一、
2.
(a)对Sena、Sensin和Omaha图像时行编码。
文件名 | 压缩前大小 | 压缩后大小 | 压缩比 |
omaha | 64kb | 58kb | 90 % |
sinan | 64kb | 61kb | 95% |
sena | 64kb | 57kb | 89% |
4.
(a) H=-0.15*log20.15-0.04*log20.04-0.26*log20.26-0.05*log20.05-0.50*log20.50
=0.411+0.186+0.505+0.216+0.50
=1.82(bits)
(b) a1: 001
a2: 0000
a3: 01
a4: 0001
a5: 1
(c) 平均长度 L=3*0.15+4*0.04+2*0.26+4*0.05+1*0.5=1.83 bits
冗余度=L-H=0.012
5.
(a) a1: 001
a2: 01
a3: 000
a4: 1
L=3*0.1+2*0.3+3*0.25+1*0.35=2
(b) a1: 11
a2: 01
a3: 10
a4: 00
L=2*0.1+2*0.3+2*0.25+2*0.35=2
a方差为:s12=(0.1+0.25)*(3-2)2+0.3*(2-2)2+0.35*(1-2)2=0.7
b方差为:s22=(0.1+0.25+0.3+0.35)*(2-2)2=0
所以b过程最优
二、
6.
(a)图像的一阶熵
EARTH.IMG:4.770801
OMAHA.IMG:6.942426
SENA.IMG:6.834299
SENSIN.IMG:7.317944
BERK.RAW:7.151537
GABE.RAW:7.116338
(b)二阶熵比一阶熵小
(c)差熵比一阶熵小,但比二阶熵大