Showing posts with label HVDN Orbital Channel. Show all posts
Showing posts with label HVDN Orbital Channel. Show all posts

Wednesday, September 18, 2019

International Space Station to be visible on Sept. 19-20




The International Space Station to be visible on Sept. 19-20. The key word being "visible" and is not the only time you can see the ISS though.

Radio amateurs can listen via wireless during most passes with the hope to either listen in during a scheduled astronaut contact with a school or to use the digital packet relay system known as a "digi-peater" to bounce short text messages through the ISS and back down to Earth.


Non-Visual Voice Communication

The astronauts do not have much time for casual amateur radio operation, but you might be lucky if you give the station a call on 144.490 MHz in North America or 145.200 MHz elsewhere in the world. You will need to listen to 145.800 MHz for transmissions from the Astronauts.

Using different receive and transmit frequencies is known as split operation.  Astronauts have the ISS radio programmed the opposite was as you would on Earth.   The reason for this is to minimize interference and increased reliability.

The below photo is of a post card confirming a contact with the ISS and a local amateur radio operator.  The "QSL" card was sent from a ground station on Earth and was not dropped 220 Miles above from the ISS, if you were wondering.





Non-Visual Data Communication

If you are interested in non-voice communication, tuning in to 145.825 MHz will allow you to receive APRS data through the ISS.  Your AX.25 capable radio will use the same frequency on transmit and receive.  A path of "ARISS" will help ensure your transmission is received by the ISS and passed back down to Earth automatically.


Viewing the ISS

Applications such as "ISS Detector" for Android smartphones, tablets and Chromebooks work great to "predict" when the next pass will come over your area.  Apple device users may use "ISS Spotter".  Many computer programs also exist such as "Orbitron" for Windows users,  "Gpredict" for multiple platforms and "Nova" as being the three most popular or easy to use options.

There are also additional augmented reality and web based tracking tools available that are easy to find.

It is best to adjust your eyesight to the dark for at least 10-15 minutes before looking at the night sky. This gives your eyes some time to adjust for maximum viewing benefit.

On September 19th, the pass coming over the Eastern United States will track from South to North




The following day at just about the same time will see the ISS pass over yet again, but just lower in the sky compared to the night before.




Beyond visual observation, it would also be good to keep an eye on the APRS activity via the APRS.fi website to see if radio amateurs are "bouncing" signals from the space station.

You can track the space station and APRS activity via the RS0ISS call sign which broadcasts from the Russian module of the ISS. It is not always active though.  The best way to confirm recent activity is by looking at the AMSAT satellite status page or by looking at the very active Facebook group focused on the International Space Station A.R.I.S.S experiments.

If anyone would like to take some pictures of the upcoming ISS pass, it would be great if they can be shared in the comments or emailed to info@hvdn.org for a future article.


Tuesday, August 20, 2019

Presentation: Radio Astronomy


It was fantastic to get invited to the Mid Hudson Astronomical Association meeting and be given an opportunity to present about radio astronomy on August 20th 2019.

What is radio astronomy?

People staring up at the night sky or through a telescope has been around for practically forever.  As early as 1860 was it speculated that wireless signals may be received from the universe. 

While the earliest forms of wireless communication were only just starting here on planet Earth,  this form of now ubiquitous communication did not start to see major exploration until the 1900's and get more interesting just before the outbreak of WWII.



It was not until 1932 by accident that radio interferometry was actually coined by Karl Jansky of Bell Laboratories.   At this time in history, so called "shortwaves" were the pinnacle of radio communication technology.

Mr. Jansky was tasked in finding a source of interference between 2 and 30 MHz.  While pointing a high gain antenna upwards did he then notice a signal source coming from somewhere else.

Fast forward to 1945 and the theory of Dutch scientist H C van de Hulst regarding the frequency of the most common element of  Hydrogen at 1420 MHz which may be used to determine the size of the universe and accurate location or formation of various interstellar bodies such as black holes or stars.

It only took six years for theory to become fact, thanks to a scientist at Harvard University named E M Purcell.  His use of the most sensitive radio receiver a the time along with a nine foot long "horn antenna" is all it took to become in some circles, one of the parents of "radio astronomy".



Modern Radio Astronomy

There has been way too much progress since 1951 regarding radio astronomy, so will leave that to you to further discover.

The rest of this article is only going to focus on how you can assemble a basic radio telescope using much lower cost equipment and obtain even better results.

Here are the slides that Steve Bossert K2GOG presented at the Mid Hudson Astronomical Association meeting for those interested in having a look.








Thursday, June 20, 2019

Mr. President: Dialing for satellites?

beige box hacker ham radio maker

Ah, the ubiquitous DTMF keypad still has some relevance as a modern communications tool in the age of voice assistants, location technology and digital communications. Lets find out if that is true.....

What is DTMF?


When you press the buttons on a telephone or most radio keypads, a connection is made that generates two tones at the same time. A “Row” tone and a “Column” tone. These two tones identify the key you pressed to any equipment you are controlling. If the keypad is on your phone, the telephone “Central Office” equipment knows what numbers you are dialing by these tones, and will switch your call accordingly.

If you are using a DTMF keypad to remotely control equipment, the tones can identify what unit you want to control, as well as which unique function you want it to perform.


DTMF tones

How do you dial satellites with DTMF Mr. President?

