Dept. of Math. Jadavpur Univ. Kolkata India;
astrophysical plasma; chromosphere; solar corona; solar magnetism; solar wind; 13th order complex polynomial dispersion equation; alpha-particles; collisional plasma; collisionless plasma; collisionless solar polar coronal hole; electron velocity; electron-ion interaction; electrons; extended energy deposition scenario; fast solar wind acceleration; magnetic flux density; maximum wave electric field; minor ion energy gain; photosphere; protons; solar radius; stochastic instability; three-fluid Maxwell model; transition point; wave frequency; Abstracts; Acceleration; Charge carrier processes; Educational institutions; Mathematical model;
机译:周期23下降阶段太阳风离子组成及其源冠孔的时间演变I.极冠孔的低纬度扩展
机译:使用极冠孔面积测量来确定太阳周期24中太阳极磁场的反转
机译:太阳极日冕孔中正离子的能量增益
机译:挖掘机太阳能极冠孔的扩展能量沉积场景
机译:重新连接驱动的太阳能冠状孔喷气机的室内结构,动力学和螺旋体影响
机译:ACE和STEREO卫星在黄道上测得的高速太阳风的峰值速度对其太阳源日冕孔的面积和共度的依赖性
机译:阿尔芬波在极地冠状孔中消散能量的观测量化:波浪驱动快速太阳风的证据。