NOAA APT transmissions are right hand circular polarized at frequences around 137 MHz. This requires the use of an antenna designed for receiving such a signal, for example a quadrifilar helix antenna or a turnstile antenna. Since none of these antenna types was available, a simple 137 MHz ground plane antenna was constructed. As usual for this type of antenna, 4 pieces of 12 gauge copper wire were attached with machine screws to a SO-239 UHF-type chassis-mount coaxial socket and a fifth wire was soldered to the center pin. All elements are 52cm in length.
The 137 Mhz ground plane antenna
The plan is to construct a double cross antenna in the near future.
The reciever consists of a FUNcube Dongle and a computer running GNU Radio.
The computer is a Dell Optiplex GX280 with a dual core 3.40 GHz Pentium processor and 3 GB RAM. The operating system is Fedora 12 Linux running a custom 22.214.171.124 kernel. It also has an ASUS Xonar D1 soundcard that is used for various SDR experiments.
FUNcube Dongle is a software defined radio receiver in a USB stick tunable over a range of 64 MHz - 1.7 GHz. It provides I/Q data via USB audio and its control interface (frequency, gains, filters) uses the USB HID api. This particular unit is serial number 980 and has been upgraded to the 18h firmware.
The FUNcube Dongle
GNU Radio is a free software development toolkit that provides the signal processing runtime and processing blocks to implement software radios using readily-available, low-cost external RF hardware and commodity processors. GNU Radio applications are primarily written using the Python programming language, while the supplied, performance-critical signal processing path is implemented in C++.
The GNU Radio portion of the receiver was built using the GNU Radio Companion, a graphical tool for creating signal flow graphs and generating flow-graph source code. It is modeled after a USRP APT receiver by Alexandru Csete (OZ9AEC). The flow chart uses the Funcube Dongle source block for GNU Radio, gr-fcd, also developed by Alexandru Csete. This block wraps both the audio input and the control interface into a GNU Radio source block with a complex data stream output. His web site has more useful GNU Radio information than almost any other site on the web.
The GNU Radio Companion flow graph of the receiver
The major components of the flow graph and their function in the receiver-
The other blocks in the flow graph define either variables or GUI components. The blocks are mostly written in C++. GRC produces a Python executable from the flow graph that basically "glues" the block together.
The receiver in operation
The end result of the receiver's operation is an audio file, a mono wav file with a sample rate of 11025. This audio file is decoded to produce the final image. A sample of the audio is available for download: sample.mp3
The audio file was decoded into the image using atpdec, a command line oriented NOAA POES weather satellite image software decoder. The software is open source and GPL licensed. Decoding the image is as simple as running the command "atpdec audio_file.wav."
There seem to be two types of noise in the image. The white bands are generally the result of poor reception, particularly at lower elevetions of the satellite. The darker bands are interference; the interference can be heard and sounds at times like FM broadcast, and at other times like aviation band.
The image decoded with atpdec
View Full Size Image
NOAA-19 is the last of a series of NOAA POES satellites using an Automatic Picture Transmission system. The satellite was launched on February 6, 2009, and is an 845 x 866 km orbit with an inclination of 98.8° and an orbital period of 102 minutes. This pass, on Saturday, May 29, 2011, was northbound during orbit number 11865. The satellite rose above the local horizon at 17:49:52UT and recording started at 17:52:27UT when the satellite was approximately 10° above the horizon. The satellite was visible for 15:33, of which 10:57 was recorded. The satellite reached a maximum elevation of 64° and at its closest point was 933km from the station.
© 2011 George S. Williams
Terrapin Swamp Radio Observatory