Not all amateur radio satellites focus on providing voice, packet, location or image sharing. A few have incorporated APRStt which makes for novel quick communication of both user call sign and location using one nice short string of DTMF codes.

DTMF satellite ham radio


Any one who has watched or conducted amateur satellite activity may be familiar with the grid square or maidenhead location system.   Using only two capital letters, two numbers and two lower case letters can the geographic position with accuracy of 7.5 miles.

While that may not seem too accurate, its good enough for quick general location exchange.  Simply speaking into a radio that you are located in FN31 or FN31bw is far easier than saying 38°53'52.6"N 77°02'11.4"W or even 38.897933, -77.036500.

Using APRStt, you can simply press *13315246402164# which works out to K2GOG located in FN31bw.   The time it takes to send 16 characters is less time than it took to read this last sentence.

For those interested in data satellite communications, but do not own a radio capable of the popular AX.25 based 1200 baud APRS functionality like the Kenwood TH-D72, TH-D74 and the newish Lanch HG-UV98 to be reviewed on HVDN later this summer, this may be an interesting communication method to experiment with.  Courtesy of Bob Wood, WA7MXZ, here is a nice calculator to compute your own APRStt sentence.


Harris Falcon2 satellite radio military green

Any amateur radio with a DTMF keypad from the lowly $25 BaoFeng radios, to more current mainstream radios like the Yaesu FT-70R and about 300+ other models to the super cool looking military "knock off" variants of the PRC-152 found on E-Bay would work just the same for APRStt since they can all send DTMF.

But how to decode APRStt?

DTMF is hard by ear to determine the DTMF code sent, so the soon to launched PSAT2 includes a  DTMF to voice transponder which will read back via computer generate voice a fully formed APRStt sentence it receives.  There are also many other very interesting things that PSAT2 will also permit such as:

  • PSK31 10m band up-link/UHF FM down-link
  • SSTV camera with UHF down-link in the same pass-band as PSK31 signals
  • DTMF Grid Square up-link and Voice/APRS down-link for Grid position reporting
  • DTMF Text messaging (APRStt).
  • APRS text messages up and Voice down.
  • Conventional APRS digipeater 
Some may choose to experiment with an SDR tuned to the appropriate PSAT2 frequencies and decode APRStt with suitable software or maybe even use an Arduino based simple DTMF decoder since not many amateur radios can decode DTMF easily. 

what is on the PSAT2 satellite?


The radios that can and often include other uses for DTMF multi tone decoders and could be programmed ahead of time to un-mute when a known APRStt is heard, but that sounds frustrating.  Maybe someone will "hack" a TYT MD-380 or other to show DTMF since it is capable at multi tone decode?  Hmmm.....

PSAT2 details please?


AMSAT APRS PSAT2 ParkinsonSat2  HVDN STEM

Once this interesting cube-sat reaches orbit and is provisioned for operations after the June 23rd or 24 or 24th 2019 launch window, we will be able to track the satellite and hopefully learn if 28.120 MHz is the actual 10m frequency to be used for the PSK31 transponder up-link or not.

PSAT2 is sure to be an exciting satellite and we wish it success and to help continue to make ham radio great again!

Related Reading

Sunday, June 16, 2019

Upcoming Balloon Launch: SSTV & APRS from "near-space"


The Binghamton, New York headquartered, Triple Cities Makerspace intends to launch a balloon with amateur radio payloads on June 29th in order to promote the convergence of various hobbies.




The Triple Cities Makerspace, Inc., a 501(c)3 not-for-profit workspace and education center is launching a high altitude balloon to near space (100,000 feet) and transmitting photos of the atmosphere during the flight.  The most recent New York based amateur radio technology assisted balloon launch was completed by the West Point Amateur Radio Club on April 6th 2019 where it reached a transmitted elevation of 98,087 feet.




The Triple Cities Makerspace launch will take place on June 29th around 10:30 AM, tentatively depending on weather. The balloon will be tracked by amateur radio and also live photos during the flight will be transmitted back to the ground via amateur radio.

The group hopes that many radio operators will participate by listening in and uploading photos they receive to the project’s website: https://reachfornearspace.com 

The flight is expected to last around 2.5 hours and the coverage area of reception within 500 miles.
Gary Dewey, an amateur radio operator (callsign KD2PYB) and member of the Triple Cities Makerspace, is leading the project. “I’ve always dreamt of going to space, but this could be the next best thing – building something that goes to (near) space. I hope this project inspires others to experiment and reach for their dreams.”

Listen Up!

Gary further shares that they are using the MicroTrak-2001 from Byonics for APRS and will be transmitting on 144.390 MHz with the call sign KD2PYB-11.

For SSTV, they are using a raspberry pi zero with the pi camera, a pHAT dac for a sound card interface and inexpensive Baofeng brand radio for the transmitter. They will be transmitting on 145.600 MHz.

The pi runs a shell script set up as a linux service (just in case it reboots midflight) that takes a picture and formats it, then converts it to Martin2, then plays it out the sound card where it will be transmitted over the handheld.

Please look at https://reachfornearspace.com/ for the most up to date information about Gary's balloon launch.

Decoding APRS & SSTV

For those looking to monitor this fascinating experiment, here are some inexpensive options for hardware and software on June 29th.

