2. Give receiver/antenna description in Notes (under Options menu)
         ii. Set Meta-data (under Options/Misc, click Radio Jove MetaData) to give antenna information.              Example Description: Jove Dual Dipole; Beam Azimuth: 180; Beam Elevation: 90;                              Polarization 1: Linear
         iii. Check Tools/Mixer (Input sound settings) – select the correct sound card input (Line or Mic)
         iv. Calibrator – run Cal Wizard to calibrate your system to Antenna Temperature (if possible do              a daily calibration)
         v. Timing – Check computer clock for accuracy. Run Atomic clock if needed.
         vi. Timing – Record ALL data in UT time

3. Site and Safety Check – check for power lines and other potential hazards

4. Data Collection
     a. Collect data for August 19 – 23, 2017, or longer if possible
     b. Collect a minimum of 6 hours each day: Set start/stop time for  3 hours from 18:30 UT
     c. 24 hr records are preferable

5. Data Analysis
     a. Load data in Radio-Skypipe and view the full data record
     b. Change Y-axis scale to 0 and 250 kK (for calibrated data)
     c. Save record as an image file, preferably a JPEG

6. Data Archive
     a. Login to the data archive: http://radiojove.org/archive.html
     b. Upload the data record (.SPD file) and the JPEG image together


Friday, June 30, 2017

Radio Frequency Interference - Basics



The only tree that I ever actually hated.


Radio astronomy's biggest nemesis is unarguably radio frequency interference or RFI.  Our electrically civilized world is full of it, and it is getting worse.  The light pollution activists in the optical astronomy world have been fighting a terrifically challenging villain, but at least people can relate to light pollution in a very personal way.  The unseen RF spectrum is much harder to get people excited about.  For the most part, you are on your own when trying to track down and re-mediate RFI.

Identifying RFI

For the purposes of this post, let's assume you have a simple Radio Jove receiver and are listening in at 20.1 MHz.  Assuming that Jupiter or the Sun is not active and there is no lightning nearby, what would you expect to hear from the receiver if there was no local RFI?  You would hear a steady hiss. White noise.  The sound would be basically featureless. Some of that hiss would come from your receiver's components and hopefully, some will be hiss from the Milky Way.

  Example of hiss. Galactic Hiss from Radio Alachua

In actual practice, you probably will hear a few pops and other imperfections especially in the HF band where lightning and man made signals can propagate from long distances away.

Displayed on a strip chart galactic radio noise should look like a "grassy" line.  When hooked to an antenna pointed to the zenith, a day-long variation occurs in that grassy line corresponding to the Earth's rotation through the plane of the galaxy. (See "A Natural Periodic Signal" below). Any sudden deviations from that slowly rolling terrain  indicates either:
  • A energetic event from space (what we may want to see).
  • An energetic event from our Earth's electromagnetic sources (lightning, radio aurorae).
  • A case of human made radio interference, RFI.

What we would like to do is sort out the cosmic events from the Earth-born ones.

Sudden Changes


Sudden changes in signal strength indicate an unnatural source (except for lightning).  Even more compelling is when a signal stops suddenly.  Nothing in the natural world behaves like that.  Things of nature do not have off/on switches and large sources of energy like solar flares have significant light travel times across them limiting how quickly its radio signature might rise or fall.  If on a chart with a multiple-samples/second sample rate, we see an instantaneous vertical leap of significant amplitude, we are safe to say it did not come from the Sun. Solar flares can reach peak amplitudes in just a few seconds, but not in a few milliseconds.

Your strip chart may look like this if you have interfering signals.  These sudden jumps above the baseline level indicate RFI.

Often there will be less dramatic but still obvious jumps in the signal level on a chart that have no obvious other symptom.  There are a number of things that can cause this. A strong out of band signal can desensitize your radio. You should observe with the AGC off if your radio has the feature, but these level jumps can still happen, perhaps when the ham next store turns on his amp.  More often these jumps are the result of  lamps, power supplies, and other appliances that put out a broad noisy spectrum without much structure.  It may sound like cosmic hiss but still be RFI.  This noise adds to the galactic background noise and does not contribute much beyond the obvious jump in baseline.

