| Journal of astrophysics and astronomy | |
| Observational Study of Solar Magnetic Active Phenomena | |
| Hongqi Zhang11  | |
| [1] National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100 012, China.$$ | |
| 关键词: Sun: activity; flares; magnetic fields.; | |
| DOI : | |
| 学科分类:天文学(综合) | |
| 来源: Indian Academy of Sciences | |
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【 摘 要 】
The electric current separated into two parts reflected the quantative properties of heterogeneity and chirality of magnetic field, and defined them as the shear and twist components of current. We analyze the basic configuration and evolution of superactive region NOAA 6580-6619-6659.It is found that the contribution of the twist component of current cannot be reflected in the normal analysis of the magnetic shear and gradient of the active regions. The observational evidence of kink magnetic ropes generated from the subatmosphere cannot be found completely in some super delta active regions.
【 授权许可】
Unknown
【 预 览 】
| Files | Size | Format | View |
|---|---|---|---|
| RO201912040493418ZK.pdf | 1366KB |
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