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Fig. 1. | Earth, Planets and Space

Fig. 1.

From: Solar wind and its evolution

Fig. 1.

Structures of corona and solar wind for different 〈dv〉 = 0.4 (blue), 0.7 (black dashed), and 1.4 km s−1 (red). I plot solar wind speed, vr (km s−1) (top left), temperature, T (K) (top right), density in logarithmic scale, log(ρ(g cm−3)) (bottom right), and rms transverse velocity, 〈dv〉 (km s−1) (bottom left). Each variable is averaged with respect to time during 28 min (the longest wave period considered).

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