SUNSPOTS AND VELOCITY-FIELD EVOLUTION IN THE HIGH SOLAR PHOTOSPHERE

被引：0

作者：

BOTTON, C ^{[1
]}

ROBILLOT, JM ^{[1
]}

机构：

[1] OBSERV BORDEAUX 1, F-33270 FLOIRAC, FRANCE

来源：

COMPTES RENDUS DE L ACADEMIE DES SCIENCES SERIE II | 1995年 / 320卷 / 07期

关键词：

D O I：

暂无

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

The comparison of solar photosphere velocity-fields with the day-by-day evolutions of sun spots reveals following phenomenn: the active centers (sun-spots and facular regions) are generally associated with up-draft areas, but sun-spot evolution (change of shape, scission and bursting into several spots) corresponds to areas of downward flow or at the boundary of upflow and downflow. A study for twelve cases suggests a systematic effect.

引用

页码：359 / 363

页数：5