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   <subfield code="a">North-South anisotropy during the quasi-stationary modulation of galactic cosmic rays</subfield>
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   <subfield code="c">[M. Storini, N. Iucci, S. Pase]</subfield>
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   <subfield code="a">Summary: High-speed solar-wind streams coming from coronal holes produce, in the interplanetary space, a quasi-stationary modulation of galactic cosmic rays. The Rome cosmic-ray group has analysed this modulation taking into account not only the charged-particle isotropic intensity but also the North-South anisotropy (A NS), derived from ground-based measurements. The obtained results for the period October 1964-December 1987 are summarized. Data from the Bartels solar rotation no. 2034 (May 23-June 18, 1982) are used to illustrate theA NS phenomenology.</subfield>
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