Any smartphone running the free Droid SSTV app simply held up to the speaker of any VHF receiver is capable to decode the image signals. This "technique" is known as passive coupling. For better signal decoding, a wired approach can be employed with the appropriate cable using the same software and interface to a smartphone or tablet.  There are too many desktop/laptop options to consider, but should be easy to configure.

For real time APRS tracking, the same passive method can be used with APRSdroid software or with an appropriate cable to interface the radio to a smartphone. Mode advanced options could include a Mobilinkd TNC2, combined with any 2m capable hand held radio.

A simple "whip" type antenna would be capable of receiving the signals, but a directional antenna such as a 3 element VHF 2m Yagi would be better.

This should be an exciting event.

Wednesday, June 12, 2019

Field Report: LimeSDR Mini Satellite Ground Station

Crowd Supply is where the Lime SDR and LimeSDR Mini can be purchased that have been reviewed and included in past HVDN articles such as the "Satellites & Amateur Radio Spectrum" presentation given at the Trenton Computer Festival by Steve Bossert, K2GOG earlier this year.

Many other interesting crowd funded projected can be found on Crowd Supply as well.  Be sure to check it out.  Our hope at HVDN is to inspire additional interest in the benefits of creating interest in a geosynchronous satellite to cover North & South America in the future.

This below article was originally posted on the Crowd Supply website thanks to Daniel Estévez.



My project uses a LimeSDR Mini as the basis for a ground-station for the amateur radio transponders on the geostationary satellite “Es’hail 2” (known as “QO-100” by the amateur radio community). This satellite includes two linear (also called “bent-pipe”) transponders, one of which is 250 kHz wide and is intended for narrowband modes, such as single-sideband analogue voice, text-based digital modes, and telegraphy. The other is 8 MHz wide and is intended for DVB-S2 and other wideband digital modulations and experiments. The satellite covers one third of the world’s surface (from Brazil to Thailand) and represents the first ever amateur radio payload in geostationary orbit. It also provides an incredible platform for experimenting with different communication schemes.

The downlink of the satellite is on the 10 GHz band, so an inexpensive satellite TV LNB can be used to receive and down-convert the signal to an intermediate frequency of around 700 MHz, where it can be easily processed by SDR or conventional radio receivers. The uplink to the satellite is on the 2.4 GHz band. Many people are using an upconverter to translate a signal from around 430 MHz to 2.4 GHz. However, using a LimeSDR it’s possible to generate the 2.4 GHz signal directly.

My design is enclosed in a weathertight box, so it can be mounted outdoors next to the transmit antenna. This is important, as it limits losses in the coaxial cable feeding the antenna. Losses at 2.4 GHz can be quite high, so it is desirable to keep coaxial cable runs as short as possible.




Using a narrowband signal through the satellite transponder does not require much power. In fact, many people are using an inexpensive WiFi amplifier module to obtain around two watts of power. However, the DVB-S2 requires much more power, especially if using a symbol rate of a few Msps to transmit high-definition video. Therefore, my weathertight box includes a 100 W amplifier, which is a repurposed amplifier for UMTS on 2.1GHz.

The LimeSDR Mini does not provide enough power to drive this 100 W amplifier. So I used a Mini-Circuits GALI-84 MMIC to boost the output of the LimeSDR from around 0 dBm to 20 dBm, which can comfortably drive the 100 W amplifier. The GALI-84 driver amplifier was built using a kit from MiniKits.

To control the LimeSDR Mini, a Beaglebone Black ARM single-board computer is included in the weathertight box. The Beaglebone Black is connected to my LAN by Ethernet, allowing control of the LimeSDR Mini as well as the other equipment (for instance, enabling or disabling the RF power amplifiers).

A power supply is also included in the box to convert from 230 VAC to 26 VDC for the 100 W amplifier, which needs a lot of current. Currently, a 10 A power supply is used, but this doesn’t provide enough current, so I plan to upgrade to a 30 A power supply. The other equipment is fed from the 26 VDC by using some small DCDC converters. The Beaglebone Black uses 5V, the GALI-84 amplifier and the 100W amplifier bias run at 12V (with an enabler controlled by a GPIO pin of the Beaglebone Black), and the amplifier fan runs at 12V (always enabled). A TMP36 temperature sensor is mounted on the heatsink of the 100W amplifier and controlled by the Beaglebone Black.

Currently, this weathertight box is only used for the uplink. For the downlink, the IF signal from the LNB goes into my home through an inexpensive 75 ohm coaxial cable to a LimeSDR which is connected to my laptop via USB3. I plan to also route the IF signal from the LNB to the LimeSDR Mini inside the weathertight box, so as to allow any computer connected to my LAN by Ethernet to control both the uplink and downlink of the ground-station.




Another planned modification to the setup is feeding a reference signal (for example, 10 MHz) into the weathertight box to be used as a frequency reference for the LimeSDR Mini. For narrowband signals at 2.4 GHz, the frequency stability of the transmitter is quite important, and while the TCXO on the LimeSDR Mini is adequate for many applications, using the 10 MHz reference from a GPSDO in my home would give the best performance and also allow very accurate frequency measurement experiments.

