немного примеров в TeX

This commit is contained in:
Kolan Sh 2011-05-27 10:19:37 +04:00
parent 6c286e1e8c
commit b2200288a2
7 changed files with 2687 additions and 84 deletions

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@ -5,3 +5,10 @@ syntax: glob
*.gcno
*.out
callgrind.out.*
*.dat
*.aux
*.dvi
*.log
*.*~
*.~*
*.pdf

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@ -172,88 +172,4 @@ $S_g^2$ & variance coefficient of the spatial gain noise~[\%] \\
\end{center}
\end{table}
%~ http://samolisov.blogspot.com/2008/06/latex_13.html
\begin{longtable}{|p{2cm}|p{8cm}|c|c|c|c|c|c|c|c|}
\kill
\caption{\spaceПеречень, параметры и вероятностные характеристики работ СГ\label{works}\\
\hline
\multirowthead{2}{Код раб.} & \multirowthead{2}{Наименование работы} & \multicolumn{3}{|c|}{Продолж., дн.} & \multicolumn{3}{|c|}{Исполн., чел.} & \multirowthead{2}{$\delta_{ij},$ дн.} & \multirowthead{2}{$\Delta_{ij}, \text{дн.}^2$} \\
\cline{3-8}
& & мин. & макс. & ожид. & рук. & прогр. & лаб. & &\\
\hline
\endfirsthead
\kill
\caption{\space}\\
\LTleft=\z@
\LTright=\fill
\def\LT@makecaption#1#2#3{%
\LT@mcol\LT@cols l{\hbox to\z@{\parbox[t]\LTcapwidth{%
\ifx#3\space
\sbox\@tempboxa{#1{}Продолжение таблицы \@arabic\c@table}%
\else
\sbox\@tempboxa{#1{#2\captionlabeldelim{}}#3}%
\fi
{\box\@tempboxa\hfil}%
\endgraf}%
\hss}}}
\setlength\abovecaptionskip{2\p@}
\setlength\belowcaptionskip{1\p@}
\def\capfigure{figure}
\def\captable{table}
\long\def\@makecaption#1#2{%
\vskip\abovecaptionskip
\ifx\@captype\capfigure
\centering #1~--~#2 \par
\else
#1~--~#2 \par
\fi
\vskip\belowcaptionskip}
\renewcommand{\@biblabel}[1]{#1}
\thead{Частное\\I-го рода}
\multirowthead{2}{Ожид.\\прод.}
\hline
\makecell[b]{Минимально\\необходимые,\\не менее} & 400 & 600 & \multirowcell{3}{от 0,4 до 1,0 включ.} \\
\end{document}

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\documentclass[a4paper,12pt,russian]{article}
\usepackage[utf8]{inputenc}
\usepackage[russian]{babel}
\usepackage{array,longtable}
\usepackage{rotating}
\usepackage{setspace}
\usepackage{geometry}
\usepackage{float}
%~ \usepackage{setspace,supertabular}
\title{Temporary Report =)}
\author{Kolan Sh.}
\date{\today}
\setcounter{LTchunksize}{100}
\begin{document}
\begin{center}
\begin{longtable}{|p{1in}@{}|p{1in}@{}|p{.4in}@{}|p{.4in}@{}|p{.4in}@{}|p{.4in}@{}|p{.4in}@{}|}
\hline \textbf{A}&\textbf{B}& \multicolumn{5}{|c|}{\textbf{C}}\\
\cline{3-7} &&\textbf{
i}&\textbf{ii}&\textbf{iii}&\textbf{iv}&\textbf{v}\\\hline
\endfirsthead
\multicolumn{7}{c}%
{{\bfseries \tablename\ \thetable{} -- continued from previous page}} \\
\hline \textbf{A}&\textbf{B}& \multicolumn{5}{|c|}{\textbf{C}}\\
\cline{3-7} &&\textbf{
i}&\textbf{ii}&\textbf{iii}&\textbf{iv}&\textbf{v}\\\hline
\endhead
\hline \multicolumn{7}{|r|}{{Continued on next page}} \\ \hline
\endfoot
%************************************************
\hline
\textbf{Blah}&\textbf{Blah}&\small{1}&\small{2}&\small{3}&\small{4}&\small{5}\\
\cline{2-7}
\textbf{Blah1}&\textbf{Blah1}&\small{1}&\small{2}&\small{3}&\small{4}&\small{5}\\
\hline
\textbf{Blah1}&\textbf{Blah1}&\small{1}&\small{2}&\small{3}&\small{4}&\small{5}\\
\cline{2-7}
\textbf{Blah1}&\textbf{Blah1}&\small{1}&\small{2}&\small{3}&\small{4}&\small{5}\\
