Changeset 1142 in Sophya for trunk/DocHFI_L2

Timestamp:

Aug 25, 2000, 5:27:57 PM (25 years ago)

Author:

ansari

Message:

DocL2 style file and example, work on WBS - Reza 25/8/2000

Location:

trunk/DocHFI_L2

Files:

• L2L3_DMC_spec.html (added)
• defdocl2.sty (added)
• exdocl2.tex (added)
• wbsl2.tex (modified) (7 diffs)

trunk/DocHFI_L2/wbsl2.tex

@@ -1 +1 @@
 \documentclass[twoside,11pt]{article}
+
+%  Definition pour Documentation L2
+\usepackage{defdocl2}
+
 %  Package standard : Utilisation de caracteres accentues, mode francais et graphique
 \usepackage[latin1]{inputenc}
 \usepackage[T1]{fontenc}
 \usepackage{babel}
-\usepackage{graphicx}
+% \usepackage{graphicx}
 % package a mettre pour faire du pdf
-\usepackage{palatino}
+% \usepackage{palatino}
+
 
 %  Extension de symboles mathematiques
 \usepackage{amssymb}
-
-%  Definition de taille de page
-\setlength{\textwidth}{16cm}
-\setlength{\textheight}{21.5cm}
-\setlength{\topmargin}{0.5cm}
-\setlength{\oddsidemargin}{0.cm}
-\setlength{\evensidemargin}{0.cm}
-\setlength{\unitlength}{1mm}
-
+\usepackage{amstex}
+
+
+%  Definition de taille de page (c'est ds defdocl2.sty)
 \newcommand{\bul}{$\bullet \ $}
 \newcommand{\gph}[1]{ {\bf GPH#1} }
 \newcommand{\ngph}[1]{ GPH#1 }
 
+%  Symboles en bold 
+\newcommand{\bnu}{\boldsymbol{\nu}}
+\newcommand{\bbold}{\boldsymbol{b}}
+\newcommand{\dbold}{\boldsymbol{d}}
+
 \begin{document}
 
 \begin{titlepage}
-\vspace{1cm}
-\makebox[30mm][c]{\includegraphics[width=3cm]{hfi_icon_vsmall.eps}}
-\raisebox{12mm}{\rule{80 mm}{0.5 mm}\makebox[50 mm]{\bf Planck HFI L2}}
-\vspace{2cm}
-\begin{center}
-\par \renewcommand{\baselinestretch}{2.0} \small 
-{\LARGE \bf 
+\titleph{
 Planck HFI L2 \\ 
 Work Breakdown Structure \\
 Package Breakdown Structure
 }
-
-\par \renewcommand{\baselinestretch}{1.0} \normalsize
-\vspace{2 cm}
-\begin{tabular}{ll}
-R. Ansari & LAL \\ % & {\tt ansari@lal.in2p3.fr} \\
-I.J. Grivell  & ICSTM \\ 
+%  Authors list
+\authors{
+R. Ansari & LAL, Orsay \\ % & {\tt ansari@lal.in2p3.fr} \\
+I.J. Grivell  & ICSTM, London \\ 
+G. Le Meur & LAL, Orsay \\
 R.G. Mann  &  IfA, Edinburgh \\ 
-C. Mercier & IAS \\ % & {\tt Claude.Mercier@ias.fr} \\
-M. Rowan-Robinson  & ICSTM \\ 
+M. Rowan-Robinson  & ICSTM, London \\ 
 S. Serjeant  & ICSTM \\ 
-J.F. Sygnet & IAS \\ % {\tt Jean-Francois.Sygnet@ias.fr} \\
-
-% {É. Aubourg} & {\tt aubourg@hep.saclay.cea.fr} \\
-% {É. Lesquoy} & {\tt lesquoy@hep.saclay.cea.fr} \\
-% {C. Magneville} & {\tt cmv@hep.saclay.cea.fr} \\
-\end{tabular}
-
-\end{center}
-\vfill
-\hfill 
-\framebox[\textwidth]{\hspace{0.5cm} \bf Planck HFI Level 2 
-\hspace{1cm} \today } \\
+J.F. Sygnet & IAS, Orsay \\ % {\tt Jean-Francois.Sygnet@ias.fr} \\
+}
+
+\titlepfd{PL-HFI-LAL-PW-L2001}{2.0}
+
 \end{titlepage}
 
