On the possible quasi-sound nature of the mechanism of global excitation of flares in the 11-year solar cycle.

Physics

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Solar Flares: Space Distribution, Solar Flares: Velocities

Scientific paper

A study is made of the possible spatial anisotropy of flare positions in longitude with respect to sunspot groups as a coordinate system moving with different angular rotation velocities. Vector (Rλ) latitude-time diagrams of average shifts of flares in solar cycles 17 and 18 are constructed. A regular picture of the "Rλ-shift" of the flares with respect to the center of the diagram is shown: the westward shift (+) at high latitudes changes to eastward (-) at low, near-equatorial latitudes. The character of regular shifts of flares confirms the hypothesis of global excitation of flares by disturbance with velocities of 1 - 3 km s-1. The vector diagrams of flares indicate that the external source of flare excitation plays an important role.

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