Changeset 6816 for trunk


Ignore:
Timestamp:
03/11/05 08:42:58 (20 years ago)
Author:
galante
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  • trunk/MagicSoft/GRB-Proposal/Monitor.tex

    r6814 r6816  
    4141inner pixel of the \ma camera.\\
    4242
    43 In case of alert, {\it gspot} stores the informations and enters
     43In case of alert, {\it gspot} stores the informations and enters into
    4444an {\bf Alarm State}. The duration of the alarm depends on the following parameters:
    4545
     
    5454distance from the GRB to the Moon has to be at least 30$^\circ$. This constant
    5555value of 30$^\circ$ will change in the future as soon as the camera experts
    56 will provide a plot of the safe distance from the Moon vs. Moon's phase.
     56will provide a plot of the safe distance from the Moon vs. Moon phase.
    5757Therefore such dynamical limit for this value will be used.
    5858\end{itemize}
     
    6363At the moment when the criteria listed above are fulfilled for this burst, and the time interval
    6464after the burst onset is smaller than 5 hours, {\it gspot} enters into \textcolor{red}{\bf Red Alarm State}.
    65 If all the mentioned conditions are satisfied from the beginning, {\it gspot} enters into Red Alarm State immediately.
    66 If more than one alert is recived and the burst can not be observed immediately, the alert information are saved in a list.
     65If all the mentioned conditions are satisfied from the beginning, {\it gspot} enters
     66into \textcolor{red}{\bf Red Alarm State} immediately.
     67If more than one alert is recived and the burst cannot be observed immediately,
     68the alert information are saved in a list.
    6769The software weights the alerts according the total amount of time in which
    68 the GRB will be observable, the delay from the onset of GRB's observability,
    69 the intensisty of the burst and the mean GRB's zenith angle during its
     70the GRB will be observable, the delay from the onset of GRB observability,
     71the intensisty of the burst and the mean GRB zenith angle during its
    7072period of observability.
    7173The best candidate is sent to the CC as soon as {\it gspot}
    72 enters the \textcolor{red}{\bf Red Alarm state}, i.e. as soon as such
     74enters into the \textcolor{red}{\bf Red Alarm state}, i.e. as soon as such
    7375candidate becomes observable.\\
    7476
     
    7678if the communication with the CC is available then {\it gspot} sends to it
    7779the GRB equatorial coordinates (RA/DEC J2000).
    78 For the communication with CC the format defined in~\cite{CONTROL} is used.
    79 At the same time, the shifters and the GRB-MAGIC group are contacted.
     80For the communication with CC, format defined in~\cite{CONTROL} is used.
     81At the same time, shifters and the GRB-MAGIC group are contacted.
    8082
    8183\subsection{The Interface to the Central Control}
     
    9092\begin{itemize}
    9193\item {\it gspot} receives from the CC the confirmation
    92 that the alert notice has been received (the CC must send back the alert in order
    93 to perform a cross-check of the relevant data);
     94that the alert notice has been received (CC must send back the alert in order
     95to perform a cross-check of relevant data);
    9496\item the \textcolor{red}{\bf RED Alarm state} expires because of the
    9597missing of one or more of the needed criteria mentioned above;
     
    106108\subsection{GRB Archive and Emails to the GRB-mailing List}
    107109
    108 In case of alert -- even if it did not contain the necessary coordinates -- the
     110In case of alert -- even if it does not contain the necessary coordinates -- the
    109111information is  translated into ``human language'' and stored in ASCII files.
    110112At the same time, an e-mail is sent to the MAGIC GRB-mailing list
     
    136138Since July 15$^{\mathrm{th}}$, 2004, {\it gspot} has been working stably at La Palma.
    137139It received about 100 alerts from HETE-2 and INTEGRAL, out of which
    138 19 contained GRB's coordinates. Time delays to the onset of the burst
     14019 contained GRB coordinates. Time delays to the onset of the burst
    139141were of the order of several minutes to tens of minutes. The Burst Monitor can be considered stable
    140 since November 2004. Since then we have received the following four significant alerts:\\
     142since November 2004. Since that date we have received the following four significant alerts:\\
    141143
    142144\begin{tabular}{lllcccl}
     
    145147\end{tabular}
    146148
    147 In the first two cases the weather conditions at La Palma were bad. In the last two
    148 a couple of GRBs were detected within two hours by SWIFT. They were observable since
    149 their own onset and for all the following 5 hours. The weather was good, but unfortunately
    150 the Telescope was off-service because of the exceptional events occured in La Palma
    151 during the previous weeks.
     149It's a pitty that weather conditions at La Palma were bad.
    152150
    153151\subsection{Experience from SWIFT GRBs until now}
     
    166164\end{tabular}
    167165
     166In the first three alerts weather conditions in La Palma were bad. In the last two
     167a couple of GRBs were detected within two hours by SWIFT. They were observable since
     168their own onset and for all the following 5 hours. The weather was good, but unfortunately
     169the Telescope was off-service because of the exceptional events occured in La Palma
     170during the previous weeks.
     171
    168172\subsection{Comparison between the Satellite Orbits}
    169173
    170174Figure~\ref{fig:orbit} shows the orbits of the \sw, \he and \ig satellites.
    171 The \sw and \he satellites are situated in a circular orbit with
     175\sw and \he satellites are situated in a circular orbit with
    17217620.6$^\circ$ and 2$^\circ$ inclination, respectively.
    173 One revolution of the \sw and \he satellites last about 100\,min.
    174 The \ig satellite has a highly eccentric orbit with a revolution period of three sidereal days around the Earth.
     177One revolution of \sw and \he satellites lasts about 100\,min.
     178\ig satellite has a highly eccentric orbit with a revolution period of three sidereal days around the Earth.
    175179
    176180\par
    177181
    178 It is difficult to draw strong conclusions from the individual satellites' orbits.
    179 The orientation of the satellites' FoV is influenced by the scheduled targets.
     182It is difficult to draw strong conclusions from the individual satellite orbits.
     183The orientation of satellites FoV is influenced by the scheduled targets.
    180184However, \sw is the satellite with the largest inclination and overlaps mostly with the FoV of \ma.
    181 This increases the chance to receive {\bf Red Alarms} from this satellite.
     185This increases the chance to receive {\bf Red Alerts} from this satellite.
    182186
    183187\begin{figure}[htp]
    184188\centering
    185189\includegraphics[width=0.6\linewidth]{GCNsatellites.eps}
    186 \caption{Orbits of the \sw (top), \he (center) and \ig (bottom) satellites: The pointed lines
    187 show the orbit while the drawn lines show the horizon of the Sun. Here, a typical night at
    188 La Palma is shown. The \sw satellite passes over the Roque seven times each night.}
     190\caption{Orbits of \sw (top), \he (center) and \ig (bottom) satellites: dot lines
     191show the orbit while drawn lines show the horizon of the Sun. Here, a typical night at
     192La Palma is shown. \sw satellite passes over Roque seven times each night.}
    189193\label{fig:orbit}
    190194\end{figure}
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