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COMPARISON OF OBSERVED CA XIX AND CA XVIII RELATIVE LINE INTENSITIES WITH THEORYJORDAN C; VECK NJ.1982; SOL. PHYS.; ISSN 0038-0938; NLD; DA. 1982; VOL. 78; NO 1; PP. 125-135; BIBL. 1 P.Article

SOLAR ABUNDANCES FROM X-RAY FLARE OBSERVATIONSVECK NJ; PARKINSON JH.1981; MON. NOT. R. ASTRON. SOC.; ISSN 0035-8711; GBR; DA. 1981; VOL. 197; NO 1; PP. 41-55; BIBL. 25 REF.Article

AN INVESTIGATION OF THE 1.9 A FEATURE IN SOLARFLARE X-RAY SPECTRAPARKINSON JH; VECK NJ; ASHFIELD MEC et al.1979; ASTROPHYS. J.; USA; DA. 1979; VOL. 231; NO 2 PART. 1; PP. 551-556; BIBL. 21 REF.Article

OBSERVATIONS OF THE LIMB SOLAR FLARE ON 1980 APRIL 30 WITH THE SMM X-RAY POLYCHROMATORGABRIEL AH; ACTON LW; CULHANE JL et al.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 244; NO 3; PART. 2; PP. L147-L151; H.T. 1; BIBL. 11 REF.Article

X-RAY LINE WIDTHS AND CORONAL HEATINGACTON LW; CULHANE JL; GABRIEL AH et al.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 244; NO 3; PART. 2; PP. L137-L140; H.T. 1; BIBL. 20 REF.Article

X-RAY SPECTRA OF SOLAR FLARES OBTAINED WITH A HIGH-RESOLUTION BENT CRYSTAL SPECTROMETERCULHANE JL; GABRIEL AH; ACTON LW et al.1981; ASTROPHYS. J.; ISSN 0004-637X; USA; DA. 1981; VOL. 244; NO 3; PART. 2; PP. L141-L145; BIBL. 24 REF.Article

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