Mariner Mission to VenusJet Propulsion Laboratory (U.S.)
Science
Mariner Mission to Venus
Jet Propulsion Laboratory (U.S.)
Project Mariner (U.S.)
It was believed that these moving plasma currents are also capable of
altering the size of a planet’s field of magnetic flux. When this
happens, the field on the sunlit face of the planet is compressed and
the dark side has an elongated expansion of the field. For example, the
outer boundary of the Earth’s magnetic field is pushed in by the solar
wind to about 40,000 miles from the Earth on the sunward side. On the
dark side, the field extends out much farther.
The solar wind was also known to have an apparent effect on the movement
of cosmic rays. As the Sun spots increase in the regular 11-year cycle,
the number of cosmic rays reaching the Earth from outside our solar
system will decrease.
Mariner II found that streams of plasma are constantly flowing out from
the Sun. This fluctuating, extremely tenuous solar wind seems to
dominate interplanetary space in our region of the solar system. The
wind moves at velocities varying from about 200 to 500 miles per second
(about 720,000 to 1,800,000 miles per hour), and measures up to perhaps
a million degrees Fahrenheit (within the subatomic structure).
With the solar plasma spectrometer working at ten different energy
levels, Mariner required 3.7 minutes to run through a complete energy
spectrum. During the 123 days, when readings were made, a total of
40,000 such spectra were recorded. Plasma was monitored on 104 of those
123 days, and on every one of the spectra, the plasma was always
present.
Mariner showed that the energies of the particles in the solar winds are
very low, on the order of a few hundred or few thousand electron volts,
as compared with the billions and trillions of electron volts measured
in cosmic radiation.
The extreme tenuousity or low density of the solar wind is difficult to
comprehend: about 10 to 20 protons (hydrogen nuclei) and electrons per
cubic inch. But despite the low energy and density, solar wind particles
in our region of the solar system are billions of times more numerous
than cosmic rays and, therefore, the total energy content of the winds
is much greater than that of the cosmic rays.
Mariner found that when the surface of the Sun was relatively inactive,
the velocity of the wind was a little less than 250 miles per second and
the temperature a few hundred thousand degrees. The plasma was always
present, but the density and the velocity varied. Flare activity on the
Sun seemed to eject clouds of plasma, greatly increasing the velocity
and density of the winds. Where the particles were protons, their
energies ranged from 750 to 2,500 electron volts.
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