Modulation

Audio modulation of the signal is not always easy to see on a strip chart but usually it is easy to hear. ANY regular pattern you hear in the signal that deviates from a white noise signal is suspect.  If the sound has any sort of buzz or trill, or tones embedded in it you can rule it out as being a natural signal. Modulated signals can arise from unintentional radiators such as switching power supplies, digital circuits, and televisions, and from intentional radiators like over the horizon radar, radio data links, shortwave stations, and ionosondes,

Power line noise is often modulated by 60 Hz in the Americas and 50 Hz elsewhere. It also tends to have a sharp raspy sound but may be more subtle.  If the noise is not constant it will often vary with the moisture level in the air. Some power line interference is only present when it is dry and other types are triggered by rain or dew. Power line noise often manifests on a strip chart as a very irregular signature. Here is a particularly nasty bit of powerline RFI from the ARRL RFI collection.

Though never really thought of as RFI, Jupiter emissions do have structure. You can learn to hear these characteristics by listening to audio recordings of them in a few sessions.  They do not have very distinctive signatures when viewed in a single frequency strip chart.  However, they are easy to identify on a wide band radio-spectrograph, so check the on line spectrographs to see what Jupiter is doing while listening on your single frequency receiver.  Check on Radio-Jupiter Pro or on the nice free iPhone app by Kazumasa Imai called Jupiter Radio Map to check on probabilities of a signal being Jupiter.

Periodicity


With the exception of pulsars, there aren't any natural signals that appear and disappear with the regularity that might be attributed to a clock (at least a 24 Earth hour clock) .  You will never be over-run by interference from a pulsar - ever!  Pulsars are much to weak. So anything that turns on and off at regular intervals, milliseconds to hours, will not be of cosmic origin.

 A common complaint from rural observers is a sudden pulse that occurs every 1 to 2 seconds.  This is often an electric fence which pulses in this fashion to save power, thank goodness, (Imagine a 60 Hz train of these!)  There is also the kind of period that occurs over the course of a day.  Some people turn things on at night and off in the morning ( or the opposite).  Motorized appliances such as blenders often show up at the time of days when they are usually used to prepare meals.

A Natural Periodic Signal

But there is also a natural daily cycle that is manifested in the galactic background (GB) and the effects of the sun directly and indirectly via the ionosphere. The signature of the GB on Karl Jansky's strip charts announced the dawn of radio astronomy. It was the period of the bump we see when our antenna beams slowly rotate through the plane of our galaxy that gave away it's origin. The bump peaked at a given spot in the sky about every 23 hours and 56 minutes, roughly 4 minutes shy of a 24 hour day. This is the time of the stars, sidereal time, and it tells us the source is located far from the Earth. If over a period of months you see a natural signal at the same sidereal time every day then you have something that doesn't move much against the backdrop of the stars and is probably very far away in origin.
The strip chart above comes from HNRAO and shows clearly the Galactic Plane bulge which you should expect to see during a 24 hour observation.  The hump is broad but should advance earlier by 2 hours every month, identifying it as a sidereal object outside our solar system.
In the example above, notice that there are lots of deflections to higher values which may or may not be unnatural RFI, but very seldom do we see a spike below the the fairly well defined lower edge of the trace. When you do see a downward spike from this lower edge, it may be interference of the desensitizing type but more likely it is just a glitch from the sound card.  Make sure you use 11025 or 12000 Hz as your audio sample rate (Options/Sound in Radio-SkyPipe).

Narrow Spectrum

If you can tune away from a signal by moving your tuning a few kHz, you are usually looking at an incidental radio signal emitted by an electronic device or an intentional signal such as a radio station.  Most cosmic radio signals have very broad spectra and they span from a few MHz to GHz in bandwidth. As you know, black-body radiators emit at all frequencies, though peaking broadly at one.  The quiet Sun, for example, emits radio waves throughout the spectrum though relatively weakly below 30 MHz unless it is flaring.  When a radio solar flare occurs it usually can be seen through much of the HF spectrum though in some cases it can be constrained to a few MHz wide.  The only thing I can think of that you might encounter in the way of a natural signal that is less than tens of kHz wide might be an N burst from Jupiter, but that will not be a regular source of interference.


Finding RFI

Your first suspect for RFI is you, that is, the electrical and electronic apparatuses that you own.  If turning off the main circuit breaker to your house stops the RFI then celebrate because the source is under your control.  When you do this test, you of course need a battery powered receiver.  The Jove receiver can run off of a small twelve volt battery for hours. You can use headphones or a small battery powered speaker/amplifier to listen. While it is informative to run Radio-SkyPipe to monitor the signal visually, be aware that your own computer could be the source of the RFI.  Turn off the monitor for a few seconds while running the strip chart and see if the RFI dips during this period.  If the RFI is coming from the CPU, you will have to just use the audio from the radio headphones to detect it.  The computer and/or monitor should be a major suspect until eliminated this way.

