我一直试图\multirow合并 x、y1 和 y2 的单元格，但我无法成功。我尝试使用在线表格生成器来制作表格在线表格生成器并尝试根据我的需求进行修改，但这里出现了问题。你能帮我修复这个错误吗？
\documentclass[14pt, a4paper, twoside]{report} % 'twoside' when printing
%\setcounter{secnumdepth}{3}
\usepackage[utf8]{inputenc} % UTF-8 input
\usepackage[english]{babel} % Set language to english
\usepackage{amsmath}
\usepackage{amsfonts}
\usepackage{amsthm}
\usepackage{geometry}
\usepackage{array}
\newcolumntype{?}{!{\vrule width 1pt}} %Thick vertical line
\newcolumntype{H}{>{\setbox0=\hbox\bgroup}c<{\egroup}@{}}
\newcolumntype{Z}{>{\setbox0=\hbox\bgroup}c<{\egroup}@{\hspace*{-\tabcolsep}}}
\usepackage{booktabs}
\usepackage{multirow}
\usepackage{subcaption}
\usepackage{tabularx}
\usepackage{floatrow, makecell}%
\makeatother
% Center the table horizontally
\newcolumntype{P}[1]{>{\centering\arraybackslash}p{#1}}
% Center the table vertically
\newcolumntype{M}[1]{>{\centering\arraybackslash}m{#1}}
% Center the table horizontally and vertically
\newcolumntype{C}[1]{>{\centering\arraybackslash}m{#1}}
\usepackage{float}
\begin{document}
\begin{table}[H]\footnotesize\setlength{\tabcolsep}{5pt}\textbf{}
\centering
\caption{Total Effect}
\bgroup
\def\arraystretch{1.5}% 1 is the default, change whatever you need
\begin{tabular}{ ? p{0.4em} | p{2em}? p{3.2cm} | p{4.1cm}| p{4.2cm} | p{3.7cm}| }
\toprule
& Si \newline index&Max & Mean &Median &Eqm \\
\Xhline{4\arrayrulewidth}
\multirow{3}{*}{$x$} &$s_{T}$&
$\left[x_{0}\right],\,\newline
\left[\left(\text{ all others}\right)\right]$ &
$\left[b\,\,\delta_{2},\,\delta_{1},\,\omega_{2},\,\omega_{1},\,\psi,\,x_{0}\right],\,\newline \left[\phi,\,\left(a,\,{y_{1}}_{0},\,{y_{2}}_{0}\right)\right]$ &
$\left[b,\,\delta_{2},\,\delta_{1},\,\omega_{2},\,\omega_{1},\,\psi,\,\phi\right],\,\newline \left[{y_{1}}_{0},\,a,\,x_{0},\,{y_{2}}_{0}\right]$ &
$\left[b,\,\delta_{2},\,\delta_{1},\,\omega_{1},\,\omega_{2},\,\psi,\,\phi\right],\,\newline \left[x_{0},\,\left({a,\,y_{1}}_{0},\,{y_{2}}_{0}\right)\right]$ \\
\hline
&$\mu^{\star}$ &
$\left[x_{0}\right],\,\newline
\left[\left(\text{ all others}\right)\right] $ &
$\left[b,\,x_{0},\,\delta_{1},\,\omega_{1},\,\delta_{2},\,\omega_{2}\right],\,\newline
\left[\psi,\,\phi,\,{y_{2}}_{0},\,{y_{1}}_{0},\,a\right]$ &
$\left[b,\,x_{0},\,\omega_{1},\,\delta_{1},\,\delta_{2}\omega_{2}\right],\,\newline
\left[\psi,\,\phi,\,a,\,{y_{2}}_{0},\,{y_{1}}_{0}\right]$ &
$\left[b,\,x_{0},\,\delta_{1},\,\omega_{1},\,\delta_{2}\omega_{2}\right],\,\newline
\left[\psi,\,\phi,\,a,\,{y_{2}}_{0},\,{y_{1}}_{0}\right]$ \\
\hline
&$\delta$ &
