この文章の和訳を教えてください。
At first sight, from these figures, a symmetric pattern with respect to b_i~=0 holds approximately and a large scattering occurs in the region 1.5≦|b_i~|≦6. This is because a particle of which |b_i~| lies between 1.5 and 6 enters the Hill sphere and, hence, is scattered heavily.
When |b_i~| is less than about 1.0, the feature of the scattering takes a new aspect. The gyrocenter of a particle comes slowly close to the planet whereas the particle rotates rapidly around the gyrocenter. When the distance between the planet and the gyrocenter is several times as short as the Hill radius, the gyrocenter of the particle gradually turns back to the opposite side of the y-axis, as if it were reflected by a mirror. The feature of the scattering is the same as that for the case e_i~=0. For the final impact parameter, b_f~, and the eccentricity, e_f~, we have again the relations
b_f~=-b_i~ and e_f~=e_i~. (3・10)
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お礼
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