Volume 25 Issue 5
Sep.  2005
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M. V. Eselevich, V. G. Eselevich. Fractal Structure of the Heliospheric Plasma Sheet at the Earth's Orbit[J]. Chinese Journal of Space Science, 2005, 25(5): 333-337. doi: 10.11728/cjss2005.05.333
Citation: M. V. Eselevich, V. G. Eselevich. Fractal Structure of the Heliospheric Plasma Sheet at the Earth's Orbit[J]. Chinese Journal of Space Science, 2005, 25(5): 333-337. doi: 10.11728/cjss2005.05.333

Fractal Structure of the Heliospheric Plasma Sheet at the Earth's Orbit

doi: 10.11728/cjss2005.05.333
  • Received Date: 1900-01-01
  • Rev Recd Date: 1900-01-01
  • Publish Date: 2005-09-15
  • An analysis of the data from the Wind and IMP-8 spacecraft revealed that a slow solar wind,flowing in the heliospheric plasma sheet, represents a set of magnetic tubes with plasma of increased density(N > 10cm-3 at the Earth's orbit). They have a fine structure at several spatial scales (fractality), from2°-3° (at the Earth's orbit, it is equivalent to 3.6-5.4 h, or(5.4-8.0) × 106 km) to the minimum about0.025°, i.e. the angular siz.e of the nested tubes is changed nearly by two orders of magnitude. The magnetic tubes at each observed spatial scale are diamagnetic, i.e. their surface sustains a flow of diamagnetic (or drift)current that decreases the magnetic field within the tube itself and increases it outside the tube. Furthermore,the value of β = 8π[N(Te + Tp)]/B2 within the tube exceeds the value of β outside the tube. In many cases total pressure P = N(Te + Tp) + B2/8π is almost constant within and outside the tubes at any one of the aforementioned scales.

     

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