Skip to main content

INTERSTELLAR TURBULENT PLASMA SPECTRUM IN THE WIDE REGION OF TURBULENCE SCALES FROM OBSERVATIONS OF PULSARS

Buy Article:

$63.00 plus tax (Refund Policy)

We present here the results of studying of interstellar plasma inhomogeneities spectrum based on different kinds of pulsar observations. Using the theory of diffractive and refractive scintillation and pulsar observations at different frequencies, we construct a composite structure function of phase fluctuations in the wide region of turbulence scales: <$>(10^{6} \div 10^{17})\,\hbox{m}<$>. We found that an outer scale of plasma spectrum is about <$>10^{15}\,\hbox{m}<$> and for scales <$>(10^{6} \div 10^{14})\,\hbox{m}<$> the spectrum is close to Kolmogorov one.
No Reference information available - sign in for access.
No Citation information available - sign in for access.
No Supplementary Data.
No Data/Media
No Metrics

Document Type: Research Article

Affiliations: Pushchino Radio Astronomy Observatory of Lebedev Physical Institute, 142290, Pushchino, Russia

Publication date: 2002-01-01

More about this publication?
  • Access Key
  • Free content
  • Partial Free content
  • New content
  • Open access content
  • Partial Open access content
  • Subscribed content
  • Partial Subscribed content
  • Free trial content
Cookie Policy
X
Cookie Policy
Ingenta Connect website makes use of cookies so as to keep track of data that you have filled in. I am Happy with this Find out more