<h2> Giotto Magnetometer (MAG) data at AMDA </h2>

Source: <a href="ftp://psa.esac.esa.int/pub/mirror/GIOTTO/MAG/" TARGET=_BLANK>ESA PSA</a><br/><br/>
<b> Principal Investigator(s): F.M. Neubauer (University of Cologne, Germany)</b><br/><br/>

<i>Please acknowledge the above Principal Investigator(s) 
as well as the European Space Agency when making a publication using the data.</i><br/><br/>
 
 <ul>
 <li>
 The Halley centered coordinate (CSE) system used   
 in these measurements is a right handed coordinate system.   
 It is defined   
 so that the coordinate system has its origin at the comet's nucleus, with    
 the XSE-axis from the nucleus to the sun, the YSE-axis parallel to the       
 ecliptic plane in the direction of retrograde planetary motion.   
 The ZSE- axis completes the coordinate system such that at the time of Halley's       
 passage through the ecliptic plane it points to the ecliptic north.
<li>Azimuthal B angle is counted positive from the X-axis toward the Y-axis.
<li>Elevation B angle is counted from ecliptic plane toward positive Z.
<li>B RMS is a pythagorean meean of the component RMS values
</ul>
<br/>
Experiment <a href="ftp://psa.esac.esa.int/pub/mirror/GIOTTO/MAG/GIO-C-MAG-4-RDR-8SEC-HALLEY-V1.0/CATALOG/INST.CAT" TARGET=_BLANK</a>full description</a>