This platform is very powerful and flexible, allowing all kinds of experiments. It is intended to be used through a computer on a home LAN, so that the Beaglebone Black only plays the role of bridging IQ samples between Ethernet and USB. However, it is also possible to deploy some simple standalone SDR applications on the Beaglebone Black, so that the ground-station can work automatically on its own.

Therefore, there is still a lot of experimentation to be done regarding the software setup. Currently, on the Beaglebone Black, I’m using limetool, by Evariste “ F5OEO” Courjaud, to send IQ samples to the LimeSDR Mini. These IQ samples are generated in GNU Radio on my laptop and streamed through TCP. I have also used simple Python scripts with SoapySDR to generate test modulations.

Besides single-sideband analogue voice and DVB-S2, which represent most of the current usage of the Es’hail 2 transponders, this equipment can also be used to perform very interesting future experiments. Some of these include transmitting very low power signals buried below the noise using spread-spectrum modulation, testing optimized data modems by trying different modulations and FEC algorithms, performing ranging of the satellite by transmitting a PRN modulation through the transponder, doing two-way frequency and time transfer, implementing a TCP/IP connection by using GSE with DVB-S2, etc.

Regarding the rest of the ground-station, I am currently using a 24 dBi WiFi grid parabola for the uplink, but the plan is to replace it with a 1.2 m offset dish with a custom built circular polarization feed for 2.4 GHz. For the downlink, I am using a 1.2 m offset dish and an inexpensive commercial Ku-band LNB modified to use an external 27 MHz reference.

The design motivation for this platform was to have something that would be very flexible to allow many different SDR experiments, and that could be controllable over Ethernet from anywhere in the house. I think this solution satisfies these goals quite well. Some of the difficulties I am facing are related to the spurious emissions of the LimeSDR. Local oscillator leakage and IQ imbalance images can be quite noticeable when its output is amplified to 100W. With some cleverness, things can be arranged so that these spurious signals do not cause interference to other users, or in some situations they could be filtered out.

---

Clearly, Daniel is very enthusiastic about the QO-100 satellite and the systems that can be assembled to communicate with it.  A very active Facebook group has many other tips and photos from other members.  Details at:  https://www.facebook.com/groups/252645695661305/  



Tuesday, May 14, 2019

Line Of Sight: Aircraft Edition



Definition: Line of Sight

Aircraft and radio waves are two great examples to talk about regarding line of sight.

Simply put, the higher the aircraft flies, the further a ground station can receive transponder signals at 1090 MHz or 978 MHz originating from an aircraft.  Obstructions on the ground such as mountains and tall buildings can obstruct the ability to receive all ADS-B transmissions at the ground level too.

The technology covered in this article is known as automatic dependent surveillance broadcast or ADS-B for short. A fancy GIF animation at the end of this article will help visualize reality from theory even further!

Compare:  Fact and Fiction   

The website "Hey, What's That!" is useful for identifying mountain peaks and line of sight for different forms of communication. The below map shows the theoretical range of ADS-B communications up to 10,000 and 30,000 feet elevation from the chosen center point at a known height.

Poughkeepsie aircraft hobby remote control plane drone

Ground based obstructions have been accounted for on the map as noted by some local summits with the red push pins that make for great amateur radio SOTA destinations. 

A calculation of 47 foot above ground level for a total height of 256 feet was used for the same latitude and longitude coordinates six digits past the decimal point on the "Hey, What's That!" website in order to match the location of the HVDN ADS-B antenna location with high accuracy.

boeing aircraft KPOU IBM helicopter
The "Blue" center dot clearly is not in the center. of the reception range. Its location was moved to calculate the distance to all aircraft from where I was located while I was authoring this article. This is one of many features available to those that gain access to the HVDN VRS. Details about HVDN membership can be found at the end of the article.

Comparison of the theoretical and real world values are very, very close when looking at both data sources.

Had the ADS-B antenna been located outside and above the roof line just a few feet higher, its possible that the two results would have been even closer.

The dark red "splat" is the historical reception report over time for aircraft up to 30,000 feet. The pink splat is for aircraft under 10,000 feet.

However, there is one thing to take in mind here, aircraft are not flying in every possible location which will account for some gaps in coverage when looking back at the theoretical map.

Is it worth the extra work in adding an outside antenna to gain the additional coverage benefits? This certainly is shaping up as a classic case of diminishing return, so read on to show how this was validated.

Detail:  Spot checking some results

The top photos are captured from the "Hey, what's that!" website for theoretical "potential" results. The lower photo is zoomed in from the HVDN Virtual Radar Server to complete the comparison against fact to cover real life reception results.

10,000 Foot Elevation Connecticut Comparison:   The projected range spike towards and over Springfield was accurate from the projection and actual reception results.

Add caption

30,000 Foot Elevation Finger Lakes Comparison: Coverage was just short of the prediction over Cayuga Lake, but awfully close.

hvdn

10,000 Foot Elevation Long Island East End Comparison: Coverage fell short of the North Fork at 10,000 feet but air traffic is captured as noted by pictured aircraft which were at 14,000 and 18,000 feet pictured to right of coverage overlay.

hamptons 2m repeater hVDN

30,000 Foot Altitude Over Delaware Bay Comparison: Coverage was pretty accurate based on traffic spikes compared to theoretical results.


Further Results:  Comparing Other ADS-B Feeder Sites

According to Flightaware's website, there are a number of close proximity feeder sites to where the HVDN primary site is located in the Hudson Valley of New York.



