Telescopic observations suggest that the solar magnetic field, which theoretically is " frozen " into the gas of the plasma in the photosphere, expands into roughly semicircular structures in the corona.
12.
In the context of the magnetic field of the Sun, the term "'magnetogram "'refers to a pictorial representation of the " spatial " variations in strength of the solar magnetic field.
13.
The first space shuttle launch for 1995 will be Feb . 2, when Discovery will perform a close-proximity rendezvous with the Russian Mir space station and will study the sun's solar magnetic fields.
14.
They write how the solar magnetic field grew over twice as strong as before over the 20th century, and they peg this as a primary driver of the approximately 0.6 �C warming over that time.
15.
This method has used the correlation between solar magnetic field strength at solar minimum to sun spot number at solar maximum to accurately predict the peak solar flux of each of the last three solar cycles.
16.
The polar auroral emissions are similar to those observed around Earth's poles : both appear when electrons are accelerated towards the planet by potential drops, during reconnection of solar magnetic field with that of the planet.
17.
A mission to send a spacecraft as close as 9 solar radii from the sun, NASA Solar probe, is planned for launch in 2015 and aims to provide in-situ measurements of the solar magnetic field, solar wind and corona.
18.
However, this process in the sun invariabily leads to a reversal of the solar magnetic field ( see : solar cycle ), and has never been observed such that the field would recover without large scale changes in field orientation.
19.
Since the solar magnetic field is continually wound up due to the faster rotation of mass at the sun's equator ( differential rotation ), sunspot activity will be more pronounced at solar maximum where the magnetic field is more twisted.
20.
When solar protons enter the Earth's magnetosphere where the magnetic fields are stronger than solar magnetic fields, they are guided by the Earth's magnetic field into the polar regions where the majority of the Earth's magnetic field lines enter and exit.
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