Abstract
Solar X-ray observations in the >20 keV range are discussed, with emphasis on their implications for electron acceleration. It is shown how measurements of fine time structure, directivity, and the production height of X-radiation may be interpreted in the contexts of thermal and non-thermal electron populations. Recent measurements are reviewed, and the expected contribution of Ulysses is discussed.
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Hurley, K. (1986). Stereoscopic Measurements of Hard Solar X-Rays, and Related Topics. In: Marsden, R.G. (eds) The Sun and the Heliosphere in Three Dimensions. Astrophysics and Space Science Library, vol 123. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4612-5_9
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DOI: https://doi.org/10.1007/978-94-009-4612-5_9
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