Only the two highlighted receivers on the map (Orange) have similar coverage of HVDN which must mean that the height above sea level for all three stations must be similar and may even be using near identical reception equipment to that of HVDN (Red)

Here is further evaluation of the public details each of the three stations provide.

Receiver Site #1:  Montgomery, NY - Flightaware 87114



Receiver #2: Poughkeepsie, NY - Flightaware 77960


Receiver #3: Middletown, NY - Flightaware 83104



For Fun:  What if.....

It would seem for the Hudson Valley, few interested seriously in ADS-B reception can really improve reception without a huge height increase or locating the antenna outside.

Steve K2GOG of HVDN thought it would be fun to model the benefits of increased antenna height, so check out our amazing use of animation skills below to see how much higher you need to go to literally receive every aircraft possible via line of site up to 10,000 (Orange line) and 30,000 (Blue line) feet.  

hvdn aircraft, ads-b range distance

Perhaps it may be worth while putting the antenna up another 30 feet located outside. Interested in setting up your own ADS-B aircraft receiver?  Helpful links follow:
Another approach may just be easier to recruit ADS-B feed providers to just aggregate into the HVDN Virtual Radar Server to increase the range of reception for aircraft under 10,000 feet. Contact the author if there is interest in contributing to this.

Saturday, March 23, 2019

Presentation: Satellite Spectrum & Amateur Radio

Steve K2GOG presented on "Satellite Spectrum & Amateur Radio" at the Trenton Computer Festival on March 23rd alongside another 50+ technology and innovation focused topics.

The goal of the presentation was to cover the valuable radio spectrum available through amateur radio and promote its use through innovative communication applications on earth and in space thanks to underlying computer technology



How much spectrum do we have?

For those that are already licensed amateur radio operators, you may have a printed version of the below spectrum chart that the ARRL publishes or at least have seen it somewhere before.

In the United States and most other countries, there are different license classes of amateur radio operators. Some countries restrict the transmit power or operating modes as well as what frequencies can be used depending on your license restrictions.


Steve decided to add up all the spectrum that is accessible to the three current United States amateur radio licenses and further highlight just how much of the total 23,126.7731 MHz of discontinuous spectrum can be used for satellite related communications. The results are pretty interesting.

What really separates the Extra from General or Technician?

Sometimes it is good to be simple. Get the highest license possible and ensure you never have to worry about operating on the wrong frequency. Currently, the only thing that separates the highest from the lowest license class in terms of spectrum access is 3.9321 MHz of operating capability.

The difference in spectrum for the different license classes is mostly found in the HF bands ranging from as low as 135.7 kHz and up to 29.7 MHz. The only other spectrum not accessible to the technician class license is the 219 to 220 MHz portion of the under utilized 1.25m which many consider as being only from 222 to 225 MHz.

The remaining spectrum is all available to the Technician class license holder!

What if your not interested in long range "HF" communication?

With advances in radio receiver sensitivity and advanced low signal to noise ratio transmission modes, large antennas often associated with HF operation are not always needed.

However, even with specialized magnetic loop antennas and FT-8 digital text modes -nothing beats a full sized dipole for global communications on the 14 MHz or 7 MHz bands often referred to as 20m and 40m respectively and not everyone has the space or interest in such an antenna.


Radio propagation theory does not always guarantee communications are possible at all times of the day which may frustrate some people who only have limited times to "play radio" with HF spectrum.

RF HF propagation is just like the weather

A forecast is still just a forecast and is generally correct, but the difference between satellite communications and HF is the predictability.  For those with limited time to gain "radio communications" gratification, satellite communications may be worth a look.

You can easily calculate when a satellite will pass over head in the case of the "Low Earth Orbit" satellites covered in Steve's presentation for example. It certainly would be great if the weather was like that, wouldn't it?




Depending on satellites

One shortcoming of most satellite communications is that you are reliant upon a man made piece of technology flying over your location in order to make long range contact.

The other shortcoming is you can only make contact with other stations in the footprint of the satellite, which is different than HF since technically you can talk around the world and sometimes even hear your own echo under the right conditions.

Benefits of satellite communication is that you can get a lot of "ham radio" done in a very short amount of time given the brevity of low earth orbit satellites for those not fortunate to live in the foot print of the only current geosynchronous satellite that covers all of Europe, Middle East, Africa, India and a few other countries across Asia.


Fight:  Innovation in amateur radio

The first amateur satellite put into orbit was OSCAR-1 in 1961, just 4 years after Sputnik was put into orbit as the first ever satellite. 

Now almost 60 years later, there has been a total of over 100 satellites put into orbit and most of them being fully operational, with a few example success stories being AO-7, SO-50, AO-92 and QO-100.

In total and thanks to international regulatory efforts, all this satellite success requires spectrum to be set aside since managing who or what can use certain frequencies is more challenging compared to how a specific country can manage its finite spectrum resources.

Its pretty clear that there has been a lot of innovation within the amateur radio satellite spectrum, but much of it has yet to be fully realized.

One example of how technology originally meant for meteor scatter or earth-moon-earth communications which involves bouncing signals off of these non-man made satellites is known as low signal to noise ratio modes, mostly invented by Joe Taylor, K1JT.  The modes can now be found in use on the HF bands rather than for space related contacts. Here is how computers and amateur radio together create innovation.

