The solar wind and solar escape velocity
Acording to your web site, the particles in the solar wind are leaving the Sun at about 400 km/s. That is less than the escape velocity from the surface of the Sun, which is about 600 km/s. Does it mean many of these particles will eventually fall back to the Sun? Is there any evidence of such as behaviour?
Reply
The solar wind does not start from the Sun's surface, but from the corona, and is accelerated somewhat gradually. Obviously, it has to overcome solar gravity, which I suspect is one of the conditions needed for accelerating the solar wind--maybe like a lid on a pressure cooker, holding down the hot corona until it can just barely escape.
You might want to look up
http://www.phy6/org/ Education/FAQs6.html#q82
Incidentally. NASA has been toying for years with the idea of a solar probe, approaching the Sun within 4 solar radii--following boost from a "hairpin" orbit around Jupiter (mentioned briefly in
http://www.phy6.org/stargaze/Stostars.htm
and in the page following it). It would be shielded from the Sun's intense heat by an "umbrella" of tungsten or similar material, and would study the solar wind in its source region. How can it do so with a metal barrier between it and the Sun? Simple: at closest approach is moves at about 300 km/s, so in its own frame of reference, solar wind particles (unlike sunlight) would seem to come in from the side, at an angle. They would seem to have the vector sum of their own velocity and that of the corona relative to the fast-moving probe.