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On the time evolution of brightness, volume and height of a coronal source in an M-class flare 期刊论文
ASTROPHYSICS AND SPACE SCIENCE, 2017, 卷号: 362, 期号: 6, 页码: 10
Authors:  Firoz, Kazi A.;  Gan, W. Q.;  Li, Y. P.;  Rodriguez-Pacheco, J.;  Su, Y.
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Solar flares  Area/volume of the flare  Volume and mean intensity  Heights of the coronal sources  Total Thermal electrons in high-temperature plasma in the corona  contribution into the flare process  Adiabatic expansion  Theoretical model for thermal source  RHESSI X-ray  GOES X-ray  SDO/AIA images  Spatial and temporal evolution of the coronal source  RHESSI image reconstruction algorithm  
AN INTERPRETATION OF GLE71 CONCURRENT CME-DRIVEN SHOCK WAVE 期刊论文
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2014, 卷号: 213, 期号: 2, 页码: 0
Authors:  Firoz, Kazi A.;  Zhang, Q. M.;  Gan, W. Q.;  Li, Y. P.;  Rodriguez-Pacheco, J.;  Moon, Y. -J.;  Kudela, K.;  Park, Y. -D.;  Dorman, Lev I.
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Sun: Corona  Sun: Coronal Mass Ejections (Cmes)  Sun: Evolution  Sun: Flares  Sun: Heliosphere  Sun: Particle Emission  
On the possible mechanism of the first ground level enhancement in cosmic ray intensity of solar cycle 24 期刊论文
ASTROPHYSICS AND SPACE SCIENCE, 2014, 卷号: 350, 期号: 1, 页码: 21-32
Authors:  Firoz, Kazi A.;  Gan, W. Q.;  Li, Y. P.;  Rodriguez-Pacheco, J.
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Cosmic Rays  Ground Level Enhancement  Solar Flare  Cme-driven Shock  Solar Radio Burst  Solar Flux Density  Relativistic Energy  Particle Release Time