\hline \textbf{Blah}&\textbf{Blah}&\small{1}&\small{2}&\small{3}&\small{4}&\small{5}\\
\cline{2-7}
\textbf{Blah1}&\textbf{Blah1}&\small{1}&\small{2}&\small{3}&\small{4}&\small{5}\\
\hline
\textbf{Blah1}&\textbf{Blah1}&\small{1}&\small{2}&\small{3}&\small{4}&\small{5}\\
\cline{2-7}
\textbf{Blah1}&\textbf{Blah1}&\small{1}&\small{2}&\small{3}&\small{4}&\small{5}\\
\hline
\textbf{Blah1}&\textbf{Blah1}&\small{1}&\small{2}&\small{3}&\small{4}&\small{5}\\
\cline{2-7}
\textbf{Blah1}&\textbf{Blah1}&\small{1}&\small{2}&\small{3}&\small{4}&\small{5}\\
\caption[ABC]{\label{tab:something}Table about something}
\endlastfoot
\end{longtable}
\end{center}
%~ \end{document}
%~ Многостраничные таблицы
%~ \begin{longtable}[h]{lp{0.7\linewidth}}
%~ $A$ & area of the (geometrical) pixel [m\textsuperscript2] \\
%~ $c$ & Speed of light $\approx 3 \cdot 10^8$ m/s \\
%~ $DYN_{in}$ & Input dynamic range [1] \\
%~ $DYN_{out}$ & Output dynamic range~[1] \\
%~ $E$ & irradiance on the sensor surface~[W/m\textsuperscript2] \\
%~ $F$ & Non-whiteness coefficient \\
%~ $h$ & Planck's constant h $\approx6.63 \cdot 10^{-34} Js$ \\
%~ $K$ & overall system gain~[DN/e-] \\
%~ $k_d$ & Doubling temperature of the dark current~[$^\circ$C] \\
%~ $N_d$ & dark current~[e-/s] \\
%~ $N_{d30}$ & dark current for a housing temperature of $30^\circ C$~[e-/s]\textsuperscript2 \\
%~ $S_g^2$ & variance coefficient of the spatial gain noise~[\%] \\
%~ \end{longtable}
\end{document}

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%% LyX 1.6.8 created this file. For more info, see http://www.lyx.org/.
%% Do not edit unless you really know what you are doing.
\documentclass[12pt,a4paper,russian]{article}
\usepackage[T1]{fontenc}
\usepackage[utf8]{inputenc}
\usepackage{array}
\usepackage{longtable}
\usepackage{textcomp}
\makeatletter
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% LyX specific LaTeX commands.
\special{papersize=\the\paperwidth,\the\paperheight}
\DeclareRobustCommand{\cyrtext}{%
\fontencoding{T2A}\selectfont\def\encodingdefault{T2A}}
\DeclareRobustCommand{\textcyr}[1]{\leavevmode{\cyrtext #1}}
\AtBeginDocument{\DeclareFontEncoding{T2A}{}{}}
%% Because html converters don't know tabularnewline
\providecommand{\tabularnewline}{\\}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% User specified LaTeX commands.
\usepackage{array}\usepackage{longtable}\usepackage{rotating}\usepackage{float}%~ \usepackage{setspace,supertabular}
\title{Temporary Report =)}
\author{Kolan Sh.}
\date{\today}
%~ \setlongtables % obsolete
\setlength{\LTleft}{\parindent}
\setlength{\LTright}{\fill}
\setcounter{LTchunksize}{4}
\makeatother
\usepackage{babel}
\begin{document}
Кое-кто из комментаторов распалялся по поводу того, что, дескать,
{}``всё уже давно написано, читайте книжки''. Я ещё раз уточню свою
позицию по этому поводу: время тыкания людей в пудовые талмуды и дурно
написанные маны прошло. Документация, как и программы, должны быть
повёрнуты к пользователю лицом, а не задницей. Специализированные
методические пособия типа этого помогут людям начать разбираться с
предметом, подталкивая к изучению книг и делая кривую обучения более
пологой. Но это лирика и я не буду на ней задерживаться.
