WSPR: RaspberryPi

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Raspberry Pi bareback LF/MF/HF/VHF WSPR transmitter

Makes a very simple WSPR beacon from your RasberryPi by connecting GPIO port to Antenna (and LPF), operates on LF, MF, HF and VHF bands from 0 to 250 MHz.

It is now compatible with both the original Raspberry Pi and the Raspberry Pi 2.

Installation / update:

 Make sure you are using the latest kernel by updating your system. The latest
 kernel includes fixes wich improve NTP ppm measurement accuracy:
   sudo apt-get update
   sudo apt-get dist-upgrade
 Download and compile code:
   sudo apt-get install git
   git clone https://github.com/JamesP6000/WsprryPi.git
   cd WsprryPi
   make
 See the accompanying BUILD file for more details.

Usage: (WSPR --help output):

 Usage:
   wspr [options] callsign locator tx_pwr_dBm f1 <f2> <f3> ...
     OR
   wspr [options] --test-tone f
 Options:
   -h --help
     Print out this help screen.
   -p --ppm ppm
     Known PPM correction to 19.2MHz RPi nominal crystal frequency.
   -s --self-calibration
     Call ntp_adjtime() before every transmission to obtain the PPM error of the xtal.
   -r --repeat
     Repeatedly, and in order, transmit on all the specified freqs.
   -x --terminate <n>
     Terminate after n transmissions have been completed.
   -o --offset
     Add a random frequency offset to each transmission:
       +/- 80 Hz for WSPR
       +/- 8 Hz for WSPR-15
   -t --test-tone freq
     Simply output a test tone and the specified frequency. Only used
     for debugging and to verify calibration.
   -n --no-delay
     Transmit immediately, do not wait for a WSPR TX window. Used
     for testing only.
 Frequencies can be specified either as an absolute TX carrier frequency, or
 using one of the following strings. If a string is used, the transmission
 will happen in the middle of the WSPR region of the selected band.
   LF LF-15 MF MF-15 160m 160m-15 80m 60m 40m 30m 20m 17m 15m 12m 10m 6m 4m 2m
 -15 indicates the WSPR-15 region of band .
 Transmission gaps can be created by specifying a TX frequency of 0
 
 Note that 'callsign', 'locator', and 'tx_power_dBm' are simply used to fill
 in the appropriate fields of the WSPR message. Normally, tx_power_dBm should
 be 10, representing the signal power coming out of the Pi. Set this value
 appropriately if you are using an external amplifier.

Radio licensing / RF:

 In order to transmit legally, a HAM Radio License is REQUIRED for running
 this experiment. The output is a square wave so a low pass filter is REQUIRED.
 Connect a low-pass filter (via decoupling C) to GPIO4 (GPCLK0) and Ground pin
 of your Raspberry Pi, connect an antenna to the LPF. The GPIO4 and GND pins
 are found on header P1 pin 7 and 9 respectively, the pin closest to P1 label
 is pin 1 and its 3rd and 4th neighbour is pin 7 and 9 respectively. See this
 link for pin layout: http://elinux.org/RPi_Low-level_peripherals Examples of
 low-pass filters can be found here: http://www.gqrp.com/harmonic_filters.pdf
 The expected power output is 10mW (+10dBm) in a 50 Ohm load. This looks
 neglible, but when connected to a simple dipole antenna this may result in
 reception reports ranging up to several thousands of kilometers.
 As the Raspberry Pi does not attenuate ripple and noise components from the
 5V USB power supply, it is RECOMMENDED to use a regulated supply that has
 sufficient ripple supression. Supply ripple might be seen as mixing products
 products centered around the transmit carrier typically at 100/120Hz.
 DO NOT expose GPIO4 to voltages or currents that are above the specified
 Absolute Maximum limits. GPIO4 outputs a digital clock in 3V3 logic, with a
 maximum current of 16mA. As there is no current protection available and a DC
 component of 1.6V, DO NOT short-circuit or place a resistive (dummy) load
 straight on the GPIO4 pin, as it may draw too much current. Instead, use a
 decoupling capacitor to remove DC component when connecting the output dummy
 loads, transformers, antennas, etc. DO NOT expose GPIO4 to electro- static
 voltages or voltages exceeding the 0 to 3.3V logic range; connecting an
 antenna directly to GPIO4 may damage your RPi due to transient voltages such
 as lightning or static buildup as well as RF from other transmitters
 operating into nearby antennas. Therefore it is RECOMMENDED to add some form
 of isolation, e.g. by using a RF transformer, a simple buffer/driver/PA
 stage, two schottky small signal diodes back to back.