$\left[x_{0}\right],\,\newline
\left[\left(\text{ all others}\right)\right]$&
$\left[b,\,\delta_{2},\,x_{0},\,\omega_{2},\,\delta_{1},\,\omega_{1}\right],\,\newline\left[\psi,\,a,\,\left({\phi,\,y_{2}}_{0},\,{y_{1}}_{0}\right)\right]$&
$\left[b,\,\delta_{2},\,\omega_{2},\,\delta_{1},\,\omega_{1},\,\psi\right],\,\newline\left[a,\,{y_{2}}_{0},\,x_{0},\,\phi,\,{y_{1}}_{0}\right]$&
$\left[b,\,\delta_{2},\,\omega_{2},\,\delta_{1},\,\omega_{1},\,\psi\right],\,\newline\left[a,\,x_{0},\,{y_{2}}_{0},\,\phi,\,{y_{1}}_{0}\right]$ \\
\Xhline{4\arrayrulewidth}
\multirow{3}{*}{$y_{1}$} &$s_{T}$&
$\left[{y_{1}}_{0}\right],\,\newline\left[\left(\text{ all others}\right)\right]$&
$\left[b,\,\delta_{2},\,\delta_{1},\,\psi,\,\omega_{1},\,\omega_{2}\right],\,\newline\left[\phi,\,{y_{1}}_{0},\,x_{0},\,{y_{2}}_{0},\,a\right]$&
$\left[b,\,\delta_{2},\,\delta_{1},\,\psi,\,\omega_{1},\,\omega_{2},\,\phi\right],\,\newline\left[x_{0},\,{y_{2}}_{0},\,\left(a,\,{y_{1}}_{0}\right)\right]$&
$\left[\omega_{1},\,b,\,\delta_{2},\,\delta_{1},\phi,\,\psi,\,\omega_{2}\right],\,\newline\left[x_{0},\,{y_{2}}_{0},\,a,\,{y_{1}}_{0}\right]$ \\
\hline
&$\mu^{\star}$&
$\left[{y_{1}}_{0}\right],\,\newline\left[\left(\text{ all others}\right)\right] $ &
$\left[b,\,x_{0},\,\phi,\,\omega_{1},\,\delta_{1},\,{y_{1}}_{0}\right],\,\newline
\left[\delta_{2},\,\psi,\,\omega_{2},\,{y_{2}}_{0},\,a\right]$ &
$\left[b,\,x_{0},\,\delta_{2},\,\omega_{1},\,\omega_{2},\,\phi,\,\psi,\,\delta_{1}\right],\,\newline\left[{y_{2}}_{0},\,{y_{1}}_{0},\,a\right]$ &
$\left[b,\,\delta_{2},\,\omega_{1},\,x_{0},\,\delta_{1},\,\omega_{2},\,\psi,\,\phi\right],\,\newline\left[a,\,{y_{1}}_{0},\,{y_{2}}_{0}\right]$ \\
\hline
&$\delta$ &
$\left[{y_{2}}_{0}\right],\,\newline\left[\left(\text{ all others}\right)\right]$&
$\left[{y_{1}}_{0},\,b,\,\psi,\,\delta_{2},\,\omega_{2},\,\phi\right],\,\newline\left[x_{0},\,{y_{2}}_{0},\,a,\,\omega_{1},\,\delta_{1}\right]$ &
$\left[\omega_{2},\,b,\,\delta_{1},\,\delta_{2},\,\psi,\,\phi,\,\right],\,\newline\left[\left(a,\,\omega_{1},\,x_{0},\,{y_{1}}_{0},\,{y_{2}}_{0}\right)\right]$ &
$\left[\left(a,\,\phi,\, \omega_{1},\,x_{0},\,{y_{1}}_{0},\,{y_{2}}_{0},\ \omega_{2}\right)\right],\,\newline\left[b,\,\delta_{2},\,\psi,\,\delta_{1}\right]$ \\
\Xhline{4\arrayrulewidth}
\multirow{3}{*}{$y_{2}$} &$s_{T}$ &
$\left[\omega_{2},\,b,{y_{2}}_{0},\,x_{0},\,\omega_{1},\,\phi,\,\psi\right],\,\newline
\left[\delta_{2},\,{y_{1}}_{0},\,\left(a,\,\delta_{1}\right)\right]$ & $\left[b,\,\delta_{2},\,\delta_{1},\,\phi,\,\omega_{2},\,\psi,\,\omega_{1}\right],\,\newline
