What  is the difference between Solar Wind and Stellar wind in Time / space?
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A solar wind is a stream of charged particles (i.e., a plasma) which are ejected from the upper atmosphere of a star. When originating from stars other than the Earth's Sun, it is sometimes called a stellar wind.
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A day is the length of time that it takes for the earth to rotate once. There is a slight difference depending on whether you use the sun for the reference point or a star. The solar day (when the sun is used) is 24 hours. The siderial day (when a star is used) is 23 hours 56 minutes. The difference is because the earth also orbits the sun and so it takes a bit longer to realign with the sun than it does with a star.
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Depends on what you mean by better.  I would say neither actually, because they both produce dangerous waste products.  Nuclear breeder reactors are probably the safest way to produce energy (limiting myself to the two choices you provided) since there are no dangerous byproducts.  Unfortunately, both of these energy forms are from limited resources (as far as we know).  I think we should be tapping into wind and solar (particularly) more than rather finite, polluting energy sources.  Hell, why not build solar fields on the opposite side of the moon and beam the energy via satellites and microwaves?  Oh well, what do I know?
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there is no word sorwind. did u mean solar wind ?
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It has to do with the path of the earth and the sun through space.\n\nThe websites I've attached should help.
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If you've ever seen a bar magnet in a pile of iron filings, you'll see that the filings will orient themselves with the magnetic field, which concentrates at the poles.  Take a look at the images in the links.  The world is similar, in that it has a magnetic polarity that makes it work like a big magnet.\n\nIonized particles fly off the sun and out toward the planets (the so-called "solar wind").  An ionized particle has a charge, and a charged particle will turn when it moves through a magnetic field.  So when these charged particles encounter the earth's magnietic field, they will begin to spin in a sort of coiled-shaped path.  The spinning stops the ions from just smaking into the earth directly, so instead it will trace the length of the magnetic field, getting dragged towards one of the poles.  As the ions cluster at the poles, one of two things might happen: it might coil so tight that it switches directions, sort of "bouncing" and making the long trek to the other pole, or it might cascade down to earth.  Those which cascade to earth will strike gases in the upper atmosphere with a lot of energy, which can cause the gases to become energetically charged.  When they release the energy, it comes out as light (pretty much the same principle as in a fuorescent light).  Due to the differences in the speed of the ions, or the differences in the types of gases encountered, the light will have different colors.\n\nThis also happens at the south pole (the other end of the magnet) in what is called Aurora Australis (the southern lights).
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Mass arrives from space, and departs to space. But also energy arrives from space (mainly from the sun) and is converted into mass through biological processes.
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A lot of wind current is caused by temperature differentials between two or more areas.  The earth's rotation is also responsible for currents and jet streams.  I had a porfessor tell me that the same wind that is blowing now is the same wind that has been blowing for 4 billion years.
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the system of a star called sun is is called Solar system.....\nall the systems of stars with planets around them are not solar systems.\nSolar system is name of our sun planets system
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Have a look here,\nhttp://outreach.physics.utah.edu/labs/star_life/starlife_main.html
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The elements are formed in the Universe in three different places and times.\n\n1) In the three first minutes after the Big Bang protons and neutrons were formed. Roughly a quarter of those combined into helium, deuterons (heavy hydrogen) and a tiny bit of lithium.\n\n2) Stars like the sun are made of 75% hydrogen, 24% helium and 1% of other stuff. Their cores are hot enough to fuse hydrogen into helium. When the hydrogen in the core is exhausted the star goes through the red giant state in which it fuses helium into heavier elements like oxygen, sulphur all the way up the periodic system upto iron.\nThe smaller stars blow their outer layers into space.\n\n3) The bigger stars however, say 5-8 times the mass of the sun explode. These are supernovas. During this explosion a large part of the energy is liberated in the form of neutrinos.\nAn incredible amount of neutrinos, in fact. These particle are capable of transforming elements into others as they can change neutrons into protons. These reactions produce the elements heavier than iron.\n\nHow do we know this? \n\nAll three processes have been modelled. These models predict abondances for the elements in the universe. Those can be mesured are turn out quite close to the predictions.
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Our sun is about 93 million miles away. To put that into perspective if you hopped into a magic race car, like the ones that race in NASCAR, but you never needed gas and it drove itself and you could go 200 miles an hour non-stop for the whole trip, it would take a little over 50 years to get to the sun. Fortunately spacecraft can go much faster than race cars. The sun is very close to us compared to the other stars. They are so far away it takes light, which travels very fast(186 thousand miles per second), years (or hundreds of years) to reach us from them.
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It is an incorrect concept that space is full of nothing.  There are dust particles and gas molecules in space.  The solar wind from our sun is always blowing particles into space.  There is also a galactic wind that is blowing particles out into space as well.\n\nSpace is as close as we can get to natural vacuum, or nothingness but it still has a density of one atom per cubic meter.
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A star is a massive body of plasma in outer space that is currently producing or has produced energy through nuclear fusion. The most familiar and closest star to the Earth is the Sun. Unlike a planet, from which most light is reflected, a star emits light because of its intense heat. Scientifically, stars are defined as self-gravitating spheres of plasma in hydrostatic equilibrium, which generate their own energy through the process of nuclear fusion. Stellar astronomy is the study of stars.
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Plasma does not cast a shadow. Plasma is the extreme for of matter. Its the core of the sun but Plasma cannot cast a shadow.
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Stars revolve around the center of the galaxy.\nThe Sun revolves around the center of the milky way galaxy.
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The sun gives off high-energy charged particles (also called ions) that travel out into space at speeds of 300 to 1200 kilometres per second. A cloud of such particles is called a plasma. The stream of plasma coming from the sun is known as the solar wind. As the solar wind interacts with the edge of the earth's magnetic field, some of the particles are trapped by it and they follow the lines of magnetic force down into the ionosphere, the section of the earth's atmosphere that extends from about 60 to 600 kilometres above the earth's surface. When the particles collide with the gases in the ionosphere they start to glow, producing the spectacle that we know as the auroras, northern and southern. The array of colours consists of red, green, blue and violet.