Geoscience Reference
In-Depth Information
Fig. 5. In-flight observation of XRF off the standard sample during the active (X1) and
moderate (C3) solar conditions are shown with clear detection of major elements.
Fig. 6. Kepler's Supernova Remnant was observed on June 15, 2003. Emission lines of
Mg, Si, and S are clearly detected as expected.
off the standard sample under the active (X1) and moderate (C3) solar
conditions.
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Intensities of each XRF are enhanced, especially for heavier
elements. In the active case shows higher enhancement of Ca and Fe as
well as larger Si/Mg that is consistent for higher temperature flare events.
Figure 6 shows cosmic X-rays from Kepler's Supernova Remnant.
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Emis-
sion line of Mg, Si, and S are clearly detected as expected.
