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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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the radial component of the magnetic field is either<br />

toward or away from the sun. The region in<br />

which such an orientation is maintained is called<br />

a sector. There are either away or toward sectors<br />

depending on the direction of the radial component<br />

of the magnetic field. At the transition from<br />

away to toward or vice versa, the magnitude of<br />

the magnetic field is fairly constant. Normally<br />

two or four sectors are observed during a solar<br />

rotation. The sectors are dependent on the solar<br />

latitude <strong>and</strong> disappear at higher latitudes where<br />

the Interplanetary Magnetic Field (IMF) has the<br />

same sign as the appropriate solar pole.<br />

solar maximum The time at which the solar<br />

cycle reaches its highest level as defined by the<br />

12-month smoothed value of the sunspot number.<br />

During solar maximum there are more active<br />

regions <strong>and</strong> sunspots on the sun, as well as<br />

more solar flares leading to greater numbers of<br />

geomagnetic storms at the Earth. The most recent<br />

solar maximum occurred in July 1989. The<br />

next is expected to occur sometime in the year<br />

2000. See solar cycle.<br />

solar maximum mission (SMM) The SMM<br />

spacecraft was launched on February 14, 1980<br />

near the height of the solar cycle, to examine<br />

solar flares in more physically meaningful detail<br />

than ever before. SMM recorded its final data<br />

in November 1989.<br />

solar minimum The time at which the solar<br />

cycle reaches its lowest point as described by the<br />

12-month smoothed value of the sunspot number.<br />

During solar minimum, there may be no<br />

sunspots or solar flares. The most recent minimum<br />

occurred around October 1996. See solar<br />

cycle.<br />

solar nebula The cloud of gas <strong>and</strong> dust out of<br />

which our solar system formed. About 4.6×10 9<br />

years ago, a slowly rotating cloud of gas <strong>and</strong> dust<br />

began to collapse under its own gravitational influence.<br />

As the cloud collapsed, it began to form<br />

a flattened disk with a central bulge. The central<br />

bulge collapsed down to eventually form the<br />

sun. In the outer part of the disk, at least two<br />

other blobs of gas <strong>and</strong> dust collapsed down to<br />

form the planets Jupiter <strong>and</strong> Saturn. Elsewhere,<br />

small material condensed out of the cloud <strong>and</strong><br />

© 2001 by CRC Press LLC<br />

solar neutrinos<br />

began to accrete to form the other planets, most<br />

of the moons, <strong>and</strong> the small icy <strong>and</strong> rocky debris<br />

that became the comets <strong>and</strong> asteroids. This<br />

scenario helps to explain the counterclockwise<br />

orbital motion of all the planets, the counterclockwise<br />

orbital motion of most of the larger<br />

moons, <strong>and</strong> the counterclockwise rotation direction<br />

of most of the planets by proposing that the<br />

solar nebula was rotating in a counterclockwise<br />

direction.<br />

Alternately, the disk of gas <strong>and</strong> dust that surrounded<br />

the newly formed sun at the time of solar<br />

system formation. The planets were formed<br />

from the material in the nebula. If we take the<br />

current masses of all the planets, <strong>and</strong> add enough<br />

hydrogen <strong>and</strong> helium to make the composition<br />

identical to that of the sun, the resulting mass is<br />

the mass of a minimum mass solar nebula.<br />

solar neutrinos Low-energy electron neutrinos<br />

released in nuclear reactions in the sun<br />

<strong>and</strong> detectable from Earth. Fewer are seen than<br />

predicted by st<strong>and</strong>ard physics <strong>and</strong> astrophysics.<br />

The reactions of the proton-proton chain produce<br />

neutrinos of energy less than 1 MeV at<br />

the deuterium-production stage <strong>and</strong> more energetic<br />

ones in connection with the reactions involving<br />

beryllium <strong>and</strong> boron. The first experiment,<br />

using Cl 37 as a detector, was constructed<br />

by Raymond Davis in the Homestake Gold Mine<br />

in Lead, South Dakota beginning in 1968. By<br />

1971 it was clear that only about a third of the<br />

expected neutrinos were being captured, but the<br />

experiment was sensitive only to the Be <strong>and</strong> B<br />

products, thus explanations focused on mechanisms<br />

that might cool the center of the sun <strong>and</strong><br />

reduce production of these high energy particles<br />

without affecting the main reaction chain.<br />

A second experiment, at Kamioka, Japan, confirmed<br />

the deficiency of B 8 neutrinos starting<br />

in 1989, but also showed that the ones being<br />

seen were definitely coming from the direction<br />

of the sun. Two experiments of the 1990 (SAGE<br />

in the Caucasus Mountains <strong>and</strong> GALLEX under<br />

the Alps) look at the lower energy neutrinos<br />

from the main reaction chain. They are also deficient<br />

by a factor of about two. The full pattern<br />

is best accounted for if the solar model is the<br />

st<strong>and</strong>ard one, but electron neutrinos can change<br />

into mu or tau neutrinos en route to us. A possible<br />

mechanism, called MSW (for its inven-<br />

429

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