Measurement of the inner turbulence scale of the interstellar plasma toward the pulsar PSR B2111+46 |
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Authors: | T V Smirnova V I Shishov |
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Institution: | 1.Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Institute of Physics,Russian Academy of Sciences,Pushchino, Moscow oblast’,Russia |
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Abstract: | The pulsar PSR B2111+46 has been observed at 112 MHz, and a new approach to analyzing pulsar pulses scattered in turbulent
interstellar plasma applied. This method is based on the dependence of the normalized energy in the trailing part of a pulse
on the intrapulse time. Since the trailing edge of a pulse follow exponential law to high accuracy, the inner turbulence scale
of the interstellar plasma exceeds the field coherence scale. The measured scattering parameter is τ
sc
= 147 ± 1 ms. Analysis of the parameters of diffractive and refractive scintillations of the pulsar at 610 MHz together with
the 112 MHz data shows that the spectrum of the interstellar plasma toward PSR B2111+46 is a piecewise power law: on scales
of 1013–1014 cm, the exponent of the turbulence spectrum is n ≃ 4, whereas n = 3.5 on scales of 2 × 108−1013 cm. The spectrum flattens with approach to the inner turbulence scale l: n = 3–3.2. The obtained inner turbulence scale is l = (3.5 ± 1.5) × 107 cm. The distribution of the interstellar plasma toward the pulsar is close to statistically homogeneous. The local density
(N
e
= 0.4 cm−3) and filling factor (F = 0.04) of the interstellar plasma have been estimated. The similarity of N
e
estimates obtained from the inner scale of the inhomogeneities and the ratio of the emission measure to the dispersion measure
provides evidence that the inner turbulence scale corresponds to the ion inertial length. |
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Keywords: | |
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