1 Some theorists even believe that solar wind particles hitting the atmosphere may trigger cloud formation.

2 Daedalus now points out that the solar wind is an exactly similar phenomenon.

3 Between the bow shock and the magnetopause the solar wind is greatly decelerated.

4 The solar wind loses its identity in the interstellar medium at a distance no less than that of the outer planets.

5 Kulcinski argues that the solar wind has implanted great quantities of hydrogen and helium into the lunar regolith.

6 When the solar wind is strong the magnetopause retreats to about 50 R J upwind.

7 Solar wind to shield Earth during pole flip New Scientist - May 2004.

8 Many photogenic auroras have been triggered from a solar wind stream that recently passed the Earth.

9 Once the transfer of energy from the solar wind abates , the flow of plasma into the inner magnetosphere slows, and ions are lost from the ring current more rapidly than new ones arrive.

10 But fortunately, most of the solar wind particles have been kept out of the Earth magnetosphere.

11 The final speed of the solar wind depends mainly on the maximum temperature in the corona.

12 Shielded from the buffeting of the solar wind, ions quietly leak out of the atmosphere.

13 The origin of the solar wind in the hot sun's outer atmosphere, the corona that well - known.

14 The phenomenon is produced by the action of solar wind on the atmosphere at Earth's Poles.

15 Solar wind: What you do there are a broom, I can sweep clean for you ... ...

16 What if you could generate your own solar wind with laser and particle beam technology?

17 The solar wind protons must sputter away the surface atoms of the dust.

18 "When the solar wind blows out plasma it too causes a bubble: the heliosphere,[]" he explains.

19 The lunar surface also contains the light isotope helium-3, which is implanted in the surface by the solar wind.

20 It is true that the Sun emits helium-3 in the solar wind, and that in principle we could intercept it.

21 An obvious question is whether the surfaces of the asteroids might be rich in helium-3 implanted by the solar wind.

22 Eruptions on the Sun inject high-speed particles into the solar wind, and these can cause geomagnetic disturbances on reaching the Earth.

23 Lab testing is underway on a similar concept that would form a magnetic shield around a ship, protecting it from harmful solar wind particles.

24 The gas pressure eventually overcomes the force of solar gravity and the corona inevitably expands into space as the solar wind .

25 A continuous stream of charged particles , called the solar wind, impinges on the earth's magnetosphere.

26 The mass - loss includes the light radiation and solar wind.

27 This energy involves tons of charged particles, hurled our way in the so - called solar wind.

28 Physics of Solar System Plasmas provides a comprehensive introduction to the plasma physics and magnetohydrodynamics that are needed to study the solar wind and magnetosphere.

29 Under certain condition of the interplanetary magnetic field, a portion of them can reach the shadow region which is usually considered to be devoid of solar wind protons.

30 The moon's lunar soil is chock-full of helium reserves, thanks to the solar wind.

31 Often considered the stuff of science fiction, sailing through space was suggested 400 years ago by astronomer Johannes Kepler who observed comet tails blown by the solar wind.

32 A burst of solar wind—charged particles from the sun—struck Earth on Tuesday, triggering auroras as far south as Michigan, as seen in this picture taken from the shores of Lake Superior in Marquette.

33 Arriving in 2014, the Mars Atmosphere and Volatile Evolution Mission (MAVEN) will see if the solar wind and radiation are behind the loss of the Martian atmosphere.

34 Under these circumstances, reconnection takes place along a wide equatorial belt, opening up nearly the entire outer boundary of the magnetosphere to the solar wind.

35 EUGENE N. PARKER is the world's leading expert on interplanetary gas and magnetic fields. He is best known for hypothesizing and explaining the solar wind in 1958.

36 Hydrogen atoms are more abundant than either helium or oxygen but their low mass means they are easily swept aside by the high-speed solar wind and can't readily be detected.

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37 The flux ropes offered channels for the transport of the solar wind plasma into the magnetosphere and the escape of the magnetospheric plasma into the interplanetary space.

38 Caption :The lunar module's starboard footpad and contact probe. In the background are the solar wind experiment, flag and camera.

39 The transfer of magnetic energy from the solar wind radically alters the shape of the magnetosphere.

40 The most likely explanation for the comet-like feature is that the star's solar wind—actually a stream of charged particles—is evaporating the gas giant a bit at a time, astronomers say.

41 Tarduno and Eric Mamajek, an astronomer at the University of Rochester, used observations of young sunlike stars to infer how strong a solar wind the Earth was up against.

42 So this really changes our understanding of solar wind - magnetosphere coupling thealso at the press conference.

43 The solar wind does not impinge directly on the earth and its atmosphere, however.

44 Fig . 3 The time evolution curve of solar wind radial speed incited by disturbance propagation.