\left[x_{0},\,{y_{2}}_{0},\,\left(a,\,{y_{1}}_{0}\right)\right]$ &
$\left[b,\,\delta_{2},\,\delta_{1},\,\omega_{2},\,\phi,\,\psi,\,\omega_{1}\right],\,\newline
\left[x_{0},\,{y_{1}}_{0},\,{y_{2}}_{0},\,a\right]$ &
$\left[\phi,\, \delta_{2},\,\psi,\,b,\,\omega_{1},\,\delta_{1},\,\omega_{2}\right],\,\newline \left[x_{0},\,\left(a,\,{y_{1}}_{0},\,{y_{2}}_{0}\right)\right]$ \\
\hline
&$\mu^{\star}$ &
$\left[\omega_{2},\,b,\,\psi,\,\omega_{1},\,\phi,\,x_{0} \right],\,\newline
\left[\delta_{2},\,{y_{2}}_{0},\,{y_{1}}_{0},\,\delta_{1},\,a\right]$ &
$\left[b,\,\omega_{2},\,\delta_{2},\,\phi,\,x_{0},\,\omega_{1},\,\psi\right],\,\newline
\left[\delta_{1},\,{y_{2}}_{0},\,{y_{1}}_{0},\,a\right]$ &
$\left[b,\,\delta_{2},\,\omega_{2},\,x_{0},\,\phi,\,\psi,\,\omega_{1},\,\delta_{1}\right],\,\newline
\left[{y_{2}}_{0},\,a,\,{y_{1}}_{0}\ \right]$ &
$\left[\delta_{2},\,\omega_{2},\,\delta_{1},\,b,a,\,x_{0},\,\omega_{1}\right],\,\newline
\left[{{y_{1}}_{0},\,\psi,\,\phi,\,y_{2}}_{0}\right]$ \\
\hline
&$\delta$&
$\left[{y_{2}}_{0},\,b,\,\omega_{2},\,\omega_{1},\,\phi,\,\psi\right],\,\newline\left[\delta_{2},\,\delta_{1},\,x_{0},\,{y_{1}}_{0},\,a\right]$ &
$\left[{y_{2}}_{0},\,b,\,\delta_{1},\,\omega_{1},\,\psi,\,{y_{1}}_{0},\,a,\,\omega_{1},\,\phi\right],\,\newline\left[\delta_{2},\,x_{0},\,a\right]$ &
$\left[b,\,\delta_{1},\,\omega_{1},\,\psi,\,{y_{1}}_{0},\,a,\,{y_{2}}_{0},\,\phi,\, x_{0}\right],\,\newline\left[\delta_{2}\right]$ &
$\left[b,\,\delta_{2},\,\omega_{2},\,\omega_{1},\,\psi,\,\phi\right],\,\newline\left[\delta_{1},\,{y_{1}}_{0},\, x_{0},\,{y_{2}}_{0},\,a\right]$ \\
\bottomrule
\end{tabular}
\egroup
输出如图所示，这不是我想要的
答案1
按照我之前的评论，下面是我重写表格代码的方法。除了删除所有\left大小\right指令和所有\,细间距指令外，我还会删除所有垂直线，并使用更少但间距适当的水平线。最后，我会使用环境tabular*而不是tabualar环境，将\tabcolsep长度参数设置为0pt，然后让 LaTeX 找出最佳的列间空白量。
\documentclass[10pt, a4paper, twoside]{report} % '14pt' is not a valid option
\usepackage[utf8]{inputenc}
\usepackage[english]{babel}
\usepackage{amsmath,amssymb,amsthm}
\usepackage[margin=2.5cm]{geometry} % select margin widths
\usepackage{array,booktabs}
\usepackage{floatrow} % place caption below table by default
\begin{document}
\begin{table}
\footnotesize
\setlength{\tabcolsep}{0pt} % make LaTeX out amount of intercol. whitespace
\caption{Total Effect}
\begin{tabular*}{\textwidth}{@{\extracolsep{\fill}}
c p{2.2em} p{2.9cm} p{3.7cm} p{3.7cm} p{3.5cm} }
\toprule
& Si \mbox{index} & Max & Mean & Median & Eqm \\
\midrule
$x$
& $s_{T}$
& $[x_0],[(\text{all others})]$
