Earth's magnetic field (and the surface magnetic field) is approximately a magnetic dipole, with the magnetic field S pole near the Earth's geographic north pole (see Magnetic North Pole) and the other magnetic field N pole near the Earth's geographic south pole (see Magnetic South Pole). This makes the compass usable for navigation. The cause of the field can be explained by dynamo theory. A magnetic field extends infinitely, though it weakens with distance from its source. The Earth's magnetic field, also called the geomagnetic field, which effectively extends several tens of thousands of kilometres into space, forms the Earth's magnetosphere. A paleomagnetic study of Australian red dacite and pillow basalt has estimated the magnetic field to be at least 3.5 billion years old
The solar magnetic cycle is driven by the magnetic flux.
magnetic fields
It depends on their position and the way solar energy is absorbed.
Scientists may have teased out a tenuous connection between solar cycles and climate, such that earth slightly heats as the 11 year solar maximum approaches and passes, and cools again slightly afterwards.
Solar flares
Yes constantly, it is affected by the Solar wind and about every 100 thousand years the poles flip.
The solar activity cycle, which includes the solar maximum and solar minimum phases, lasts about 11 years. This cycle correlates with the flipping of the Sun's magnetic field every 11 years. This is known as the solar magnetic activity cycle.
T. E. Berger has written: 'On the dynamics of small-scale solar magnetic elements' -- subject(s): Morphology, Magnetic flux, Magnetic field configurations, Solar magnetic field
B. Coppi has written: 'Magnetic energy conversion processes and solar flares' -- subject(s): Plasma turbulence, Solar flares, Solar magnetic fields
The sun's magnetic fields are mainly produced by the movement of electrically charged particles within its interior. This process, known as the solar dynamo, generates complex magnetic fields that influence solar activity like sunspots and solar flares.
M. J Hagyard has written: 'Studies of solar magnetic fields during the solar maximum year' -- subject(s): Observations, Solar magnetic fields
Robert W. Noyes has written: 'Study of magnetic motions in the solar photosphere and their implications for heating the solar atmosphere' -- subject(s): Astrophysics, Chromosphere, Dynamic characteristics, Magnetic field configurations, Photosphere, Solar magnetic field