TX Timing:

 This software is using system time to determine the start of WSPR
 transmissions, so keep the system time synchronised within 1sec precision,
 i.e. use NTP network time synchronisation or set time manually with date
 command. A WSPR broadcast starts on an even minute and takes 2 minutes for
 WSPR-2 or starts at :00,:15,:30,:45 and takes 15 minutes for WSPR-15. It
 contains a callsign, 4-digit Maidenhead square locator and transmission
 power.  Reception reports can be viewed on Weak Signal Propagation Reporter
 Network at: http://wsprnet.org/drupal/wsprnet/spots

Calibration:

 Frequency calibration is REQUIRED to ensure that the WSPR-2 transmission
 occurs within the narrow 200 Hz band. The reference crystal on your RPi might
 have an frequency error (which in addition is temp. dependent -1.3Hz/degC
 @10MHz). To calibrate, the frequency might be manually corrected on the
 command line or a PPM correction could be specified on the command line.
 NTP calibration:
 NTP automatically tracks and calculates a PPM frequency correction. If you
 are running NTP on your Pi, you can use the --self-calibration option to
 have this program querry NTP for the latest frequency correction before
 each WSPR transmission. Some residual frequency error may still be present
 due to delays in the NTP measurement loop and this method works best if your
 Pi has been on for a long time, the crystal's temperature has stabilized,
 and the NTP control loop has converged.
 AM calibration:
 A practical way to calibrate is to tune the transmitter on the same frequency
 of a medium wave AM broadcast station; keep tuning until zero beat (the
 constant audio tone disappears when the transmitter is exactly on the same
 frequency as the broadcast station), and determine the frequency difference
 with the broadcast station. This is the frequency error that can be applied
 for correction while tuning on a WSPR frequency.
 Suppose your local AM radio station is at 780kHz. Use the --test-tone option
 to produce different tones around 780kHz (eg 780100 Hz) until you can
 successfully zero beat the AM station. If the zero beat tone specified on the
 command line is F, calculate the PPM correction required as:
 ppm=(F/780000-1)*1e6 In the future, specify this value as the argument to the
 --ppm option on the comman line. You can verify that the ppm value has been
 set correction by specifying --test-tone 780000 --ppm <ppm> on the command
 line and confirming that the Pi is still zero beating the AM station.

PWM Peripheral:

 The code uses the RPi PWM peripheral to time the frequency transitions
 of the output clock. This peripheral is also used by the RPi sound system
 and hence any sound events that occur during a WSPR transmission will
 interfere with WSPR transmissions. Sound can be permanently disabled
 by editing /etc/modules and commenting out the snd-bcm2835 device.

Example usage:

 Brief help screen
   ./wspr --help
 Transmit a constant test tone at 780 kHz.
   sudo ./wspr --test-tone 780e3
 Using callsign N9NNN, locator EM10, and TX power 33 dBm, transmit a single
 WSPR transmission on the 20m band using NTP based frequency offset
 calibration.
   sudo ./wspr --self-calibration N9NNN EM10 33 20m
 Transmit a WSPR transmission slightly off-center on 30m every 10 minutes for
 a total of 7 transmissions, and using a fixed PPM correction value.  sudo
   sudo ./wspr --repeat --terminate 7 --ppm 43.17 N9NNN EM10 33 10140210 0 0 0 0
 Transmit repeatedly on 40m, use NTP based frequency offset calibration,
 and add a random frequency offset to each transmission to minimize collisions
 with other transmissions.
   sudo ./wspr --repeat --offset --self-calibration N9NNN EM10 33 40m



Usage:

 sudo ./wspr <[prefix]/callsign[/suffix]> <locator> <power in dBm> [<frequency in Hz> ...]
       e.g.: sudo ./wspr PA/K1JT JO21 10 7040074 0 0 10140174 0 0
       where 0 frequency represents a interval for which TX is disabled,
       wspr-2 or wspr-15 mode selection based on specified frequency.
 WSPR is used on the following frequencies (local restriction may apply):
    LF   137400 - 137600
         137600 - 137625 (WSPR-15)
    MF   475600 - 475800
         475800 - 475825 (WSPR-15)
   160m  1838000 - 1838200
         1838200 - 1838225 (WSPR-15)
    80m  3594000 - 3594200
    60m  5288600 - 5288800
    40m  7040000 - 7040200
    30m  10140100 - 10140300
    20m  14097000 - 14097200
    17m  18106000 - 18106200
    15m  21096000 - 21096200
    12m  24926000 - 24926200
    10m  28126000 - 28126200
     6m  50294400 - 50294600
     4m  70092400 - 70092600
     2m  144490400 -144490600


Reference documentation:

 http://www.raspberrypi.org/wp-content/uploads/2012/02/BCM2835-ARM-Peripherals.pdf
 http://www.scribd.com/doc/127599939/BCM2835-Audio-clocks
 http://www.scribd.com/doc/101830961/GPIO-Pads-Control2
 https://github.com/mgottschlag/vctools/blob/master/vcdb/cm.yaml
 https://www.kernel.org/doc/Documentation/vm/pagemap.txt

Credits:

 Credits goes to Oliver Mattos and Oskar Weigl who implemented PiFM [1]
 based on the idea of exploiting RPi DPLL as FM transmitter.
 Dan MD1CLV combined this effort with WSPR encoding algorithm from F8CHK,
 resulting in WsprryPi a WSPR beacon for LF and MF bands.
 Guido PE1NNZ <pe1nnz@amsat.org> extended this effort with DMA based PWM
 modulation of fractional divider that was part of PiFM, allowing to operate
 the WSPR beacon also on HF and VHF bands.  In addition time-synchronisation
 and double amount of power output was implemented.
 James Peroulas <james@peroulas.com> added several command line options, a
 makefile, improved frequency generation precision so as to be able to
 precisely generate a tone at a fraction of a Hz, and added a self calibration
 feature where the code attempts to derrive frequency calibration information
 from an installed NTP deamon.  Furthermore, the TX length of the WSPR symbols
 is more precise and does not vary based on system load or PWM clock
 frequency.



Referensi