12 January, 1999
min. -31.1 C
max. -27.7 C
Wind Chill -39
If the microphones on string #13 of the AMANDA telescope would work properly, we could listen to the ice move. If the ice above the bedrock that carried the telescope with it moved in a stop/start fashion it would sound more noisy, and the resulting friction between the ice and rock may produce light that may interfere with AMANDA's eyesight, or "seeing." It may also be that in the future sound may also be used to detect the presence of neutrinos.
The sound of the blast would travel through the ice at about 3,840 meters/second and hopefully be received in the 7Hz - 5 kHz frequency range of the micropohones. By comparison, we hear sound in the 30 Hz - 20 kHz range and a speaking voice ususally falls within the 400Hz - 3kHz frequency range. The hydrophones were attached to the string
at a depth of 2,250 and 2,350 meters beneath the surface of the ice; the last 100 meters of the string.
About mid-morning, Ryan stood by the oscilloscope and adjusted it's settings. The spike of sound received from the blast would have to
be large enought to go beyond the background noise now registering on the scope.
I was outside the Martin A. Pomerantz Observatory (MAPO) with "Blaster" John Wright holding a spool of detonation cable containing explosive. John knelt by the pit that was 48 meters deep and 15 meters away from string #13. When everything was ready, we communicated through walkie-talkie (radio) with Ryan inside
John shouted "Fire in the hole!" A geyser of white and red was followed by a loud boom. The test hole had caved in from the blast. Ryan radioed that he saw the spike of the blast register on the microphone at 2,250 meters below the ice. Much to his delight,
later, after filtering out the rest of the background interference, he found the second spike--that of the microphone at the bottom
of the string, 2,350 meters below the surface. The mikes still worked having weathered being buried in the ice for a year.
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