Technology Improvements: We all benefit 

OSCAR 100 which was put into functional orbit by the Qatar Amateur Radio Society along with technical guidance from the German branch of the Amateur Satellite Corporation known as AMSAT pushes the boundaries of technology and spectrum management.

In 2018, various digital voice modes such as those enabled and made more accessible due to Multi Mode Digital Voice Modem (MMDVM) hot spot devices created an issue for certain satellites operating in the congested 435 to 438 MHz band.   A LEO satellite such as AO-92 speeds overhead at an average altitude of 220 miles and can easily be interfered with by 20mW hot spots and the lower power radios people use to access them. OSCAR 100 is the only satellite that does not have this issue.



Price has driven the adoption of MMDVM hot spots and radios such as the Anytone D868, TYT MD-380 and others. 

Today, thanks to the QO-100 satellite, there is a lot of rapid innovation taking place which shows that cost and user benefits generate lots of excitement that highlights the growth of the radio arts as specified in FCC Part 97.1.

The only unfortunate thing for North American amateur radio operators is that its not possible to utilize this innovative satellite and its great use of spectrum because it is in geosynchronous orbit. However, the AMSAT project GOLF is coming near which is exciting!

Looking beyond, satellite is just one way to show innovation through the use of spectrum. The future of amateur radio is dependent on finding other innovative applications for spectrum, so why not look at what else may be possible outside of the HF bands, even going as high as the mmW bands -
GigaHertz.... not MegaHertz!!!

Full Presentation & Added Bonus

The complete, but non-animated version of the presentation can be found at the link below in addition to the amateur spectrum database compiled to help develop some of the content Steve K2GOG presented both at the HVDN Quarterly meeting this past March 11th as well as TCF on March 23rd.



Friday, January 25, 2019

How To Guide: Satellite Based APRS iGate

There is so much amazing activity these days surrounding satellite and software defined radio (SDR), but there are not many clear and current guides for those interested in creating receive only gateways to send satellite born APRS signals over the internet. Let's change that.



APRS & Satellites (and balloons, drones, etc)

Currently there are three active satellite based digipeaters in low earth orbit. The International Space Station (ISS), PCsat NO-44, and SAT NO-84 all operate on 145.825 MHz.

There is also a fourth APRS satellite named FalconSat-3 that was turned over from the United States Air Force in 2017 for amateur radio use, but is operated on 145.840 MHz and requires a little more work to use. There are other amateur digital mode satellites in the planning stages.


othernet amateur radio aprs
Image Courtesy of  http://aprs.org/outnet.html


What is an iGateway?

An iGateway is nothing more than a radio receiver that is connected to the internet. Signals received by the antenna are passed from the radio over the internet.  The iGateway is designed for digital or data signals and not voice however. Websites such as findu.com and aprs.fi are two examples are where the benefit of igateways can be shown and show APRS data.

There is also the Othernet (Formerly known as Outernet) project that sends information from its ground station back up towards different satellites that "datacast" to special receivers such as the Dreamcatcher. Properly addressed APRS messages are in turn broadcast over this separate satellite network. This is not the same as an iGateway, but does add some other unique potential.  For an amateur to route a message with APRS through one of the mentioned satellites earlier, one must use the path of "OUTNET" instead of "ARISS".

General users of APRS for ground based modes typically leave the path as WIDE1-1 or WIDE2-1, but those interested in satellite communications must use the alternatives listed since a satellite works differently from a propagation perspective to ground based or even low altitude aircraft or balloons.

How To:  SDR & Raspberry Pi iGateway

To create an iGateway you will require:

  • An inexpensive USB SDR
  • Raspberry Pi Computer or other similar device
  • Antenna capable of overhead reception
  • Various cables and stuff for your installation

There are way too many variables on antennas and cabling specific to every installation so we will keep this brief and skip that part. The shortest run of coaxial cable from antenna to radio is needed. The highest and clearest view towards the horizon in as many directions as possible is required for optimal reception when considering setting up a iGateway.

The satellites we will be monitoring pass over most locations about 3-5 times every day for just a few moments, so it's possible a APRS capable satellite will pass over once every 60-90 minutes.

Lets setup the software bits and bobs....

The main goal of this article is to only share the steps for configuring software to get a SDR dongle working with a Raspberry Pi.  These steps can also work for those looking for alternate uses for SDR based hardware such as the now out of date L-band focused Dreamcatcher v 2.03 boards that were replaced with the newer Ku-band Dreamcatcher v3 and likely could be used too.

The real magic here is the software and how it will all work together.

First step, is get a working operating system on your device of choice such as the Raspberry Pi or Dreamcatcher v2.03. Most of these instructions will work for other linux based computers but is not the focus of this article.

Please run sudo apt-get update and sudo apt-get upgrade first to ensure your operating system is current and has most all of the popular packages installed for general use before continuing.