& $[b,\delta_2,\delta_1,\omega_2,\omega_1,\psi,x_0],
\newline
[\phi,(a,y_{1_0},y_{2_0})]$
& $[b,\delta_2,\delta_1,\omega_2,\omega_1,\psi,\phi],
\newline
[y_{1_0},a,x_0,y_{2_0}]$
& $[b,\delta_2,\delta_1,\omega_1,\omega_2,\psi,\phi],
\newline
[x_0,({a,y_1}_0,y_{2_0})]$ \\
\addlinespace
& $\mu^{\star}$
& $[x_0],[(\text{all others})] $
& $[b,x_0,\delta_1,\omega_1,\delta_2,\omega_2],
\newline
[\psi,\phi,y_{2_0},y_{1_0},a]$
& $[b,x_0,\omega_1,\delta_1,\delta_2\omega_2],
\newline
[\psi,\phi,a,y_{2_0},y_{1_0}]$
& $[b,x_0,\delta_1,\omega_1,\delta_2\omega_2],
\newline
[\psi,\phi,a,y_{2_0},y_{1_0}]$ \\
\addlinespace
& $\delta$
& $[x_0],[(\text{all others})]$
& $[b,\delta_2,x_0,\omega_2,\delta_1,\omega_1],
\newline
[\psi,a,({\phi,y_2}_0,y_{1_0})]$
& $[b,\delta_2,\omega_2,\delta_1,\omega_1,\psi],
\newline
[a,y_{2_0},x_0,\phi,y_{1_0}]$
& $[b,\delta_2,\omega_2,\delta_1,\omega_1,\psi],
\newline
[a,x_0,y_{2_0},\phi,y_{1_0}]$ \\
\midrule
$y_1$
& $s_{T}$
& $[y_{1_0}],[(\text{all others})]$
& $[b,\delta_2,\delta_1,\psi,\omega_1,\omega_2],
\newline[\phi,y_{1_0},x_0,y_{2_0},a]$
& $[b,\delta_2,\delta_1,\psi,\omega_1,\omega_2,\phi],
\newline
[x_0,y_{2_0},(a,y_{1_0})]$
& $[\omega_1,b,\delta_2,\delta_1,\phi,\psi,\omega_2],
\newline
[x_0,y_{2_0},a,y_{1_0}]$ \\
\addlinespace
& $\mu^{\star}$
& $[y_{1_0}],[(\text{all others})] $
& $[b,x_0,\phi,\omega_1,\delta_1,y_{1_0}],
\newline
[\delta_2,\psi,\omega_2,y_{2_0},a]$
& $[b,x_0,\delta_2,\omega_1,\omega_2,\phi,\psi,\delta_1],
\newline
[y_{2_0},y_{1_0},a]$
& $[b,\delta_2,\omega_1,x_0,\delta_1,\omega_2,\psi,\phi],
\newline
[a,y_{1_0},y_{2_0}]$ \\
\addlinespace
& $\delta$
& $[y_{2_0}],[(\text{all others})]$
& $[y_{1_0},b,\psi,\delta_2,\omega_2,\phi],
\newline
[x_0,y_{2_0},a,\omega_1,\delta_1]$
& $[\omega_2,b,\delta_1,\delta_2,\psi,\phi,],
\newline
[(a,\omega_1,x_0,y_{1_0},y_{2_0})]$
& $[(a,\phi, \omega_1,x_0,y_{1_0},y_{2_0},\omega_2)],
\newline
[b,\delta_2,\psi,\delta_1]$ \\
\midrule
$y_2$
& $s_{T}$
& $[\omega_2,b,y_{2_0},x_0,\omega_1,\phi,\psi],
\newline
[\delta_2,y_{1_0},(a,\delta_1)]$
& $[b,\delta_2,\delta_1,\phi,\omega_2,\psi,\omega_1],
\newline
[x_0,y_{2_0},(a,y_{1_0})]$
& $[b,\delta_2,\delta_1,\omega_2,\phi,\psi,\omega_1],
\newline
[x_0,y_{1_0},y_{2_0},a]$
& $[\phi, \delta_2,\psi,b,\omega_1,\delta_1,\omega_2],
\newline
[x_0,(a,y_{1_0},y_{2_0})]$ \\
\addlinespace
& $\mu^{\star}$
& $[\omega_2,b,\psi,\omega_1,\phi,x_0 ],
\newline
[\delta_2,y_{2_0},y_{1_0},\delta_1,a]$
& $[b,\omega_2,\delta_2,\phi,x_0,\omega_1,\psi],
\newline
[\delta_1,y_{2_0},y_{1_0},a]$
