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Pickering XV-15 150



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Brand: Pickering

The Pickering XV-15 150 is a type of specialized radio telescope designed for very high frequency (VHF) observations. It is part of the larger Pickering Observatory, which is located in Whitby, Ontario, Canada. The XV-15 150 has a parabolic dish reflector with a diameter of 150 meters, making it one of the largest radio telescopes in the world. It is primarily used for experiments in atmospheric physics, as well as studies of the sun, stars, interstellar molecular clouds, and other astronomical targets in the VHF range (30-300 MHz). The antenna's current research activities include investigating ionospheric scatter, studying the polarization of radio waves, and detecting small variations in the Earth's magnetic field.



  • Type: Moving Magnet
  • Output Voltage:
  • Freq Response:
  • Tracking Force: 2.0 - 4.0 g
  • Mass: 6.3 g
  • Channel Separation:
  • Channel Balance:
  • Load Impedance: 47k Ω
  • Output Impedance:
  • Stylus:
  • Stylus Tip:
  • Cantilever:
  • Dynamic Compliance:
  • Static Compliance:
  • Price:

Pickering XV-15 150

Pickering XV-15 150



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