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<oembed><version>1.0</version><provider_name>Norwegian Centre for Space Weather (NOSWE)</provider_name><provider_url>https://site.uit.no/spaceweather</provider_url><author_name>Norwegian Centre for Space Weather (NOSWE)</author_name><author_url>https://site.uit.no/spaceweather</author_url><title>Xray Flux - Norwegian Centre for Space Weather (NOSWE)</title><type>rich</type><width>600</width><height>338</height><html>&lt;blockquote class="wp-embedded-content" data-secret="DHMA1RGhQZ"&gt;&lt;a href="https://site.uit.no/spaceweather/xray-flux/"&gt;Xray Flux&lt;/a&gt;&lt;/blockquote&gt;&lt;iframe sandbox="allow-scripts" security="restricted" src="https://site.uit.no/spaceweather/xray-flux/embed/#?secret=DHMA1RGhQZ" width="600" height="338" title="&#x201C;Xray Flux&#x201D; &#x2014; Norwegian Centre for Space Weather (NOSWE)" data-secret="DHMA1RGhQZ" frameborder="0" marginwidth="0" marginheight="0" scrolling="no" class="wp-embedded-content"&gt;&lt;/iframe&gt;&lt;script&gt;
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</html><description>Xrays The observed solar X-rays are a result of solar activity and solar flares. Solar flares are intense emissions of electromagnetic radiation from active regions on the Sun. Solar flares, especially larger flares, can be accompanied by coronal mass ejections (CMEs) and Solar Proton Events (SPEs). The increased X-ray flux &#x2026;</description></oembed>
