This is a signal acquisition and HRPT decoder component of the STaR project which reads the NOAA 18 and NOAA 19 polar orbiting weather satellites. It is an enhanced version of the GnuRadio gr-noaa module.
- 1 Description
- 2 Graphical Displays
- 3 Software Defined Radio Receivers
- 4 Required Software
- 5 Post-acquisition processing
Use this module in conjunction with a tracking antenna, such as STaR.
This module digitizes the antenna signal and decodes a High Resolution Picture Transmission (HRPT) into a raw file that can be used to produce image and sounder data. Current applicable satellites include NOAA-18 and NOAA-19. Local oscillator mixer frequency, sample rate, and gain can be specified. The module can be run from the GnuRadio Companion or from the command line. For example,
> gr_hrpt_lime.py -d /data/pi/SCRB/process -s noaa-19 -g 28 -f 1698.0e6 -l 1565.0e6
where: gr_hrpt_lime.py is this module using a LimeSDR receiver -d specifies the directory for the output file -s names the satellite -g is the SDR gain -f is the satellite broadcast frequency -l is the LO mixer frequency
This is an enhanced version of the GnuRadio gr-noaa module with some parameter tweaks and added graphics. Different receivers or file input can be used. You can find STaR's version of gr-noaa module at https://gitlab.com/planetaryimaging/STaR under the scripts/noaa directory.
Graphical displays can turned on or off by enabling or disabling them in the GRC glyph code. Depending on compute power, only one or two displays should be active. Display options are given below.
A Root Mean Square power bar is displayed and is a handy and efficient way to gauge the signal.
The time domain display is used to see the voltage range driven by the antenna and SDR amplifiers. Voltages are typically in the range of +- 0.4v to +- 0.8v and can vary depending on the satellite distance from the ground station.
This display gives the relative power gain for the signal in the frequency domain and can show the noise floor. It is also interesting that the Doppler effect can be seen by following the carrier spike as the satellite approaches towards and recedes from the ground station.
The binary phase shift keying can be seen by enabling one of two methods. (TODO: clarify)
Software Defined Radio Receivers
Most current Software Defined Radios (SDR) can be used with this module, as the required sample rate is as low as 2MS. Higher sample rates can also be used. In addition, it is important to consider data delivery interfaces and rates. For example, USB devices inserted into slower USB port versions can impact data delivery. Be sure to check device interfaces with programs like "lsusb".
Based on experience, the input signal power to the SDR can range from -44dBm to -15dBm and is dependent on the acquisition electronics of the antenna rig. The objective is to match the output power from the acquisition to the input power range of the receiver while maintaining maximum linear amplification throughout the stream, including the front-end SDR amplification.
Different rigs and receivers will need to be individually matched to maintain amplification linearity. For example, on a -44dBm input signal to a LimeSDR receiver a relative amplification of 28dB is sufficient to give a -0.6 to 0.6 voltage signal to the digitizer (voltage does vary with satellite distance). Using a greater power range can introduce non-linearities and so minimal input power is generally preferred. Keep in mind that the optimal amplification occurs at the antenna and that subsequent amplifications can distort the signal.
A (draft) list of necessary software to run the NOAA 18,19 module follows below.
SDR Receiver Software
Software Defined Receivers (SDR) have their own software that should be installed, so if you are using a USRP you should install the software from https://Ettus.com, or using a LimeSDR install software from https://myriadrf.org, or an RTL-SDR install software from https://osmosdr.org, etc. You should consider downloading the Osmosdr software even if you are not using RTL-SDR receivers as they provide an API for other receivers (USRP, LimeSDR included). Hints: Install the receiver code in /usr/local (default) before installing GnuRadio. Also, be sure to test the receiver with its own software before using it with GnuRadio.
Download locations (not all are needed, just the ones to acquire):
UHD git clone --recursive https://github.com/EttusResearch/uhd.git
RTL-SDR git clone git://git.osmocom.org/rtl-sdr.git use: cmake -DINSTALL_UDEV_RULES=ON -DDETACH_KERNEL_DRIVER=ON ../
SOAPYSDR git clone --recursive https://github.com/pothosware/SoapySDR.git
SOAPYUHD git clone --recursive https://github.com/pothosware/SoapyUHD.git
The NOAA 18,19 module has been tested on GnuRadio version 188.8.131.52. Previous versions may work. Be sure to install the SDR receiver software first so that GnuRadio installer can find them. If you add a new receiver later you can re-run the GnuRadio install to incorporate it. Be sure to include the GnuRadio Companion in the install.
NOTE: I do not install receiver software or GnuRadio from package managers as these have a tendency to trip over each other. I install from source in /usr/local/src and recommend the default locations (/usr/local/bin,/usr/local/lib, etc.).
GnuRadio is now at version 3.8 and is a substantial revision from 3.7. The out-of-tree modules used in this module have not been ported to 3.8 and will require some effort. To get the 184.108.40.206 version go to https://www.gnuradio.org/releases/gnuradio and download the tarball.
Below are the post-acquisition packages used in STaR for the NOAA18,19 satellites.
Terrenus HRPT 2.2 package
A Java-based, High Resolution Picture Transmissio (HRPT) ingestor from Terrenus Earth Sciences http://www.terrenus.ca/ is used to produce an intermediate data file that is value calibrated and georeferenced but not projected. The program hrptingest takes a raw HRPT file (eg. In STaR, output from the gr-hrpt module) and produces a NetCDF output file which is used in the CoastWatch package described below. Note that raw HRPT file may need to be byte swapped.
Visible band radiance (reflections) calibration requires an external file found in the $HRPT_HOME/resource/orbit directory, one for each satellite, eg. noaa18.properties, noaa19.properties. This file contains the coefficients needed to adjust the visible radiance and should be updated monthly from data available at https://www.ospo.noaa.gov/Products/ppp/notices.html.
Calibration coefficients to update with typical values: avhrr.ch1.s1 = 0.05203 avhrr.ch1.i1 = -2.023 avhrr.ch1.s2 = 0.1535 avhrr.ch1.i2 = -52.76 avhrr.ch1.cut = 496.43
avhrr.ch2.s1 = 0.05909 avhrr.ch2.i1 = -2.292 avhrr.ch2.s2 = 0.1760 avhrr.ch2.i2 = -60.76 avhrr.ch2.cut = 500.37
Orbital two line elements (TLE)
The hrptingest program requires an external file for the orbital elements (TLE) for each satellite and is found in the $HRPT_HOME/resource/orbit directory, eg. noaa18.txt, noaa19.txt. The STaR package provides the script $STAR_HOME/aux/getelements_terrenus which retrieves the current TLEs and appends them to the satellite TLE file. If the HRPT package is installed in /usr/local then root will have to update the files, in a crontab or manually.
Review the script "hrpt_process" for implementation details.