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- W2488392778 abstract "Abstract A solar coronal loop system has been photographed in soft X-rays using a normal incidence telescope based on multilayer mirror technology. The telescope consisted of a spherical objective mirror of 4 cm aperture and 1 m focal length, a film cassette, and a focal plane shutter. A metallized thin plastic film filter was used to exclude visible light. The objective mirror was covered with a multilayer coating consisting of alternating layers of tungsten and carbon whose combined thicknesses satisfied the Bragg diffraction condition for 44 Å radiation. The image was recorded during a rocket flight on 1985 October 25, and was dominated by emission lines arising from the Si XII spectrum. The rocket also carried a high resolution soft X-ray spectrograph that confirmed the presence of Si XII line radiation in the source. This image represents the first successful use of multilayer technology for astrophysical observations." @default.
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- W2488392778 date "1988-01-01" @default.
- W2488392778 modified "2023-09-27" @default.
- W2488392778 title "Soft X-Ray Images of the Solar Corona Using Normal Incidence Optics" @default.
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- W2488392778 doi "https://doi.org/10.1017/s0252921100107559" @default.
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