OTTER
发表于 2025-3-26 22:47:23
http://reply.papertrans.cn/67/6661/666083/666083_31.png
最有利
发表于 2025-3-27 01:07:18
http://reply.papertrans.cn/67/6661/666083/666083_32.png
头脑冷静
发表于 2025-3-27 06:43:30
http://reply.papertrans.cn/67/6661/666083/666083_33.png
抛物线
发表于 2025-3-27 09:40:44
http://reply.papertrans.cn/67/6661/666083/666083_34.png
安心地散步
发表于 2025-3-27 13:48:59
http://reply.papertrans.cn/67/6661/666083/666083_35.png
FLIC
发表于 2025-3-27 20:55:47
http://reply.papertrans.cn/67/6661/666083/666083_36.png
不如屎壳郎
发表于 2025-3-27 22:17:28
http://reply.papertrans.cn/67/6661/666083/666083_37.png
pantomime
发表于 2025-3-28 05:06:13
ral limit theorems for totally modified and conditionally modified sums, and their empirical versions. Our goal is to obtain invariance principles for a large class of functions ..(.) which includes those for which ..(.) ≤ ..(.)≤ ..(.). These functions .. might be called influence functions because
多嘴多舌
发表于 2025-3-28 09:02:28
Raudelio Machin Suareznd to illustrate the methods with a variety of new results. The presentation has been divided into two parts. Part I explores the approaches which have evolved from classical analytical techniques (condi tionin~, Fourier methods, symmetrization, triangular array theory). Part II is Msed on the quan
吹牛大王
发表于 2025-3-28 14:25:06
Plínio W. Prado Jretween a star’s rate of rotation and its magnetic field amplitude are also difficult, although observations of late-type stars suggest such a relationship. A transition between two modes of dynamo operation may occur as the star’s rotation slows down by magnetic braking.