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The unusual anisotropic solar particle event of November 18, 1968

โœ Scribed by S. P. Duggal; I. Guidi; M. A. Pomerantz


Book ID
104642524
Publisher
Springer
Year
1971
Tongue
English
Weight
638 KB
Volume
19
Category
Article
ISSN
0038-0938

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โœฆ Synopsis


The ground level event of November 18, 1968, was unusual in that pronounced anisotropy persisted essentially until the cessation of the arrival at the earth of relativistic protons. Real and significant differences were observed in the intensity profiles at different neutron monitor stations. By a method of successive approximations, the geographical coordinates of the axis of symmetry were determined as: latitude .~ = -25 ~ 4-10 ~ and longitude r ----35 ~ 4-10 ~ The exponent in a power law spectral representation over the narrow range covered by the nucleonic intensity measurements was ~5.

The onset times of the GLE were related to the angular differences between the mean directions of viewing and the axis of symmetry. The event differed markedly from earlier isotropic events that were well described by diffusion theory, but was compatible with the predictions of a model envisaging diffusion only in the vicinity of the Sun (radius R of solar envelope ,m 34 solar radii). The diffusion coefficient D ~ 3 โ€ข 1021 cm~/s is consistent with that deduced for earlier isotropic events, but the values of other parameters are smaller than those derived for the only previously observed event to which the model of diffusion in an inhomogeneous medium was applicable (May 4, 1960).

It is concluded that the observed one hundred percent anisotropy was a direct consequence of the propagation mechanism rather than other postulated causes. Furthermore, the observed large pitchangle distribution was produced by scattering from small scale field irregularities.


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