Examples of using Solar wind in English and their translations into Turkish
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Ecclesiastic
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Ecclesiastic
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Programming
Jupiter and Saturn don't need the solar wind to make auroras.
You see this unseen and constant solar wind.
It's brewing up a solar wind big enough to blow this whole planet away.
By contrast, the fast solar wind has a typical velocity of 750 km/s,
Venus and Mars do not have magnetic fields, and as a result the solar wind is causing their atmospheres to gradually bleed away into space.
Extent of the interplanetary medium==The outer edge of the Solar System is the boundary between the flow of the solar wind and the interstellar medium.
The atoms that compose the solar wind- mostly helium,
The magnetosphere is embedded within the plasma of the solar wind, which carries the interplanetary magnetic field.
Even if the internal magnetic field did disappear, the solar wind can induce a magnetic field in the Earth's ionosphere sufficient to shield the surface from energetic particles.
The solar wind travels outward continuously through the heliosphere, forming the solar
Modern probes discovered a comet-like tail that stretches back to the Earth's orbit. The clouds on Venus are also being eroded by the solar wind.
And the new solar wind is being generated by this early star is pushing the material out
Another important source is the bombardment of the lunar surface by micrometeorites, the solar wind, and sunlight, in a process known as sputtering.
In other words, the Solar Wind consists of both negative electrons
Because the sun also ejects the solar wind, an energised stream of particles that head out into space.
When the solar wind hits the Earth's magnetic field, it stretches the
The slow solar wind is observed to have a velocity of 300-500 km/s,
Both the fast and slow solar wind can be interrupted by large,
To discover how the magnetic loops trigger the solar wind, a team of scientists at CalTech re-create the surface of a star right here on Earth.
That extends beyond the outer planets. This solar wind blows a vast magnetic bubble.