-\vspace*{1cm}
-\begin{center}
-\mbox{
-\rule{50 mm}{0.6 mm} \makebox[60 mm]{\bf Revision history} \rule{50 mm}{0.6 mm} }
-\end{center}
-\vspace{2 mm}
+%   -------- Revision history
+\revisionhistory
 \begin{itemize}
 \item Version 1.0 (February 2000 - CVS version 1.1) \\
@@ -72 +58 @@
 \item Version 1.1 (April 2000 - CVS version 1.2) \\
 Draft updated using the document prepared at ISCTM and IfA (Edinburgh)
-\end{itemize}
-
+\item Version 2.0 (August 2000 - CVS version 1.3) \\
+Inclusion of a section describing notation and conventions, 
+flow charts. A more detailed description of deliverables is also included.
+\end{itemize}
+
+%   -------- Table of content
 \newpage
-
 \tableofcontents
-
 \newpage
-% \tableofcontents
 
 \section{Introduction}
@@ -106 +93 @@
 \item[]\gph{422}  TOI processing
 \item[]\gph{423}  Polarised TOI processing
-\item[]\gph{424}  Simple 2-D map reconstruction from TOI's
-\item[]\gph{425}  Global 2-D map reconstruction
-\item[]\gph{426}  Global 2-D polarised map reconstruction
+\item[]\gph{424}  Basic 2-D map reconstruction from TOI's
+\item[]\gph{425}  Optimal 2-D map reconstruction
+\item[]\gph{426}  Optimal 2-D polarised map reconstruction
 \item[]\gph{427}  Early Compact Source Catalogue
 \item[]\gph{428}  General software architecture and support modules
@@ -114 +101 @@
 \end{itemize}
 
-In addition to the specific Level 2 workpackages, the following are 
-also related to Level 2 data processing:
+The package \gph424 should provide a resonably fast and simple 
+method for reconstructing 2-D maps from cleaned TOI's (from 
+\gph422 and \gph423), removing systematic effects (destriping) 
+and deconvolving the antenna beam pattern. An iterative method 
+is foreseen, capable of dealing with partial knowledge of 
+instrument caracteristics.
+The optimal 2-D map reconstruction packages (\gph425 and \gph426)
+will implement the best feasible method for analysing the whole
+data set from the HFI instrument and building the full sky frequency 
+maps.
 
 \begin{itemize}
@@ -158 +153 @@
 \end{table}
 
-
+\section{HFI data processing steps}
+The major steps for processing Planck-HFI data are briefly described here.
+For the sake of clarity, we define here the notation and conventions used
+throughout this document for referring to the different data components 
+in planck HFI. Most of these data components are also defined in 
+\cite{datamodel}.
+
+\subsection{Notation and conventions}
+\begin{itemize}
+\item[] {\bf Coordinates:} The spacecraft attitude is defined by the spin 
+axis direction $SA (\theta, \phi)$. $\psi$ is the third angle defining
+the position of the spacecraft and thus a given detectors view 
+direction and beam pattern orientation.
+A given sky direction is denoted $(\alpha,\delta)$ in equatorial coordinates, 
+$(l,b)$ in Galactic coordinates or $(\lambda,\beta)$ in ecliptic coordinate.
+\item[] {\bf Detector:} A given HFI bolometer read-out channel. The corresponding
+signal is denoted $\dbold(t)$ or $\bbold(t)$ $\dbold^j(t)$ or $\bbold^j(t)$ where $j$ is the 
+bolometer number.
+\item[] {\bf Frequency channel:} The set of detectors working in the 
+same frequency range. This information is only obtained by combining 
+information from several detectors in the corresponding frequency band.
+The subscript $\bnu$ is used to denote a frequency channel. The sky map
+in a given frequency band would be written as $Sky  (\theta,\phi) \vert ^{\bnu}$.
+\item[] {\bf Scan:} The time interval corresponding to a nominal spin axis
+direction
+
+\end{itemize}
+
+\subsection{Processing steps}
+
+
+ 
 \section{GPH421: RTA/QLA Real Time Assesment, Quick Look Analysis}
 \begin{itemize}
@@ -173 +199 @@
 perfomed on TOI's (Time Ordered Information ) for either a 
 single-detector or multpile-detector, single-frequency set 
-of TOI's.
+of TOI's. A very rough sketch of data flow and processing 
+steps for GPH422 is given in figure \ref{fig422}.
+
+\begin{figure}[htbp]
+\mbox{\hspace*{1cm} \includegraphics[width=7cm]{gph422_1.eps}
+      \includegraphics[width=7cm]{gph422_2.eps} }
+\caption{Data flow and processing steps for GPH422}
+\label{fig422}
+\end{figure}
 
 \begin{itemize}
@@ -422 +456 @@
 \end{itemize} 
 
+\begin{thebibliography}{10}
+\bibitem{datamodel}
+\newblock {\bf PL-COM-OAT-TN-003}
+\newblock {Planck IDIS Data Model Description Document}
+\end{thebibliography}
+
+
 \end{document}