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pro vyhledávání: '"Kayat, M"'
Autor:
Gabriel, A, Acton, L, Culhane, J, Phillips, K, Wolfson, C, Rapley, C, Antonucci, E, Bentley, R, Jordan, C, Kayat, M, Leibacher, J, Levay, M, Sherman, J, Strong, K, Veck, N
Soft X-ray observations of the limb event on 1980 April 30 are summarized. These consist of maps made with the Flat Crystal Spectrometer and calcium and iron spectra obtained with the Bent Crystal Spectrometer. The physical conditions, e.g., temperat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ea2551de5ad8c831faa13b0ed08a34d0
https://ora.ox.ac.uk/objects/uuid:b7e90fc9-e2c7-47ab-b105-50f162d4ee70
https://ora.ox.ac.uk/objects/uuid:b7e90fc9-e2c7-47ab-b105-50f162d4ee70
Autor:
Culhane, J, Gabriel, A, Acton, L, Rapley, C, Phillips, K, Wolfson, C, Antonucci, E, Bentley, R, Catura, R, Jordan, C, Kayat, M, Kent, B, Leibacher, J, Parmar, A, Sherman, J, Springer, L, Strong, K, Veck, N
Preliminary results obtained for three solar flares with the bent crystal spectrometer on the SMM are presented. Resonance and satellite lines of Ca XIX and XVIII and Fe XXV and XXIV are observed together with the Fe XXVI Lyman-alpha line. Plasma pro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f14310416c494d37a02a387d61878925
https://doi.org/10.1086/183499
https://doi.org/10.1086/183499
Autor:
Acton, L, Culhane, J, Gabriel, A, Wolfson, C, Rapley, C, Phillips, K, Antonucci, E, Bentley, R, Hayes, R, Joki, E, Jordan, C, Kayat, M, Kent, B, Leibacher, J, Nobles, R, Parmar, A, Strong, K, Veck, N
Publikováno v:
ASTROPHYSICAL JOURNAL. 244(3)
Preliminary results of spectroscopy and imaging of a solar active region and flare plasma in soft X-ray emission lines are presented. Observed X-ray line widths in a nonflaring active region are broader than the Doppler width corresponding to the loc
Akademický článek
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Akademický článek
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Autor:
Kayat, Michael Anthony
Supernovae and supernova remnants (SNR) are probably important energy sources in the interstellar medium (ISM) and an understanding of the intermediate and advanced stages of SNR evolution are particularly essential. This thesis describes, first a br
Externí odkaz:
http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.259237