& $[b,\delta_2,\omega_2,x_0,\phi,\psi,\omega_1,\delta_1],
\newline
[y_{2_0},a,y_{1_0}]$
& $[\delta_2,\omega_2,\delta_1,b,a,x_0,\omega_1],
\newline
[{y_{1_0},\psi,\phi,y_2}_0]$ \\
\addlinespace
& $\delta$
& $[y_{2_0},b,\omega_2,\omega_1,\phi,\psi],
\newline
[\delta_2,\delta_1,x_0,y_{1_0},a]$
& $[y_{2_0},b,\delta_1,\omega_1,\psi,y_{1_0},a,\omega_1,\phi],
\newline
[\delta_2,x_0,a]$
& $[b,\delta_1,\omega_1,\psi,y_{1_0},a,y_{2_0},\phi, x_0],
\newline
[\delta_2]$
& $[b,\delta_2,\omega_2,\omega_1,\psi,\phi],
\newline
[\delta_1,y_{1_0}, x_0,y_{2_0},a]$ \\
\bottomrule
\end{tabular*}
\end{table}
\end{document}
答案2
这样的表格很难适应合理的文本宽度：即使\footnotesize我得到了 145pt 的超宽，这大约是标准文本宽度的三分之一。
您可以使用 旋转桌子sidewaystable。
\documentclass[a4paper, twoside]{report} % 'twoside' when printing
\usepackage{booktabs,array,amsmath,rotating}
\begin{document}
\begin{sidewaystable}[htp]
\centering
\caption{Total Effect}\label{te}
\begin{tabular}{@{} *{2}{>{$}c<{$}} *{4}{>{$}l<{$}} @{}}
\toprule
& \begin{tabular}{@{}c@{}}Si \\ index\end{tabular}
& \multicolumn{1}{c}{Max}
& \multicolumn{1}{c}{Mean}
& \multicolumn{1}{c}{Median}
& \multicolumn{1}{c@{}}{Eqm}
\\
\midrule
x
& s_{T}
& [x_{0}],
& [b\, \delta_{2}, \delta_{1}, \omega_{2}, \omega_{1}, \psi, x_{0}],
& [b, \delta_{2}, \delta_{1}, \omega_{2}, \omega_{1}, \psi, \phi],
& [b, \delta_{2}, \delta_{1}, \omega_{1}, \omega_{2}, \psi, \phi],
\\
&
& [(\text{all others})]
& [\phi,(a,{y_{1}}_{0}, {y_{2}}_{0})]
& [{y_{1}}_{0}, a, x_{0}, {y_{2}}_{0}]
& [x_{0}, ({a, y_{1}}_{0}, {y_{2}}_{0})]
\\
\addlinespace
& \mu^{\star}
& [x_{0}],
& [b, x_{0}, \delta_{1}, \omega_{1}, \delta_{2}, \omega_{2}],
& [b, x_{0}, \omega_{1}, \delta_{1}, \delta_{2}\omega_{2}],
& [b, x_{0}, \delta_{1}, \omega_{1}, \delta_{2}\omega_{2}],
\\
&
& [(\text{all others})]
& [\psi, \phi, {y_{2}}_{0}, {y_{1}}_{0}, a]
& [\psi, \phi, a, {y_{2}}_{0}, {y_{1}}_{0}]
& [\psi, \phi, a, {y_{2}}_{0}, {y_{1}}_{0}]
\\
\addlinespace
& \delta
& [x_{0}],
& [b, \delta_{2}, x_{0}, \omega_{2}, \delta_{1}, \omega_{1}],
& [b, \delta_{2}, \omega_{2}, \delta_{1}, \omega_{1}, \psi],
& [b, \delta_{2}, \omega_{2}, \delta_{1}, \omega_{1}, \psi],
\\
&
& [(\text{all others})]
& [\psi, a, ({\phi, y_{2}}_{0}, {y_{1}}_{0})]
& [a, {y_{2}}_{0}, x_{0}, \phi, {y_{1}}_{0}]
& [a, x_{0}, {y_{2}}_{0}, \phi, {y_{1}}_{0}]
\\
\midrule
y_{1}
& s_{T}
& [{y_{1}}_{0}],
& [b, \delta_{2}, \delta_{1}, \psi, \omega_{1}, \omega_{2}],
& [b, \delta_{2}, \delta_{1}, \psi, \omega_{1}, \omega_{2}, \phi],
& [\omega_{1}, b, \delta_{2}, \delta_{1},\phi, \psi, \omega_{2}],
\\
&
& [(\text{all others})]
