Nature, Količina 454Sir Norman Lockyer Macmillan Journals Limited, 2008 |
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Stran 78
... Plasma waves are a characteristic feature of shocks in plasmas , and are produced by non - thermal particle ... plasma - wave electric fields at the solar wind termination shock . The observations were obtained from the plasma - wave ...
... Plasma waves are a characteristic feature of shocks in plasmas , and are produced by non - thermal particle ... plasma - wave electric fields at the solar wind termination shock . The observations were obtained from the plasma - wave ...
Stran 79
... plasma teams , although there are variations in the magnetic field ' around this time . No plasma waves were detected at TS - 2 . 9,10 plasma oscillations , a series of five closely spaced crossings of the : ermination shock were ...
... plasma teams , although there are variations in the magnetic field ' around this time . No plasma waves were detected at TS - 2 . 9,10 plasma oscillations , a series of five closely spaced crossings of the : ermination shock were ...
Stran 80
... plasma density with increasing radial distance ( R ) from the Sun. If the electric field spectral densities are normalized by dividing by the solar wind energy density and the frequencies are normalized by dividing by the electron plasma ...
... plasma density with increasing radial distance ( R ) from the Sun. If the electric field spectral densities are normalized by dividing by the solar wind energy density and the frequencies are normalized by dividing by the electron plasma ...
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