Indicating the Deep Structure (Below the Icy and Liquid Layers) of Europa and Titan by Measurements with a Giant Solenoid System on Board of an Orbiting Space Probe

Details Indicating the Deep Structure (Below the Icy and Liquid Layers) of Europa and Titan by Measurements with a Giant Solenoid System on Board of an Orbiting Space Probe Indicating the Deep Structure (Below the Icy and Liquid Layers) of Europa and Titan by Measurements with a Giant Solenoid System on Board of an Orbiting Space Probe

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001iaop.work...28f&link_type=abstract

Forum on Innovative Approaches to Outer Planetary Exploration 2001-2020, p. 28

Computer Science

Satellite Surfaces, Planetary Crusts, Ice, Europa, Titan, Near Fields, Oscillators

Scientific paper

We propose a large, few wind solenoid experiment to measure on a circular orbit the depth of the ice crust of Europa and Titan. The solenoid is orbiting the Jovian or Saturnian satellite, it represents an oscillator with ultralong wavelength (from 100 Hz to 40,000 Hz). The diameter of the few wind solenoid may be between 200 m and 800 m. The oscillator is established as a putch-hull oscillator. We use the solenoid as a special antenna. We do not use it as a radar, so we do not consider its far field. Instead of it, we use the near field of the antenna. The near field of the antenna can be deduced from the emitted and received oscillation. In an ideal case the near field is pi/2 phase delayed as compared to their field of the antenna. In a real case the phase delay between the two fields (because of the losses in the near field) is a little bit different from pi/2 phase delayed. This difference from pi/2 is caused by the ice covered deep mountains (if they exist) below the icy crust of Europa or Titan. By this measurement it can be derived that how deep is the rocky material below the volatile ice and liquid spheres. Additional information is contained in the original extended abstract.

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