How To Use Solar wind In A Sentence
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In our own solar system, the solar wind is responsible for shaping comets' tails and producing the Aurorae Borealis on Earth.
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It slows as it begins to collide with the interstellar medium, and the point where the solar wind slows down is the termination shock; the point where the interstellar medium and solar wind pressures balance is called the heliopause; the point where the interstellar medium, traveling in the opposite direction, slows down as it collides with the heliosphere is the bow shock.
Spacecraft Detects Mysterious "Ribbon" at Edge of Solar System | Universe Today
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The gas pressure eventually overcomes the force of solar gravity and the corona inevitably expands into space as the solar wind .
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Its last assignment was to find the heliopause, where the solar wind is offset by the galactic wind, but in April 1997 it was passed by a younger, faster Voyager spacecraft.
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The clouds of gas swirled and mixed as their electrons changed polarity, flickering colors that moved with the solar winds of a million suns.
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With the brilliant disk of the Sun blocked, the faint light of the corona reveals streamers of solar wind blowing out into space.
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The magnetosphere varies in size and shape, and its outer boundary - the magnetopause - gently undulates like a wave due to buffeting by the solar wind.
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Like the Solar Wind, the magnetosphere is full of plasma, consisting of ions and electrons.
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Either it was deposited by comets hitting the moon, or produced by solar winds hitting the lunar surface.
Times, Sunday Times
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Like the Solar Wind, the magnetosphere is full of plasma, consisting of ions and electrons.
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And that's critical to the analysis of the solar wind, the particles of which contain infinitesimal traces of the 83 naturally occurring elements.
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The solar wind loses its identity in the interstellar medium at a distance no less than that of the outer planets.
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The space shuttle has a rough landing, a superstorm fries the Roman Coliseum, and the solar winds dismantle the Golden Gate Bridge.
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When the charged particles of the solar wind hit the atmosphere, various gases present in the atmosphere heat up, split apart molecules, and ionize atoms.
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Solar wind is responsible for the direction of a comet's tail, which always points away from the Sun.
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Parker also showed how the solar wind would carry the solar magnetic field into interplanetary space.
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The Shade was also heavily magnetized to provide shielding from the potentially deadly solar wind, and cosmic rays.
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Like the Solar Wind, the magnetosphere is full of plasma, consisting of ions and electrons.
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This animation shows conceptually how solar wind might create electrically charged ambipolar environments in certain regions at the lunar poles.
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The tail effectively becomes a windsock for measuring the speed of the solar wind.
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The ion and electron monitors were turned on several months ago in preparation for their role during solar wind collection.
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We used this same technique when the instrument measuring the solar wind speed was still working.
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They are weaker than cosmic and galactic rays, and tend to get buffeted around like clouds of manic dandelion spores on the solar wind.
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Both spacecraft are now in a region known as the "heliosheath", the outermost layer of the Solar System, where the solar wind, which can travel 16 miles per second, is being slowed down by the rising pressure of interstellar gas.
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To solve these interrelated problems, her mother had the original windows retrofitted with state-of-the-art solar window film.
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Our relatively puny magnetic field holds the Solar Wind at bay, at the magnetopause, a distance of 60,000 km from Earth.
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Voyager 1 has left the termination shock to enter the heliosphere, a region still influenced by the solar wind.
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The capsule held billions of charged atoms - a total haul no bigger than a few grains of salt - that were harvested from solar wind on five collecting disks during the 884-day, $260-million mission.
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This exhaust is a superheated plasma (a charged gas) commonly referred to as the solar wind.
Canada Day
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The solar wind protons must sputter away the surface atoms of the dust
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One from Cassini, also of the interaction between the solar wind and Jupiter's magnetosphere, is here.
Boing Boing: October 20, 2002 - October 26, 2002 Archives
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It is this solar wind - seen only in comet tails - that carries storms from the Sun to Earth.
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One from Voyager's passage through the bow shock of the solar wind against Jupiter's magnetosphere is here.
Boing Boing: October 20, 2002 - October 26, 2002 Archives
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Some theorists even believe that solar wind particles hitting the atmosphere may trigger cloud formation.
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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.
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The solar wind slows as it crashes into the thin gas that fills the space between stars.
Times, Sunday Times
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The corona is composed of charged particles that become what we call the solar wind as they radiate outward from the Sun at 450 kilometers per second and are responsible for the aurora borealis.
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The samples of solar wind particles, collected on ultra-pure wafers of gold, sapphire, silicon and diamond were designed to be returned for analysis by Earth-bound scientists.
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Although the solar wind produces beautiful auroras, it can also cause a variety of undesirable consequences.
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Chris Carr of Imperial College London is using a magnetometer on the craft to study interactions with the solar wind as Venus Express flies through the boundary layer above the planet.
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Any other ship - any other dead ship - would have joined the rest of the flotsam and debris that formed the Pendulum Nebula, and been moved around by the whims of solar winds.
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The magnetosphere is a sheath that at once protects and interacts with the Sun's solar wind.
New Field in Planetology Opened by Aurora Lights Finding
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It has long been known to the astronomical community that the fast solar wind comes from coronal holes.
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The solar wind loses its identity in the interstellar medium at a distance no less than that of the outer planets.
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This solar wind inflates a giant bubble in interstellar space called the heliosphere -- the region of space dominated by the Sun's influence in which the
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The fast solar wind from the polar regions flowed uniformly to fill a large fraction of the heliosphere, and variability was confined to a narrow region around the solar equator.
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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.
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The fact that a man-made object is now approaching the heliopause, where the solar winds cease to blow, is a remarkable achievement.
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The Universe has its own heavenly sounds, such as pulsars, planetary magnetospheres and solar winds.
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Fig . 3 The time evolution curve of solar wind radial speed incited by disturbance propagation.
