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FPGAs and DSPs unite in solar studies

A Sundance Multiprocessor Technology product story
Edited by the Electronicstalk editorial team Jul 31, 2007

Two Sundance boards will provide image acquisition and camera control on the Sunrise mission to study the structure and dynamics of the solar magnetic field.

Sunrise is a mission to study the structure and dynamics of the solar magnetic field.

The Instituto de Astrofisica de Andalucia (CSIC) in collaboration with other research institutes are in charge of designing the IMaX imaging magnetograph experiment.

IMaX is an experimental solar magnetograph that produces very high resolution vector magnetograms of the solar surface with a spatial resolution of 70km.

IMaX is one of the post focal instruments of the Sunrise mission that contains a 1m-aperture telescope.

The stratospheric balloon is planned to fly for 10-12 days from Antarctica in the basket of the NASA Long Duration Stratospheric Balloon.

Image acquisition and camera control is made with two dedicated SMT374 boards, each combining FPGAs with digital signal processors.

The FPGAs' main tasks are camera control, image accumulation and preprocessing (demodulating the Stokes signals).

The DSPs are in charge of compressing the image with a lossless algorithm.

The DSP master synchronises the host computer, the acquisition and demodulation logic, the optical devices logic, and the other three DSP coprocessors.

The coprocessors are used for the lossless JPEGLS compression of images.

Communication between DSPs is done through a proprietary bus called IMaXBus: a hardware and software layer that abstracts the connections between DSPs and FPGA.

As information transferred through the IMaxBus is accessed by a custom SDRAM controller, all memory operations use long bursts making the whole system very efficient.

It allows the images to be directly transferred from one CCD (connected to the DSP master) to any other DSP in the system.

The images are demodulated, compressed and sent to the DSP master.

A header is added to every image and then it is sent to the host for further processing, telemetry and storage.

The continuation of IMaX project includes the integration and calibration tests with solar light (2007), integration in the Sunrise platform (2008) and polar flight (2009).

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