\begin{center}
\begin{longtable}{|p{0.1\linewidth}|p{0.1\linewidth}|p{0.1\linewidth}|p{0.1\linewidth}|p{0.1\linewidth}|p{0.1\linewidth}|p{0.1\linewidth}|p{0.1\linewidth}|}
\caption[SuperPuperMyTable]{Заголовок таблицы =)}
\label{label_grid1} \tabularnewline
\caption[SuperPuperMyTable]{Заголовок таблицы =)}
\label{label_grid1} \tabularnewline
\hline
\multicolumn{1}{|p{0.1\linewidth}|}{\textbf{Канал(1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Полином(1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Минимум / Максимум(1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Замер №34(1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Замер №42(1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Замер №65(1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Единицы измерения(1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Приведённые единицы измерения(1)}}\tabularnewline
\multicolumn{1}{|p{0.1\linewidth}|}{\textbf{Время(1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{15:54:32.65(1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{НЕ ОПР.(1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{2011.05.26 15:54:32.65(1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Поле3(1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Поле3(1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Поле3(1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Поле4(1)}}\tabularnewline
\endfirsthead
\hline
% подпись и заголовки при переносе
\multicolumn{8}{c}{{\bfseries \tablename\ \thetable{} -- продолжение}} & & & & & & & \tabularnewline
\hline
\multicolumn{1}{|p{0.1\linewidth}|}{\textbf{Канал(!1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Полином(!1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Минимум / Максимум(!1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Замер №34(!1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Замер №42(!1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Замер №65(!1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Единицы измерения(!1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Приведённые единицы измерения(!1)}}\tabularnewline
\multicolumn{1}{|p{0.1\linewidth}|}{\textbf{Время(!1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{15:54:32.65(!1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{НЕ ОПР.(!1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{2011.05.26 15:54:32.65(!1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Поле3(!1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Поле3(!1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Поле3(!1)}} & \multicolumn{1}{p{0.1\linewidth}|}{\textbf{Поле4(!1)}}\tabularnewline
\hline
\endhead
\hline
\multicolumn{8}{|r|}{{Продолжение на следующей странице}}\tabularnewline
\hline
\endfoot
\hline
t{*}вх & 2.5500000E-5;2.5500000E-5;2.5500000E-5; & 18.00 / 19.00 & 21.32 & 19.11 & 18.33 & Град.$\,^{\circ}\mbox{C}$ & Град.$\,^{\circ}\mbox{C}$ \tabularnewline
t{*}вх & 2.5500000E-5;2.5500000E-5;2.5500000E-5; & 18.00 / 19.00 & 21.32 & 19.11 & 18.33 & Град.$\,^{\circ}\mbox{C}$ & Град.$\,^{\circ}\mbox{C}$ \tabularnewline
t{*}вх & 2.5500000E-5;2.5500000E-5;2.5500000E-5; & 18.00 / 19.00 & 21.32 & 19.11 & 18.33 & Град.$\,^{\circ}\mbox{C}$ & Град.$\,^{\circ}\mbox{C}$ \tabularnewline
t{*}вх & 2.5500000E-5;2.5500000E-5;2.5500000E-5; & 18.00 / 19.00 & 21.32 & 19.11 & 18.33 & Град.$\,^{\circ}\mbox{C}$ & Град.$\,^{\circ}\mbox{C}$ \tabularnewline
t{*}вх & 2.5500000E-5;2.5500000E-5;2.5500000E-5; & 18.00 / 19.00 & 21.32 & 19.11 & 18.33 & Град.$\,^{\circ}\mbox{C}$ & Град.$\,^{\circ}\mbox{C}$ \tabularnewline
t{*}вх & 2.5500000E-5;2.5500000E-5;2.5500000E-5; & 18.00 / 19.00 & 21.32 & 19.11 & 18.33 & Град.$\,^{\circ}\mbox{C}$ & Град.$\,^{\circ}\mbox{C}$ \tabularnewline
t{*}вх & 2.5500000E-5;2.5500000E-5;2.5500000E-5; & 18.00 / 19.00 & 21.32 & 19.11 & 18.33 & Град.$\,^{\circ}\mbox{C}$ & Град.$\,^{\circ}\mbox{C}$ \tabularnewline
\end{longtable}
