Plasmas in space

MAR 01, 1963

The following summary of present knowledge and speculation concerning properties of the interplanetary medium gives a brief account of some theoretical ideas advanced in the past twenty years and reviews some experimental observations which have been made from the earth. Particular attention is given to direct measurements of plasma properties carried out by means of the Explorer X satellite.

DOI: 10.1063/1.3050802

Herbert S. Bridge

About twenty years ago, the so‐called “infall” theory had been thoroughly worked out by Hoyle and by Alfvén. They reasoned that, since the sun moves through clouds of interstellar hydrogen gas, the neutral hydrogen must fall in toward the sun under the influence of the gravitational field. On its way toward the surface of the sun, the hydrogen encounters a strong flux of ultraviolet radiation and, because of the small rate of recombination, it becomes completely ionized. Thus the inner solar system is filled with a dilute, highly conducting plasma. At about the same time the infall theory was worked out, it became rather generally accepted that the corona of the sun has a temperature of 1 or 2 million degrees. In fact, Hoyle tried to account for the heating of the corona in terms of the energy released by the hydrogen falling into the sun.

This article is only available in PDF format

More about the Authors

Herbert S. Bridge. Massachusetts Institute of Technology.