PSK Reporter

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Screenshot of PSK Reporter Pskreporter 2022-10-06-2033UTC.jpg
Screenshot of PSK Reporter
24 Hours of Reception Reports for Station D2UY Pskreporter 2022-10-06-2033UTC-D2UY.jpg
24 Hours of Reception Reports for Station D2UY

PSK Reporter is an amateur radio signal reporting and spotting network and website started by Philip Gladstone in 2014 which allows operators to see where their radio signals are being received. [1] [2] The platform works by collecting digital signal reports from software clients such as WSJT [3] and FLDIGI, [4] then mapping them to show which stations are being heard by other clients. [5] [6] The website takes its name from the popular amateur radio digital mode PSK31 and supports numerous digital modes, [7] [8] [9] but now the vast majority of digital modes recorded by the service are FT8 traffic. [10] Most traffic recorded on PSK Reporter is in the HF amateur radio bands but the platform also supports MF, VHF, and UHF bands. [11] [12] As of 2021 PSK Reporter had collected over 20 billion reception reports. [13]

Contents

Scientific uses

Reporting networks such as PSK Reporter allow researchers in near real time to evaluate space weather conditions, particularly changes in the earth's ionosphere. [14] [15] There are multiple examples of PSK Reporter being used to aid researchers as well as aiding in the prediction and understand of radio propagation. [16] [17] For example, observations made during the 2017 eclipse where over 5,000 amateur radio operators reception reports helped researchers document the eclipse's effect on HF communications. [18]

PSK Reporter data has been used for research in UHF and VHF radio propagation; [11] [19] [20] to help improve machine learning algorithms that predict HF propagation; [21] [22] and to evaluate and test the performance of installed antennas. [23]

PSK Reporter Homepage

Related Research Articles

<span class="mw-page-title-main">Ionosphere</span> Ionized part of Earths upper atmosphere

The ionosphere is the ionized part of the upper atmosphere of Earth, from about 48 km (30 mi) to 965 km (600 mi) above sea level, a region that includes the thermosphere and parts of the mesosphere and exosphere. The ionosphere is ionized by solar radiation. It plays an important role in atmospheric electricity and forms the inner edge of the magnetosphere. It has practical importance because, among other functions, it influences radio propagation to distant places on Earth. It also affects GPS signals that travel through this layer.

Ground waves are radio waves propagating parallel to and adjacent to the surface of the Earth, following the curvature of the Earth beyond the visible horizon. This radiation is known as Norton surface wave, or more properly Norton ground wave, because ground waves in radio propagation are not confined to the surface.

<span class="mw-page-title-main">High frequency</span> The range 3-30 MHz of the electromagnetic spectrum

High frequency (HF) is the ITU designation for the range of radio frequency electromagnetic waves between 3 and 30 megahertz (MHz). It is also known as the decameter band or decameter wave as its wavelengths range from one to ten decameters. Frequencies immediately below HF are denoted medium frequency (MF), while the next band of higher frequencies is known as the very high frequency (VHF) band. The HF band is a major part of the shortwave band of frequencies, so communication at these frequencies is often called shortwave radio. Because radio waves in this band can be reflected back to Earth by the ionosphere layer in the atmosphere – a method known as "skip" or "skywave" propagation – these frequencies are suitable for long-distance communication across intercontinental distances and for mountainous terrains which prevent line-of-sight communications. The band is used by international shortwave broadcasting stations (3.95–25.82 MHz), aviation communication, government time stations, weather stations, amateur radio and citizens band services, among other uses.

Radio propagation is the behavior of radio waves as they travel, or are propagated, from one point to another in vacuum, or into various parts of the atmosphere. As a form of electromagnetic radiation, like light waves, radio waves are affected by the phenomena of reflection, refraction, diffraction, absorption, polarization, and scattering. Understanding the effects of varying conditions on radio propagation has many practical applications, from choosing frequencies for amateur radio communications, international shortwave broadcasters, to designing reliable mobile telephone systems, to radio navigation, to operation of radar systems.

<span class="mw-page-title-main">Skywave</span> Propagation of radio waves beyond the radio horizon.

In radio communication, skywave or skip refers to the propagation of radio waves reflected or refracted back toward Earth from the ionosphere, an electrically charged layer of the upper atmosphere. Since it is not limited by the curvature of the Earth, skywave propagation can be used to communicate beyond the horizon, at intercontinental distances. It is mostly used in the shortwave frequency bands.

<span class="mw-page-title-main">6-meter band</span>

The 6-meter band is the lowest portion of the very high frequency (VHF) radio spectrum internationally allocated to amateur radio use. The term refers to the average signal wavelength of 6 meters.

Shortwave bands are frequency allocations for use within the shortwave radio spectrum. Radio waves in these frequency ranges can be used for very long distance (transcontinental) communication because they can reflect off layers of charged particles in the ionosphere and return to Earth beyond the horizon, a mechanism called skywave or “skip” propagation. They are allocated by the ITU for radio services such as maritime communications, international shortwave broadcasting and worldwide amateur radio. The bands are conventionally named by their wavelength in metres, for example the ‘20 meter band’. Radio propagation and possible communication distances vary depending on the time of day, the season and the level of solar activity.

