ION-CYCLOTRON-RESONANCE HEATING MECHANISM OF THE HELY IONS IN LOWER SOLAR POLAR CORONA

SHU Chuanzheng; CHEN Fei; TU Chuanyi

doi:10.11728/cjss2001.03.20010301

Volume 21 Issue 3

Aug. 2001

Turn off MathJax

Article Contents

Article Navigation > Chinese Journal of Space Science > 2001 > 21(3): 193-199

SHU Chuanzheng, CHEN Fei, TU Chuanyi. ION-CYCLOTRON-RESONANCE HEATING MECHANISM OF THE HELY IONS IN LOWER SOLAR POLAR CORONA[J]. Chinese Journal of Space Science, 2001, 21(3): 193-199. doi: 10.11728/cjss2001.03.20010301

Citation:

SHU Chuanzheng, CHEN Fei, TU Chuanyi. ION-CYCLOTRON-RESONANCE HEATING MECHANISM OF THE HELY IONS IN LOWER SOLAR POLAR CORONA[J]. Chinese Journal of Space Science, 2001, 21(3): 193-199. doi: 10.11728/cjss2001.03.20010301

Citation:

PDF( 442 KB)

ION-CYCLOTRON-RESONANCE HEATING MECHANISM OF THE HELY IONS IN LOWER SOLAR POLAR CORONA

doi: 10.11728/cjss2001.03.20010301 cstr: 32142.14.cjss2001.03.20010301

Department of Geophysics, Peking University, Beijing 100871

Received Date: 2000-12-25
Rev Recd Date: 2001-05-08

Abstract

Abstract

In this paper, the four-fluid model, and replace O⁵⁺ with one of Fe¹¹⁺, Mg⁹⁺, Mg⁷⁺, Ne⁷⁺, Si⁷⁺ ions respectively are adopted. The bulk velocity and temperature of the heavy ions are obtained, and compared with the SUMER observation data.
- Solar coronal hole,
- Heating of heavy ions