By Nicole Meyer-Vernet
Advent to sunlight wind for researchers and graduate scholars in atmospheric physics and astrophysics.
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Additional info for Basics of the Solar Wind
24 refers to a highly idealised situation, the real corona might sometimes resemble it, as suggested by Fig. 25, which is an old drawing of the visual appearance of the corona during a solar eclipse . One must be cautious in interpreting such visual appearances since they result from diﬀerent structures lying along the line of sight of the observer, and projection eﬀects can be misleading. However, the ﬁgure suggests a current sheet extending into space near the solar magnetic equatorial plane, that separates regions of opposite magnetic polarities.
271. -P. 1980, The scientiﬁc objectives of the international solar polar mission, Phil. Trans. Roy. Soc. London A 297 565. -P. 1992, The Ulysses mission, Astron. Astrophys. Suppl. Ser. 92 207.  Zirker, J. B. 2002, Journey from the Center of the Sun, Princeton University Press. 2 Tool kit for space plasma physics Most of the Universe is made of plasma. And yet, plasmas are very rare on the Earth, where solids, liquids and gases – the three primary states of matter – are ubiquitous (Fig. 1). These states are the result of a competition between thermal energy and intermolecular forces.
Ser. 92 237), and the density from thermal noise analysis of data from the URAP instrument (Stone, R. G. et al. 1992, Astron. Astrophys. Suppl. Ser. 92 291), that are the best ways of measuring these respective properties on Ulysses (Issautier, K. et al. 1999, J. Geophys. Res. 104 6691). 22 Solar wind speed as a function of heliocentric latitude, plotted in polar co-ordinates during Ulysses’ ﬁrst two orbits. 95 µm). e. the distance from the centre is proportional to the speed at each latitude. The left and right panels show the ﬁrst and second orbits, which took place respectively around solar activity minimum and maximum.
Basics of the Solar Wind by Nicole Meyer-Vernet