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By Arthur Pehr Robert Wadlund

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Here, the VPOL signals were further split into four separate paths, with each signal path filtered into one of four bands, shown in Fig. 15: • • • • Low: 200–350 MHz Mid: 350–700 MHz High: 600–1,150 MHz Full: 150–1,250 MHz The filtered sub-band channel signals were then passed through a tunnel diode, also situated in the SHORT. The tunnel diode effectively acted as a square law detector and output a unipolar pulse that tracked the power passed through the diode. The SHORT outputs were then fed into a field-programmable gate array (FPGA), mounted on the relevant SURF board for the channel in question.

Rev. Lett. 0035] 5. S. Hoover, in A Search for Ultrahigh-Energy Neutrinos and Measurement of Cosmic Ray Radio Emission with the Antarctic Impulsive Transient Antenna, PhD thesis, (University of California, Los Angeles, 2010) 6. W. , Phys. Rev. 2961] 7. A. Vieregg, in The Search for Astrophysical Ultra-High Energy Neutrinos Using Radio Detection Techniques, PhD thesis, (University of California, Los Angeles, 2010) 8. The AMANDA Collaboration, M.

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Absolute X-Ray Wave-Length Measurements by Arthur Pehr Robert Wadlund


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