This provides strong support for the hypothesis that solar irradiance variations are caused by changes in the amount and distribution of
magnetic flux at the solar surface.
This is in agreement with the recent results of [CITE], but it is in contrast to the earlier analysis of [CITE], and suggests that the source of the irradiance variations is the same for cycles 22 and 23, namely the evolution of
the magnetic flux at the solar surface.
The planets may have a spin - orbit coupling effect on the Sun which affects its rotation rate, which would then affect the solar dynamo and sunspot production, and therefore the build up of
magnetic flux at the poles, and the length of a solar cycle: if the solar cycle is weaker with less sunspots, it'll take longer for the build up of opposing flux to reach the point when it flips the poles.
Not exact matches
«Faraday said changing
magnetic flux generates an electromotive force — a voltage, if you like,» says Blandford, who is now
at Stanford University.
Examining a small, high - quality crystal grown
at Tulane University, the team was able to determine the
magnetic structure of Sr1 - yMn1 - zSb2, using neutrons
at the Four - Circle Diffractometer instrument
at the High
Flux Isotope Reactor.
«
Magnetic flux lines interfere with the wires» ability to transport electricity, lowering its performance,» says Venkat Selvamanickam
at the University of Houston, Texas, where the US government is funding work via its Advanced Research Projects Agency — Energy.
Fine details of a
magnetic flux rope captured by the New Solar Telescope
at Big Bear Solar Observatory for Solar Active Region 11817 on 2013 August 11.
Scientists
at NJIT's Big Bear Solar Observatory (BBSO) have captured the first high - resolution images of the flaring
magnetic structures known as solar
flux ropes
at their point of origin in the Sun's chromosphere.
«They look
at geothermal heat
flux through seismic signals or
magnetic data in Greenland, but not crustal thickness or rock type or distance from a hot spot.
Another scientist examined the inner workings of the sun through the oscillation of sound waves propagating through the solar interior; yet another looked
at magnetic maps to chart the shifting
flux across the sun.
The high frequency AC current of the primary winding generates a
magnetic field, and then the linkage
magnetic flux induces the voltage
at the secondary winding.
the distance of the body from the Sun, determining the properties of solar wind and solar energetic particles (SEPs), the solar photon
flux and the properties of the Interplanetary
Magnetic Field (IMF)
at that location;
Starting in the 1960's
at the Mt. Wilson Observatory O.C. Wilson (sic) began a long - term study of
magnetic cycles in cool stars using as his observational indicator the variable emission
flux of the H and K resonance lines of ionized calcium whose appearance in emission is characteristic of stellar chromospheres.
The solar wind is a
flux of charged particles that flows
at supersonic velocity from the Sun's outer atmosphere (the corona) and carries with it the solar
magnetic field.
The solar
magnetic cycle that flips polarity
at the poles approximately every 11 years is dependent on the reversing
flux from spent sunspots that migrate to the poles.
Volker Doormann says: July 27, 2011
at 2:38 pm http://adsabs.harvard.edu/abs/2010JGRA..11501104S We have reconstructed the interplanetary
magnetic field (IMF), its radial component, and the open solar
magnetic flux using the solar modulation potential derived from cosmogenic 10Be radionuclide data for a period covering the past 9300 years.
As the process continues and
magnetic flux strength of the sunspot group declines, the lifetime of a sunspot group (of the few sunspot groups that do form) has decreased to where we are now
at the point that a sunspot group's lifetime is for a number of cases only a few days.
how does that differ from TSI and variables such as
magnetic flux variation
at poles + + + plus other variables.