Young, C. Alex

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  1. Gilbert H, Inglis A, Mays M, Ofman L, Thompson B, Young C. ENERGY RELEASE FROM IMPACTING PROMINENCE MATERIAL FOLLOWING THE 2011 JUNE 7 ERUPTION. Astrophys. J. Lett. 2013;776 (1):6.
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  2. Ryan D, Milligan R, Gallagher P, Dennis B, Tolbert A, Schwartz R, Young C. THE THERMAL PROPERTIES OF SOLAR FLARES OVER THREE SOLAR CYCLES USING GOES X-RAY OBSERVATIONS. Astrophys. J. Suppl. Ser. 2012;202 (2):15.
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  3. Gallagher P, Young C, Byrne J, McAteer R. CORONAL MASS EJECTION DETECTION USING WAVELETS, CURVELETS AND RIDGELETS: APPLICATIONS FOR SPACE WEATHER MONITORING. Advances in Space Research. 2011;47 (12):2118-2126.
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  4. Ireland J, Marsh M, Kucera T, Young C. AUTOMATED DETECTION OF OSCILLATING REGIONS IN THE SOLAR ATMOSPHERE. Sol. Phys. 2010;264 (2):403-431.
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  5. Milligan R, McAteer R, Dennis B, Young C. EVIDENCE OF A PLASMOID-LOOPTOP INTERACTION AND MAGNETIC INFLOWS DURING A SOLAR FLARE/CORONAL MASS EJECTION ERUPTIVE EVENT. Astrophys. J. 2010;713 (2):1292-1300.
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  6. Byrne J, Gallagher P, McAteer R, Young C. KINEMATICS OF CORONAL MASS EJECTIONS USING MULTISCALE METHODS. Astron. Astrophys. 2009;495 (1):325-334.
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  7. Conlon P, Gallagher P, McAteer R, Ireland J, Young C, Kestener P, Hewett R, Maguire K. MULTIFRACTAL PROPERTIES OF EVOLVING ACTIVE REGIONS. In: Solar Image Analysis and Visualization. 2009.
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  8. Conlon P, Gallagher P, McAteer R, Ireland J, Young C, Kestener P, Hewett R, Maguire K. MULTIFRACTAL PROPERTIES OF EVOLVING ACTIVE REGIONS. Sol. Phys. 2008;248 (2):297-309.
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  9. Ireland J, Young C, McAteer R, Whelan C, Hewett R, Gallagher P. MULTIRESOLUTION ANALYSIS OF ACTIVE REGION MAGNETIC STRUCTURE AND ITS CORRELATION WITH THE MOUNT WILSON CLASSIFICATION AND FLARING ACTIVITY. Sol. Phys. 2008;252 (1):121-137.
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  10. Young C, Gallagher P. MULTISCALE EDGE DETECTION IN THE CORONA. In: SOLAR PHYSICS. 3rd Solar Image Processing Workshop; SEP, 2006; Dublin, ISRAEL. 2008. p. 457-469.
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  11. McAteer R, Young C, Ireland J, Gallagher P. BURSTY NATURE OF SOLAR FLARE X-RAY EMISSION. Astrophys. J. 2007;662 (1):691-700.
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