DXing, taken from DX, the telegraphic shorthand for "distance" or "distant", is the hobby of receiving and identifying distant radio or television signals, or making two-way radio contact with distant stations in amateur radio, citizens band radio or other two-way radio communications. Many DXers also attempt to obtain written verifications of reception or contact, sometimes referred to as "QSLs" or "veries".

Non-line-of-sight (NLOS) radio propagation occurs outside of the typical line-of-sight (LOS) between the transmitter and receiver, such as in ground reflections. Near-line-of-sight conditions refer to partial obstruction by a physical object present in the innermost Fresnel zone.

Multiple frequency-shift keying (MFSK) is a variation of frequency-shift keying (FSK) that uses more than two frequencies. MFSK is a form of M-ary orthogonal modulation, where each symbol consists of one element from an alphabet of orthogonal waveforms. M, the size of the alphabet, is usually a power of two so that each symbol represents log2M bits.

Long delayed echoes (LDEs) are radio echoes which return to the sender several seconds after a radio transmission has occurred. Delays of longer than 2.7 seconds are considered LDEs. LDEs are considered anomalous and have a number of proposed scientific origins.

Near vertical incidence skywave, or NVIS, is a skywave radio-wave propagation path that provides usable signals in the medium distances range — usually 0–650 km. It is used for military and paramilitary communications, broadcasting, especially in the tropics, and by radio amateurs for nearby contacts circumventing line-of-sight barriers. The radio waves travel near-vertically upwards into the ionosphere, where they are refracted back down and can be received within a circular region up to 650 km from the transmitter. If the frequency is too high, refraction is insufficient to return the signal to earth and if it is too low, absorption in the ionospheric D layer may reduce the signal strength.

Amateur radio frequency allocation is done by national telecommunication authorities. Globally, the International Telecommunication Union (ITU) oversees how much radio spectrum is set aside for amateur radio transmissions. Individual amateur stations are free to use any frequency within authorized frequency ranges; authorized bands may vary by the class of the station license.

WSJT-X is a computer program used for weak-signal radio communication between amateur radio operators. The program was initially written by Joe Taylor, K1JT, but is now open source and is developed by a small team. The digital signal processing techniques in WSJT-X make it substantially easier for amateur radio operators to employ esoteric propagation modes, such as high-speed meteor scatter and moonbounce. Additionally WSJT is able to send signal reports to spotting networks such as PSK Reporter.

An amateur radio propagation beacon is a radio beacon, whose purpose is the investigation of the propagation of radio signals. Most radio propagation beacons use amateur radio frequencies. They can be found on LF, MF, HF, VHF, UHF, and microwave frequencies. Microwave beacons are also used as signal sources to test and calibrate antennas and receivers.

The International Beacon Project (IBP) is a worldwide network of radio propagation beacons. It consists of 18 continuous wave (CW) beacons operating on five designated frequencies in the high frequency band. The IBP beacons provide a means of assessing the prevailing ionospheric signal propagation characteristics to both amateur and commercial high frequency radio users.

<span class="mw-page-title-main">FT8</span> Frequency shift keying digital mode

FT8 or Franke & Taylor 8 is a frequency shift keying digital mode of radio communication used by amateur radio operators worldwide. Following release on June 29, 2017, by its creators Joe Taylor, K1JT, and Steve Franke, K9AN, along with the software package WSJT, FT8 was adopted rapidly and, in little over two years, it became the most popular digital mode recorded by automatic spotting networks such as PSK Reporter. FT8DMC is the most important club dedicated to this mode of digital communication.

The 5-meter band (60 MHz) is the middle portion of the very high frequency (VHF) radio spectrum allocated to amateur radio use.

<span class="mw-page-title-main">Yaesu FT-891</span> Amateur radio transceiver

The Yaesu FT-891 is a HF and 6 meters all mode mobile amateur radio transceiver. The FT-891 was first announced to the public by Yaesu at the 2016 Dayton Hamvention. The radio has 100 watts output on CW, SSB, and FM modulations and 25 watts of output in AM. As a mobile transceiver the FT-891 is well suited for mobile installation in vehicles, and weighing less than 5 pounds it is often used for field activations such as Summits On The Air and Parks On The Air. The radio has been praised for its noise reduction and sensitive receiver. Common criticisms of the radio include its many menus that are difficult to navigate with its small screen, the lack of VHF/UHF capabilities, and lack of an internal antenna tuner. Although the radio lacks an internal sound card it still has input and output jacks for audio and be controlled over a USB cable allowing the radio to use digital modes such as WinLink, PSK31 and FT8.

The ICOM IC-7100 is a multimode HF/VHF/UHF mobile amateur radio transceiver. The IC-7100 has support for a wide variety of commonly used amateur radio modes including ICOMs proprietary digital voice mode DSTAR. Additionally the radio offers 100 watts on HF, 50 watts on VHF, and 35 watts on UHF. The IC-7100 is unique in that it has a large detachable control head with a slanted display so the transmitter can be installed elsewhere in a vehicle or home. The receiver used in the IC-7100 is a triple conversion superheterodyne and has excellent DSP and audio filters. The IC-7100 allows for connection to a computer over USB which enables the radio to be used for popular digital modes such as FT8, Winlink, and Packet Operation. Locations of nearby repeaters and sending APRS locations can be done with an optional GPS receiver attachment. Notable features that the IC-7100 lacks is an internal antenna tuner.