Second step, involves setup of Dire Wolf which translates sound to packet decoding. Run the following on your device to install it.
sudo apt-get install libasound2-dev
git clone https://github.com/wb2osz/direwolf
cd direwolf
make
sudo make install
make install-conf
Next, you need to configure the operating system to take virtual audio from an inexpensive SDR dongle and pass it to direwolf.  Go ahead and plug in your SDR dongle to your raspberry pi. If you are using a Dreamcatcher, there is no need since the SDR is part of the board already!
sudo apt-get install cmake build-essential libusb-1.0-0-dev
cd
git clone git://git.osmocom.org/rtl-sdr-git
cd rtl-sdr
mkdir build
cd build
cmake ../ -DINSTALL-UDEV_RULES=ON -DDETACH+KERNAL_DRIVER=ON
make
sudo make install
sudo ldconfig
sudo reboot

Let's pause for a moment and test the SDR to make sure its recognized.

run "rtl_test"  and ensure you get a status update like this before continuing. This shows that the SDR is being recognized by your Raspberry Pi, Dreamcatcher 2.03 or other single board linux computer.


Now we need to configure Dire Wolf and the best way to do that is copy some of the great work that Keith G6NHU has compiled. Head on over to his interesting site here:

http://qso365.co.uk/2017/02/a-guide-to-setting-up-an-aprs-receive-only-igate-using-a-raspberry-pi-and-an-rtl-sdr-dongle/ 

The only basic change you need to make is to select the correct frequency. In the United States much of the APRS activity is on 144.390 MHz, but since we are interested in satellite based APRS, change it to 145.825 MHz instead.

What did you say about balloons?

Perhaps you may tire of the same general activity on APRS terrestrial activity or even what may be bouncing off a satellite.  The next logical thing to look into would be tracking a balloon of some sort.

Taner DB1NTO has a new product out to cater to people looking to track something that can only carry a very light weight device.  He calls it PicoAPRS Lite and should open up lots of possibilities to experiment with alongside perhaps with a portable version of an iGateway connected via cellular hotspot.



If anyone in the Hudson Valley is interested in experimenting with tracking objects other than a house which does not move much, or a car, lets start talking.

The STEM (31630) DMR talk group seems a logical spot as well as the AMSAT (98006) talk group, so lets make something happen here when spring time arrives!










Tuesday, December 4, 2018

64 Satellites: Can I get a ride too?

T- Minus     10...9...8...7...6...5...4...3...2...1...LIFTOFF!!!

SpaceX was able to put 64 various size satellites into orbit with only one Falcon 9 rocket. The total payload weighed in at 8,800 pounds (4,000 kilograms).

learn about satellites class students
Jerry Buxton, N0JY of AMSAT pictured at the SpaceX launch facility.
AMSAT was responsible for the Fox1Cliff (OSCAR-95) communications
satellite available to amateur radio operators world wide

Payload Details

Of the 64 objects launched on December 3rd,  the amateur radio Fox-1Cliff which is now known as OSCAR 95 is just one of many satellites, so here is the full list of publicly known 60 satellites and basic details, so let's get going.....



amsat satellite amateur radio student space


Lists: We love lists!

Not every satellite was a "CubeSat" which are normally 10cm cube weighing less than 4 kilograms.The largest satellite part of this launch was potentially the 231-pound (105-kilogram) KazSTSAT Earth-imaging satellite.  

There was also the Elysium Star 2 which carries the remains of Robert Lawrence, an African American astronaut was selected for the U.S. Air Force’s Manned Orbiting Laboratory program.

64 satellites launched  AMSAT OSCAR 9


#1 - AISTECHSAT 2: The second in the AISTECHSAT series and is a 6U CubeSat developed by Aistech to provide thermal images of the Earth. It will also help with maritime and aeronautical tracking as a prototype for a larger constellation.

Thermal imaging system is on board that is used in forest management, fire detection, gathering data for agriculture like identifying the health of the plant, analysing land for expansion. It can also detect energy consumption and loss of buildings.

The satellite also provides airborne and maritime vessel tracking via AIS and ADS-B receivers. The AISTECHSAT can also use a bidirectional communication system on board to send and receive automatic information from the vessel or remote asset worldwide.

For aircraft tracking an ADS-B receiver is on board. HVDN has its own ADS-B receiver that tracks aircraft in the Hudson Valley and is available to its membership. More information can be found here

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#2 - Astrocast 0.1: Astrocast is a planned network of Nanosatellites providing global L-band machine-to-machine (M2M) services. The satellites are orbiting in a low earth polar orbit. This allows the creation of a global network covering the entire globe, including the poles. 

After integration of the NanoLink terminal, the ground based assets can reliably and securely send any kind of sensor data to the constellation of nanosatellites that will acknowledge the reception. Astrocast enables transmission of 1KB/day from any region on the earth.

A geographically distributed network of ground stations collects the data gathered by the satellites. The data are then uploaded to a cloud storage for access by the customer.

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#3 - Audacy:   Audacy is building a space-based data relay network via a constellation of medium Earth orbit relay satellites along with our ground facilities. These satellites will maintain constant connectivity for our customers’ spacecraft from any point on Earth to lunar orbit


Details on 59 more satellites

Fantastic research has already been done by Gunter Krebs on all the other satellites that were part of this historic launch.  Have a look at all his hard work at  https://space.skyrocket.de/index.html 


https://space.skyrocket.de/index.html
Add caption
Talk about stuff like this?