Assuming the RFI went away when you turned off the main breaker, locate the circuit by trying the breakers one at a time until you have found which circuit powers the problem device.  Then begin eliminating devices on that circuit until you find the offender.

Here is my list of common RFI sources you might find in your home or lab.
  • Any device with a switching power supply.
  • Any device with a motor including AC and furnaces and heat pumps.
  • Computers.
  • Computer monitors.
  • LED lighting.
  • Fluorescent lights.
  • Televisions old and new. (Plasma screens are sometimes bad enough that your neighbor's is suspect.)
  • Light Dimmers and motor speed controls.
  • Touch Lamps.
  • Battery chargers, especially for power tools. (Always unplug these when not in use.)
  • Bug zappers.
  • Ionizing air purifiers.
  • Electrostatic air cleaners.
  • Aquarium heaters.

Mitigating Device Noise

There are a number of steps that you can take to reduce or eliminate RFI from electrical devices. The simplest, though perhaps least economical, is to replace the device with one that does not radiate RFI. Unfortunately,  this can be a trial and error process so hold on to your receipts!  You may also find that physically moving the device to a new location is helpful.

Place your antenna as far as possible from the RFI source and use good quality coax cable to your antenna.  Chokes on  the antenna coax shield may be helpful.

If the problem is your own computer or monitor, the issue becomes more difficult.  There is only so much you can do besides replacing them.  Split core RF chokes may sometime be helpful.  These may be placed on any cable entering or exiting the computer.  If using a separate monitor (not a laptop), the monitor cable is a primary suspect.   Many come un-shielded. Replace with a high quality shielded cable and/or add RF chokes to each end. In some cases you just need to leave the monitor off while observing.  You can put remote control on the computer such as TeamViewer, the control the computer remotely and just leave the monitor off. USB and network cables also may be purchased with an range of shielding levels.

Replace noisy switching power supplies with transformer based ones where possible. Add chokes when needed to on both ends of the DC cable.  It usually does no good to add a choke to the 120V AC cord.  Route wires away from your receiver and its feedline.  Add chokes to the DC supply line leading to the receiver.  Twisting a pair of power or digital leads can also reduce emissions.

Power Line RFI

To hunt down power line RFI you have to use a portable battery powered receiver.  One option is a small AM transistor radio, but you can also buy a RFI sniffer receiver that like the one below MFJ Enterprises if you are so inclined.  These MFJ noise monitors are VHF devices seem to work best with strong power line interference. The AM radio is more sensitive but may lead to false detections.



With your radio, walk around to all of the power poles in your neighborhood listening for the offending noise in your headphones.  Sometimes, the bad insulator or transformer will make an audible noise that you can hear without the receiver.  I bought one of the "toy" $30 parabolic microphones shown below and found it helpful in sniffing out audibly detectable problem poles.


Mitigating Power Line Noise


Hopefully you don't need me to discourage you from trying to fix a problem on your power company's pole but just in case, Don't Do That!  You need to enlist the help of your power company. When you find the offending pole take note of the pole number which is usually found on a metal ID tag.  The response you get from the utility company can range from excellent service and a quick repair, to absolute disinterest.  Most companies will send out a mobile unit to inspect the reported pole, so you want to be sure that you have found the right pole. Some utilities will have special technicians with spectrum analyzers and noise receivers just for the purpose of tracking down power line arcing. You can let those people doing the hunting for you, but it is nice if you can have a suspect of your own ready for them if they find nothing.  If you can correlate the arcing with the weather point that out to them.  Make an audio recording and offer to let the technicians listen to it. Be nice and you may find them very cooperative, but you may have to also be persistent to get anything done. It all depends on who you are working with. Intermittent problems may require them to make multiple trips, testing everyone's patience. If your description is good enough they may try to replace the insulators, transformer, etc. based on evidence you present to them. Take a look at W8JI 's RFI page where he looks more closely at the problem components on a power pole.


Lots More Information

Dave Typinski has put together a wonderful comprehensive page of RFI resources for the Radio Jove Project.  Along with the many articles and book references there is a nice collection of HF spectrograms of a number of types of RFI.   Don't miss this resource!

SUG RFI Resource


Radio-Sky Spectrograph works with Radio-Jupiter Pro,

There are a number of ways that Radio-Sky programs can interact with one another.  For example, RTL Bridge can send signal strength from a R...