& [\phi, {y_{1}}_{0}, x_{0}, {y_{2}}_{0}, a]
& [x_{0}, {y_{2}}_{0}, (a, {y_{1}}_{0})]
& [x_{0}, {y_{2}}_{0}, a, {y_{1}}_{0}]
\\
\addlinespace
& \mu^{\star}
& [{y_{1}}_{0}],
& [b, x_{0}, \phi, \omega_{1}, \delta_{1}, {y_{1}}_{0}],
& [b, x_{0}, \delta_{2}, \omega_{1}, \omega_{2}, \phi, \psi, \delta_{1}],
& [b, \delta_{2}, \omega_{1}, x_{0}, \delta_{1}, \omega_{2}, \psi, \phi],
\\
&
& [(\text{all others})]
& [\delta_{2}, \psi, \omega_{2}, {y_{2}}_{0}, a]
& [{y_{2}}_{0}, {y_{1}}_{0}, a]
& [a, {y_{1}}_{0}, {y_{2}}_{0}]
\\
\addlinespace
& \delta
& [{y_{2}}_{0}],
& [{y_{1}}_{0}, b, \psi, \delta_{2}, \omega_{2}, \phi],
& [\omega_{2}, b, \delta_{1}, \delta_{2}, \psi, \phi, ],
& [(a, \phi, \omega_{1}, x_{0}, {y_{1}}_{0}, {y_{2}}_{0},\ \omega_{2})],
\\
&
& [(\text{all others})]
& [x_{0}, {y_{2}}_{0}, a, \omega_{1}, \delta_{1}]
& [(a, \omega_{1}, x_{0}, {y_{1}}_{0}, {y_{2}}_{0})]
& [b, \delta_{2}, \psi, \delta_{1}]
\\
\midrule
y_{2}
& s_{T}
& [\omega_{2}, b,{y_{2}}_{0}, x_{0}, \omega_{1}, \phi, \psi],
& [b, \delta_{2}, \delta_{1}, \phi, \omega_{2}, \psi, \omega_{1}],
& [b, \delta_{2}, \delta_{1}, \omega_{2}, \phi, \psi, \omega_{1}],
& [\phi, \delta_{2}, \psi, b, \omega_{1}, \delta_{1}, \omega_{2}],
\\
&
& [\delta_{2}, {y_{1}}_{0}, (a, \delta_{1})]
& [x_{0}, {y_{2}}_{0}, (a, {y_{1}}_{0})]
& [x_{0}, {y_{1}}_{0}, {y_{2}}_{0}, a]
& [x_{0}, (a, {y_{1}}_{0}, {y_{2}}_{0})]
\\
\addlinespace
& \mu^{\star}
& [\omega_{2}, b, \psi, \omega_{1}, \phi, x_{0} ],
& [b, \omega_{2}, \delta_{2}, \phi, x_{0}, \omega_{1}, \psi],
& [b, \delta_{2}, \omega_{2}, x_{0}, \phi, \psi, \omega_{1}, \delta_{1}],
& [\delta_{2}, \omega_{2}, \delta_{1}, b,a, x_{0}, \omega_{1}],
\\
&
& [\delta_{2}, {y_{2}}_{0}, {y_{1}}_{0}, \delta_{1}, a]
& [\delta_{1}, {y_{2}}_{0}, {y_{1}}_{0}, a]
& [{y_{2}}_{0}, a, {y_{1}}_{0}]
& [{{y_{1}}_{0}, \psi, \phi, y_{2}}_{0}]
\\
\addlinespace
& \delta
& [{y_{2}}_{0}, b, \omega_{2}, \omega_{1}, \phi, \psi],
& [{y_{2}}_{0}, b, \delta_{1}, \omega_{1}, \psi, {y_{1}}_{0}, a, \omega_{1}, \phi],
& [b, \delta_{1}, \omega_{1}, \psi, {y_{1}}_{0}, a, {y_{2}}_{0}, \phi, x_{0}],
& [b, \delta_{2}, \omega_{2}, \omega_{1}, \psi, \phi],
\\
&
& [\delta_{2}, \delta_{1}, x_{0}, {y_{1}}_{0}, a]
& [\delta_{2}, x_{0}, a]
& [\delta_{2}]
& [\delta_{1}, {y_{1}}_{0}, x_{0}, {y_{2}}_{0}, a]
\\
\bottomrule
\end{tabular}
\end{sidewaystable}
\end{document}
我避开了所有\newline说明和繁琐的规则。没有必要\multirow，这甚至可能使表格变得模棱两可。
答案3
目前还不清楚你到底想要什么改变，但我认为你需要研究一下\cline（提示：在你不想在左列有一行的地方写\cline{2-6}而不是），然后用和替换，因为它们搞砸了表格底部和顶部的间距\hline\toprule\bottomrule\hline