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The tenuous material surrounding a comet is pushed away from the sun by radiation pressure and solar wind.
A ‘bizzare star’, an incomplete explanation « Skulls in the Stars
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Some theorists even believe that solar wind particles hitting the atmosphere may trigger cloud formation.
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Many photogenic auroras have been triggered from a solar wind stream that recently passed the Earth.
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The Universe has its own heavenly sounds, such as pulsars, planetary magnetospheres and solar winds.
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Or you could use those same satellites to weave and unravel those “magnetic ropes” to manipulate the flow of solar wind particles, as one would strum the strings of a cello to create certain photonic vibrations.
Aurora Bibliothèque
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Solar wind to shield Earth during pole flip New Scientist - May 2004.
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Since then, the solar wind has gradually eroded the Martian atmosphere so that today it is less than 1% as thick as that of the Earth.
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The lack of atmosphere also means there's no protection from harmful radiation in the solar wind.
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Some theorists even believe that solar wind particles hitting the atmosphere may trigger cloud formation.
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Bolstering that view, simple models of the heliosphere require that the magnetic field intensifies in regions where the solar wind slows.
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Rosetta's instruments will analyse the gases and dust grains in the coma that forms when the comet becomes active, as well as the interaction with the solar wind.
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“They act as magnetic channels or open windows that allow solar wind plasma from the sun, very fast and very hot, to come right down those field lines and impacts the surface,” said Jim Slavin of NASA Goddard Spaceflight Center.
Monday
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Specifically, that means a time when liquid water appears to have run freely around the planet, and when Mars had a magnetic field surrounding it that enabled a much thicker atmosphere to act as a shield against the ravages of the solar wind and the ultraviolet radiation that now desiccate the surface.
First Contact
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The lunar surface also contains the light isotope helium-3, which is implanted in the surface by the solar wind.
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Both solar wind ions and neutrals will impact with enough energy to ionize and/or cause many reactions – 100s of eV, AFAIU, as opposed to a few eV.
LCROSS Confirms "Buckets" of Water on the Moon | Universe Today
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The simple reason for that assertion is plain scientific logic: we would expect that a positively charged Sun would repel positively charged protons, and attract negatively charged electrons; however, what we actually observe is that both electrons & protons are being 'repelled' by the Sun, and that immediately negates any consideration of the Sun having a net electric charge that can be detected anywhere in the solar wind flow.
Do "Skeleton" Filaments Give Structure to the Universe? | Universe Today
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The solar wind is a stream of electrically charged particles (electrons and ions) blown constantly from the sun.
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The Moon's regolith was created by the ceaseless bombardment of micrometeorites, cosmic rays and particles of solar wind breaking down rocks for billions of years.
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If implanted by the solar wind after eruption, hydrogen measured by the OH- anions sputtered from the glass should be higher near the surface of each bead.
Water on the Moon: What Does it Mean? | Universe Today
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The magnetosphere varies in size and shape, and its outer boundary - the magnetopause - gently undulates like a wave due to buffeting by the solar wind.
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This solar wind inflates a giant bubble in interstellar space called the heliosphere -- the region of space dominated by the Sun's influence in which the Earth and other planets reside.
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Solar wind to shield Earth during pole flip New Scientist - May 2004.
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We already know that the poles of the Moon contain elevated hydrogen content (the rare element on the Moon); this hydrogen is there regardless of its physical form, either as water ice or as solar wind protons.
Back to the Moon We Go - NASA Watch
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After that, all thatremains will be three piles of anhydrous powder left to be borne upon the solar winds.
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The two Voyagers are located in the outermost layer of the heliosphere, or "heliosheath," where the solar wind is slowed by the pressure of interstellar gas.
Signs of the Times
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The solar wind loses its identity in the interstellar medium at a distance no less than that of the outer planets.
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Between the bow shock and the magnetopause the solar wind is greatly decelerated.
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The atoms become ionized by the sun's ultraviolet radiation and are then accelerated to enormous energies by the solar wind.
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Even that data is suspect at the claimed resolutions due to the variabilityies of the satellite orbits due to variations in atmospheric drag, solar wind, etc. affecting orbits.
Jack Schmitt on Global Warming - NASA Watch
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If the magnetic field in the solar wind is directed southward, it can interconnect with the Earth's northward-oriented magnetic field.
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It appears that these seed populations of energetic protons near the sun could provide the answer, because it's easier to accelerate a proton that already has an energy of 1 MeV than a proton that is at 1 keV the solar wind.
MESSENGER Solves Solar Flare Mystery | Universe Today
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Why the average Caprican would want to know the solar wind speed and solar wind density (468.3 km/sec and 4.1 protons/cm3, respectively) on a daily basis is anyone's guess, but the info is there.
‘Caprica’ News Site For ‘The Caprican’ Launches » MTV Movies Blog
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The tail is pushed outwards from the Sun by the solar wind and radiation pressure, and so the popular conception that a comet's tail streams away behind it is wrong.
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Together, the results create the first map of the heliosphere and its thick outer layer known as the heliosheath, where solar wind streaming out from the sun gets heated and slowed as it interacts with the interstellar medium.
Space News From SpaceDaily.Com
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The average strength of the magnetic field carried by the solar wind depends on solar location as well.
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The magnetotail is the part of the magnetosphere pushed in the direction of the solar wind - shaped like a giant windsock and stretching at least two million kilometres into space on the night side of the Earth.
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In the solar case, plasma motion towards us, which means away from the solar surface, is detected as blue shift in the ultraviolet spectrum, and thus can be used to identify the beginning of the solar wind outflow.
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On Earth, the atmosphere and the magnetosphere deflect the charged particles that stream in from the Sun at a million miles an hour: the solar wind.
