スライドショーにすると、アニメーションが動きます。
アニメーション上で右クリックすると、アニメーションが一時停止します。
� ( � ) = 1
� ∑
�=1
�
cos ( ��
0� )
ω0=1.0, N=700 でアニメーション作成
桑名杏奈先生 作成
� ( � ) = 1
� ∑
�=1
�
sin ( ��
0� )
ω0=1.0, N=700 でアニメーション作成
桑名杏奈先生 作成
∑ = cos 1
2
0
0
全文
(2)
関連したドキュメント
Theorem 3 implies strong asymptotic stability results: the energy of strong solutions decays to zero, with an explicit decay rate
There is a bijection between left cosets of S n in the affine group and certain types of partitions (see Bjorner and Brenti (1996) and Eriksson and Eriksson (1998)).. In B-B,
Actually a similar property shall be first de- rived for a general class of first order systems including the transport equation and Schr¨odinger equations.. Then we shall consider
(The Elliott-Halberstam conjecture does allow one to take B = 2 in (1.39), and therefore leads to small improve- ments in Huxley’s results, which for r ≥ 2 are weaker than the result
“Breuil-M´ezard conjecture and modularity lifting for potentially semistable deformations after
lines. Notice that Theorem 4 can be reformulated so as to give the mean harmonic stability of the configuration rather than that of the separate foliations. To this end it is
S., Oxford Advanced Learner's Dictionary of Current English, Oxford University Press, Oxford
At the end of the section, we will be in the position to present the main result of this work: a representation of the inverse of T under certain conditions on the H¨older