\par\end{center}
\begin{tabular}{|p{0.1\linewidth}|p{0.1\linewidth}|p{0.1\linewidth}||}
\hline
longlong text & longl-ongtext & longlon-glongtext \tabularnewline
\hline
lsajf;slkfa-slk;jflsdjf;ls & lskdjf;lsd-jf;ldskjf & sldkf-j;lsdjfsds \tabularnewline
\hline
\end{tabular}
\begin{longtable}{@{*}r||p{1in}@{*}}
\caption[]{(continued)}
\tabularnewline
KILLED & LINE!!!! \kill \caption[An optional table caption ...]{A long table\label{long}}
\tabularnewline
\hline
\hline
\multicolumn{2}{@{*}c@{*}}{}\tabularnewline
\textsc{First} & \textsc{Second}\tabularnewline
\hline
\endfirsthead
\caption[]{(continued)}
\tabularnewline
\hline
\multicolumn{2}{@{*}c@{*}}{}\tabularnewline
\textbf{First} & \textbf{Second}\tabularnewline
\hline
\endhead
\hline
This goes at the & bottom.\tabularnewline
\hline
\endfoot
\hline
These lines will & appear\tabularnewline
in place of the & usual foot\tabularnewline
at the end & of the table\tabularnewline
\endlastfoot
\hline
%~ \env{longtable} columns are specified& in the \\
%~ same way as in the \env{tabular}& environment.\\
%~ ...
\multicolumn{2}{||c||}{This is a ...} & \tabularnewline
%~ ...
Some lines may take... & \raggedleft This last column is a p column... \tabularnewline
%~ ...
Lots of lines & like this.\tabularnewline
\hline
%~ ...
Lots%
\footnote{...%
} of lines & like this.\tabularnewline
Lots of lines & like this%
\footnote{...%
}\tabularnewline
\hline
Lots of lines & like this.\tabularnewline
%~ ...
& \tabularnewline
\end{longtable}
\end{document}

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#LyX file created by tex2lyx 1.6.8
\lyxformat 264
\begin_document
\begin_header
\textclass article
\begin_preamble
\usepackage{array}\usepackage{longtable}\usepackage{rotating}\usepackage{float}
\end_preamble
\language russian
\inputencoding utf8
\font_roman default
\font_sans default
\font_typewriter default
\font_default_family default
\font_sc false
\font_osf false
\font_sf_scale 100
\font_tt_scale 100
\graphics default
\paperfontsize 12
\spacing single
\papersize a4paper
\use_geometry false
\use_amsmath 1
\use_esint 1
\cite_engine basic
\use_bibtopic false
\paperorientation portrait
\secnumdepth 3
\tocdepth 3
\paragraph_separation indent
\defskip medskip
\quotes_language french
\papercolumns 1
\papersides 1
\paperpagestyle default
\tracking_changes false
\output_changes false
\end_header
\begin_body
\begin_layout Standard
\begin_inset Tabular
<lyxtabular version="3" rows="12" columns="2">
<features islongtable="true">
<column alignment="left" valignment="top">
<column alignment="none" valignment="top" width="70line%">
<row>
<cell alignment="left" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
\begin_inset Formula $A$
\end_inset
\end_layout
\end_inset
</cell>
<cell alignment="none" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
area of the (geometrical) pixel [m
\begin_inset ERT
status collapsed
\begin_layout Standard
\backslash
textsuperscript
\end_layout
\end_inset
2]
\end_layout
\end_inset
</cell>
</row>
<row>
<cell alignment="left" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
\begin_inset Formula $c$
\end_inset
\end_layout
\end_inset
</cell>
<cell alignment="none" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
Speed of light
\begin_inset Formula $\approx 3 \cdot 10^8$
\end_inset
m/s
\end_layout
\end_inset
</cell>
</row>
<row>
<cell alignment="left" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
\begin_inset Formula $DYN_{in}$
\end_inset
\end_layout
\end_inset
</cell>
<cell alignment="none" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
Input dynamic range [1]
\end_layout
\end_inset
</cell>
</row>
<row>
<cell alignment="left" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
\begin_inset Formula $DYN_{out}$
\end_inset
\end_layout
\end_inset
</cell>
<cell alignment="none" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
Output dynamic range\InsetSpace ~
[1]
\end_layout
\end_inset
</cell>
