论文信息 - Statistical relationship between CME speed and soft X-ray peak flux of the associated flare during solar cycle 23

Statistical relationship between CME speed and soft X-ray peak flux of the associated flare during solar cycle 23

Abstract The relationship between the speed of coronal mass ejections and the peak soft X-ray flux of the associated flares is studied for events occurring near the solar limbs between 1996 and 2008. An improved, though still moderate, correlation between the two parameters is found.

K. Klein | L. Taliashvili | C. Salas-Matamoros

[1] M. Temmer,et al. IMPULSIVE ACCELERATION OF CORONAL MASS EJECTIONS. II. RELATION TO SOFT X-RAY FLARES AND FILAMENT ERUPTIONS , 2012, 1206.2144.

[2] R. Jain,et al. X-ray emission characteristics of flares associated with CMEs , 2008 .

[3] B. Vršnak,et al. The CME-flare relationship: Are there really two types of CMEs? , 2005 .

[4] A. Hundhausen,et al. Role of projection effects on solar coronal mass ejection properties: 1. A study of CMEs associated with limb activity , 2004 .

[5] Haimin Wang,et al. RELATIONSHIP BETWEEN CME KINEMATICS AND FLARE STRENGTH , 2003 .

[6] Mark S. Giampapa,et al. Cosmic Winds and the Heliosphere , 1997 .

[7] H. Carmichael. in Physics of Solar Flares , 1964 .