A 27‐day periodicity in outer zone trapped electron intensities

Data from the polar orbiting satellite 1963 38C show the existence of a 27-day periodicity in the intensities of trapped, ≥280-kev and ≥1.2-Mev electrons for L ≥3.5. This effect is seen for the four sequential solar rotations commencing October 6, 1963. The trapped energetic electron intensities are observed to undergo two large increases every 27 days and are shown to be intimately linked with the passage of the recently observed interplanetary magnetic field sector boundaries. It is also shown that these electron intensity increases are triggered by variations in the parameter β, the ratio of the directed solar wind kinetic energy density to the interplanetary magnetic field energy density. Equivalently, large variations in the Alfven Mach number MA are shown to be responsible for these trapped electron variations.

[1]  福島 直 B. M. McCormac編: Radiation Trapped in the Earth's Magnetic Field-Proceedings of the Advanced Study Institute held at the Chr. Michelsen Institute, Bergen, Norway, Aug. 16-Sept. 3, 1965-D.Reidel Pub. Co., Dordrecht-Holland, 1966, 901頁, 17×25cm, 15,600円. , 1967 .

[2]  J. Wilcox,et al.  Quasi‐stationary corotating structure in the interplanetary medium , 1965 .

[3]  N. Ness The Earth's magnetic tail , 1965 .

[4]  J. Wilcox,et al.  Sector Structure of the Quiet Interplanetary Magnetic Field , 1965, Science.

[5]  D. Williams,et al.  Daytime trapped electron intensities at high latitudes at 1100 kilometers , 1965 .

[6]  C. S. Scearce,et al.  Initial results of the imp 1 magnetic field experiment , 1964 .

[7]  H. K. Hills,et al.  A STUDY OF CHARGED PARTICLES IN THE EARTH'S OUTER RADIATION ZONE WITH EXPLORER 14 , 1964 .

[8]  G. K. Walters Effect of oblique interplanetary magnetic field on shape and behavior of the magnetosphere , 1964 .

[9]  J. Freeman The morphology of the electron distribution in the outer radiation zone and near the magnetospheric boundary as observed by Explorer 12 , 1964 .

[10]  G. K. Walters,et al.  Hydromagnetic coupling between solar wind and magnetosphere , 1964 .

[11]  R. Hoffman,et al.  Observations of the Van Allen radiation regions during August and September 1959: 6. Properties of the outer region , 1962 .

[12]  W. Axford The interaction between the solar wind and the Earth's magnetosphere , 1962 .

[13]  G. Pizzella,et al.  The Morphology and Temporal Variations of the Van Allen Radiation Belt, October 1959 to December 1960 , 1962 .

[14]  P. Kellogg Flow of plasma around the Earth , 1962 .

[15]  C. O. Hines,et al.  A UNIFYING THEORY OF HIGH-LATITUDE GEOPHYSICAL PHENOMENA AND GEOMAGNETIC STORMS , 1961 .

[16]  J. Dungey Interplanetary Magnetic Field and the Auroral Zones , 1961 .

[17]  E. Parker,et al.  Geomagnetic storm sudden‐commencement rise times , 1960 .

[18]  E. Parker Dynamics of the Interplanetary Gas and Magnetic Fields , 1958 .

[19]  L. J. Cahill,et al.  Transition region magnetic field and polar magnetic disturbances. , 1966 .

[20]  Donald J. Williams Outer Zone Electrons , 1966 .

[21]  J. Virginia Lincoln,et al.  Geomagnetic and solar data , 1966 .

[22]  W. Axford Viscous interaction between the solar wind and the earth's magnetosphere , 1964 .