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<p>(XRF) of crystal compounds created through the interaction of the electron shell with the solar wind particles to measure the abundance of the three main components: <a href="page.php?w=magnesium">magnesium</a>, <a href="page.php?w=silicon">silicon</a> and <a href="page.php?w=aluminium">aluminium</a>. The detection of <a href="page.php?w=iron">iron</a>, <a href="page.php?w=calcium">calcium</a> and <a href="page.php?w=titanium">titanium</a> depended on the solar activity. The detection range for X-rays was 0.5 to 10 keV. The spectrometer and XSM</p><p>
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