WANG Xueyi, WU Jingsheng, LI Yi, WANG Shui, ZHAO Jikuen, CAO Jinbin. ALFVEN WWES IN THE MAGNETIC RECONNECTION REGIONS AND THE ACCELERATION OF NEWBORN IONS[J]. Chinese Journal of Space Science, 2001, 21(3): 208-218.
Citation:
WANG Xueyi, WU Jingsheng, LI Yi, WANG Shui, ZHAO Jikuen, CAO Jinbin. ALFVEN WWES IN THE MAGNETIC RECONNECTION REGIONS AND THE ACCELERATION OF NEWBORN IONS[J]. Chinese Journal of Space Science, 2001, 21(3): 208-218.
WANG Xueyi, WU Jingsheng, LI Yi, WANG Shui, ZHAO Jikuen, CAO Jinbin. ALFVEN WWES IN THE MAGNETIC RECONNECTION REGIONS AND THE ACCELERATION OF NEWBORN IONS[J]. Chinese Journal of Space Science, 2001, 21(3): 208-218.
Citation:
WANG Xueyi, WU Jingsheng, LI Yi, WANG Shui, ZHAO Jikuen, CAO Jinbin. ALFVEN WWES IN THE MAGNETIC RECONNECTION REGIONS AND THE ACCELERATION OF NEWBORN IONS[J]. Chinese Journal of Space Science, 2001, 21(3): 208-218.
By means of 2D-hybrid simulation code, magnetic driven reconnection in the low plasma β case. Results show that the Alfven waves can be produced in the magnetic reconnection process. The newborn ions can be pitch angle scattered by Alfven waves and have the shell distribution. Some newborn ions are accelerated and the maximum energy is about 4miVA02/2. The acceleration takes about 100/Ωi and is thus extremely rapidly acceleration process.