References

  1. Gladstone, Philip (2018-02-23). "Pskreporter.info & FT8" (PDF). HamSCI 2018.
  2. Casler, David (2016) PSK Reporter: How You Can Be Part! AD #33 , retrieved 2022-10-06
  3. Taylor, Joseph (2022). "WSJT-X User Guide". WSJT-X. Retrieved 2022-10-06.
  4. van den Hoff, Rob. "PSK reporter | PAØROB". PAØROB Dutch Amateur Radio Station. Retrieved 2022-10-06.
  5. Barron, Robert (2020-02-08). "PSK Reporter". KA5WSS. Retrieved 2022-10-06.
  6. 力武健次. (2020). インターネットとオープンな無線技術の今後. 研究報告セキュリティ心理学とトラスト (SPT), 2020(1), 1-8. https://rand.pepabo.com/papers/iot51-jj1bdx.pdf
  7. "FreeDV Activity Day | Southgate Amateur Radio News". www.southgatearc.org. Retrieved 2022-10-06.
  8. Kinney, Jack (2021). "Getting Stated with JS8/JS8Call" (PDF). Upper Pinellas Amateur Radio Club. Retrieved 2022-10-06.
  9. Peterson, Bill (2018-04-11). "PSKReporter.info: a walk-thur" (PDF). Clallam County Amateur Radio Club, Inc. Retrieved 2022-10-06.
  10. Silver, H. Ward (2021). Ham Radio For Dummies (4th ed.). Hoboken, NJ: Wiley. p. 120. ISBN   978-1-119-69576-9. OCLC   1245417767.{{cite book}}: CS1 maint: date and year (link)
  11. 1 2 Pearce, Nolan; Duncan, Kate J. (2021-03-10). "Simulation and Comparison of Weak-Signal VHF Propagation". SoutheastCon 2021. Atlanta, GA, USA: IEEE. pp. 1–5. doi:10.1109/SoutheastCon45413.2021.9401847. ISBN   978-1-6654-0379-5. S2CID   233333428.
  12. Silver, H. Ward (July 2017), "The Solar Eclipse and Ham Radio", Nuts and Volts Magazine, pp. 50–55, retrieved 2022-10-06
  13. Desmond, John (2021-05-08). "PSK Reporter website passes 20 Billion Reception Records". EI7GL....A diary of amateur radio activity. Retrieved 2022-10-06.
  14. Frissell, N. A.; Miller, E. S.; Kaeppler, S. R.; Ceglia, F.; Pascoe, D.; Sinanis, N.; Smith, P.; Williams, R.; Shovkoplyas, A. (2014-10-22). "Ionospheric Sounding Using Real-Time Amateur Radio Reporting Networks: FRISSELL ET AL". Space Weather. 12 (12): 651–656. doi:10.1002/2014SW001132. S2CID   53355527.
  15. Frissell, Nathaniel A.; Kaeppler, Stephen R.; Sanchez, Diego F.; Perry, Gareth W.; Engelke, William D.; Erickson, Philip J.; Coster, Anthea J.; Ruohoniemi, J. Michael; Baker, Joseph B. H.; West, Mary Lou (2022-03-16). "First Observations of Large Scale Traveling Ionospheric Disturbances Using Automated Amateur Radio Receiving Networks". Geophysical Research Letters. 49 (5). Bibcode:2022GeoRL..4997879F. doi:10.1029/2022GL097879. hdl: 10919/111219 . ISSN   0094-8276. S2CID   247006312.
  16. Nunes, Jose (2021). "There is nothing magic about propagation: In search of MUF isolines" (PDF). Contest University. Retrieved 2022-10-06.
  17. "The K7RA Solar Update". ARRL The National Association for Amateur Radio. 2022-09-23. Retrieved 2022-10-06.
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  19. Kemmerer, Fred (2021-06-06). "A 6m DX Opening to Europe". Nashua Area Radio Society. Retrieved 2022-10-06.
  20. Desmond, John (2020-05-06). "VHF & UHF Trans-Atlantic path between Cape Verde Islands and the Caribbean opens up". EI7GL....A diary of amateur radio activity. Retrieved 2022-10-06.
  21. Buckley, Richard; Furman, William N. (2021-11-29). "Application of Machine Learning Techniques to HF Propagation Prediction". MILCOM 2021 - 2021 IEEE Military Communications Conference (MILCOM). San Diego, CA, USA: IEEE. pp. 623–628. doi:10.1109/MILCOM52596.2021.9653108. ISBN   978-1-6654-3956-5. S2CID   245594949.
  22. Старнавський, І. І.; Швайченко, В. Б. (2020). "Сучасні особливості моніторингу умов поширення радіохвиль". Технології та дизайн (in Ukrainian). ISSN   2304-2605.
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