NEW OBSERVATIONS OF THE SOLAR 0.5โ5 KEV SOFT X-RAY SPECTRUM
NEW OBSERVATIONS OF THE SOLAR 0.5โ5 KEV SOFT X-RAY SPECTRUM
The solar corona is orders of magnitude hotter than the underlying photosphere, but how the corona attains such high temperatures is still not understood. Soft X-ray (SXR) emission provides important diagnostics for thermal processes in the high-temperature corona, and is also an important driver of ionospheric dynamics at Earth. There โฆ