Abstract
ON December 17, 1964, at 03 h 35 m U.T. the firing of the second, three-axis stabilized Skylark research rocket occurred at Woomera. It carried an X-ray pinhole camera, a second version of the apparatus which produced the soft X-ray image of the Sun discussed in an earlier communication1. Part of the negative obtained from this flight is reproduced in Fig. 1. Table 1 gives details of the filters and the pinholes used to obtain these images.
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References
Russell, P. C., Nature, 205, 684 (1965).
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RUSSELL, P. Further Soft X-ray Images of the Sun. Nature 206, 281–282 (1965). https://doi.org/10.1038/206281a0
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DOI: https://doi.org/10.1038/206281a0
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