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Solar plasma temperature diagnostics in flares and active regions from spectral lines in the range 280–330 Å in the SPIRIT/CORONAS-F experiment

✍ Scribed by S. V. Shestov; S. V. Kuzin; A. M. Urnov; A. S. Ul’yanov; S. A. Bogachev

No coin nor oath required. For personal study only.

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