</row>
<row>
<cell alignment="left" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
\begin_inset Formula $E$
\end_inset
\end_layout
\end_inset
</cell>
<cell alignment="none" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
irradiance on the sensor surface\InsetSpace ~
[W/m
\begin_inset ERT
status collapsed
\begin_layout Standard
\backslash
textsuperscript
\end_layout
\end_inset
2]
\end_layout
\end_inset
</cell>
</row>
<row>
<cell alignment="left" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
\begin_inset Formula $F$
\end_inset
\end_layout
\end_inset
</cell>
<cell alignment="none" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
Non-whiteness coefficient
\end_layout
\end_inset
</cell>
</row>
<row>
<cell alignment="left" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
\begin_inset Formula $h$
\end_inset
\end_layout
\end_inset
</cell>
<cell alignment="none" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
Planck's constant h
\begin_inset Formula $\approx6.63 \cdot 10^{-34} Js$
\end_inset
\end_layout
\end_inset
</cell>
</row>
<row>
<cell alignment="left" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
\begin_inset Formula $K$
\end_inset
\end_layout
\end_inset
</cell>
<cell alignment="none" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
overall system gain\InsetSpace ~
[DN/e-]
\end_layout
\end_inset
</cell>
</row>
<row>
<cell alignment="left" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
\begin_inset Formula $k_d$
\end_inset
\end_layout
\end_inset
</cell>
<cell alignment="none" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
Doubling temperature of the dark current\InsetSpace ~
[
\begin_inset Formula $^\circ$
\end_inset
C]
\end_layout
\end_inset
</cell>
</row>
<row>
<cell alignment="left" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
\begin_inset Formula $N_d$
\end_inset
\end_layout
\end_inset
</cell>
<cell alignment="none" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
dark current\InsetSpace ~
[e-/s]
\end_layout
\end_inset
</cell>
</row>
<row>
<cell alignment="left" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
\begin_inset Formula $N_{d30}$
\end_inset
\end_layout
\end_inset
</cell>
<cell alignment="none" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
dark current for a housing temperature of
\begin_inset Formula $30^\circ C$
\end_inset
\InsetSpace ~
[e-/s]
\begin_inset ERT
status collapsed
\begin_layout Standard
\backslash
textsuperscript
\end_layout
\end_inset
2
\end_layout
\end_inset
</cell>
</row>
<row>
<cell alignment="left" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
\begin_inset Formula $S_g^2$
\end_inset
\end_layout
\end_inset
</cell>
<cell alignment="none" valignment="top" usebox="none">
\begin_inset Text
\begin_layout Standard
variance coefficient of the spatial gain noise\InsetSpace ~
[%]
\end_layout
\end_inset
</cell>
</row>
</lyxtabular>
\end_inset
\end_layout
\end_body
\end_document

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\documentclass[a4paper,12pt,russian]{article}
\usepackage[utf8]{inputenc}
\usepackage[russian]{babel}
\usepackage{array,longtable}
\usepackage{rotating}
\usepackage{setspace}
\usepackage{geometry}
\usepackage{float}
\begin{document}
\begin{longtable}[h]{lp{0.7\linewidth}}
$A$ & area of the (geometrical) pixel [m\textsuperscript2] \\
$c$ & Speed of light $\approx 3 \cdot 10^8$ m/s \\
$DYN_{in}$ & Input dynamic range [1] \\
$DYN_{out}$ & Output dynamic range~[1] \\
$E$ & irradiance on the sensor surface~[W/m\textsuperscript2] \\
$F$ & Non-whiteness coefficient \\
$h$ & Planck's constant h $\approx6.63 \cdot 10^{-34} Js$ \\
$K$ & overall system gain~[DN/e-] \\
$k_d$ & Doubling temperature of the dark current~[$^\circ$C] \\
$N_d$ & dark current~[e-/s] \\
$N_{d30}$ & dark current for a housing temperature of $30^\circ C$~[e-/s]\textsuperscript2 \\
$S_g^2$ & variance coefficient of the spatial gain noise~[\%] \\
\end{longtable}
\end{document}