Care to talk with others interested in satellite communications and technology plus the experiments conducted up above?   Here are some spots to check out related to amateur radio:
  • AMSAT DMR Talk Group:  98006 (Listen in here)

Sunday, October 28, 2018

SSTV: Images from the ISS

Zipping around planet Earth at 220 miles above on October 27th to 29th 2018 was the International Space Station and its special series of image transmissions using amateur radio slow scan television (SSTV)


What is SSTV?

Slow Scan Television or SSTV for short is a method of sending images over very narrow wireless bandwidth with fairly good color resolution in a short amount of time.

There are many different types of SSTV signals or modes and the one currently in use by the International Space Station is known as Robot36 or PD120

145.800 MHz is the "down-link" frequency for amateur radio operation from the ISS.  Sometimes it is used for voice communication and other times it is used for experiments such as SSTV.   On 145.825 MHz is data "packet" APRS operation for two way "text message" like contact with or through the ISS>

How To Receive SSTV Images?

There are two inexpensive ways to receive and decode an ISS SSTV transmission that can be done with less than $50 of equipment, not including the cost of your computer or smartphone.

Method #1:  USB SDR Dongle & Computer Setup 
Wide band software defined radio (SDR) receivers such as the RTL-SDR v3 can be used for many things, including the reception of signals orbiting above you and around you.  
Other things you can use this 24 MHz to 1.7 GHz  "SDR" receiver for include finding your lost car key remote, monitoring smart home devices, listening to weather, music and so much more.
With free software such as SDR#, its possible to record a "visualization" of the signal for later playback and decoding of SSTV signals. The same signal can also be sent from SDR# to MMSSTV software in real time for decoding of the SSTV transmission.



Method #2:  Inexpensive VHF/UHF Hand Held Radio & Smartphone Setup 
A basic dual band hand held radio can be purchased for about the same price or less as the receive only SDR but will also offer the ability to transmit on a narrow range of amateur frequencies also used by the ISS as well as by over 2,500,000 amateur radio operators globally. 
A very simple way of decoding a SSTV transmission is to simply hold the radio next to your smartphone while running the Robot36 application found on in your favorite mobile app store. By turning the radio volume up, the microphone on your smartphone will hear the SSTV signal and decode it. Sample signals to listen to are found later in this article.
The application will decode the received audio with no physical connection to the radio which makes this very easy to demonstrate for those not very computer savvy.  

Antenna Stuff:   Very important!

While any combination of radio receiver and computing device can be used beyond the examples provided, antennas are just as critical if not more so for receiving the best signal possible.

Having what is called a good "Signal To Noise Ratio" or SNR is needed to help differentiate white noise and static from the actual SSTV signal.  Any interference to the SSTV signal will just look like static like on a television screen, so a good antenna helps increase the SNR and produce a better picture

The good new is that the ISS SSTV signal is often very strong and easy to pick up with basic antennas, but a high power directive antenna is a good idea for optimal reception since it will focus the maximum signal strength from the ISS into your radio.

The reverse polarity SMA-J connector is common on Chinese origin radios such
as those for sale by Baofeng, Wouxon and a few others. 


While good reception results will often be had with the including telescoping dipole antenna with the RTL-SDR V3 or the longer "whip" antenna included with many of the inexpensive hand held analog radios such as the UV-8, a directional antenna is a good idea to consider.

Some options that can be purchased separately made by companies such as Nagoya, Comet and Diamond are easily sourced for VHF only of VHF/UHF operation.

It is best to pay close attention to what type of connector on an antenna like this can be used with your radio as they are not all the same.

The SMA antenna connector version of this same antenna is more common for radios
\made by Alinco, Kenwood, Icom, Yaesu, TYT and Retevis.


An alternate and higher gain antenna called the tape measure yagi beam can be constructed with simple hand tools and materials for less than $20.

There is also a ready made antenna available for purchase from the Arrow Antenna Company as well as the Elk Periodic from vendors such as Ham Radio Outlet.



The beam antenna is a great club project or one for a few like minded hobbyists. Many can be constructed quickly at one time if people work together in cutting and preparing different parts of the antenna for final construction..

What does a SSTV signal sound like and how do I find it? 

In order to know what to listen for, below are three very good signals and the resultant decoded image.

Feel free to try decoding these files with the MMSSTV or Robot36 applications to get familiar with the software since you do not want to miss the fast traveling ISS the next time they are transmitting SSTV images.

The "ISS Detector" app for Android is a great way to find out when the ISS will pass over your location next.
You an also track other satellites and even planets too with this program


To find out when the ISS will be over your location next, please visit AMSAT.org for more information about tracking the ISS, satellites and other interesting space related amateur radio topics.

SSTV space station file
Play MP3 Recording:  10:28AM 10/28/2018 ISS SSTV


slow scan television amateur radio space station
Play MP3 Recording:  10:31 AM 10/28/2018 ISS SSTV

space station contact amsat SSTV ISS
Play MP3 Recording: 12:00 PM 10/28/2018 ISS SSTV

How about SSTV with an SDR?

A nice feature with the SDR# software is you can play back a recording of spectrum at any point in time.

This is also called a base-band IQ file and was discussed in prior articles about receiving voice transmissions from the International Space Station.

This file is a base-band IQ file for the "Atlantis and Mir" SSTV image to help with your own testing.



Select the  IQ file option  in SDR#
and play back the 225 MB recording 

Share your success stories, questions and comments below.  Thanks for reading!