FORMATION OF SOLAR MAGNETIC FLUX TUBES WITH KILOGAUSS FIELD STRENGTH INDUCED BY CONVECTIVE INSTABILITY

Shinichi Nagatal; Saku Tsuneta; Yoshinori Suematsu; Kiyoshi Ichimoto; Yukio Katsukawa; Toshifumi Shimizu; Takaaki Yokoyama; Theodore D. Tarbell; Bruce W. Lites; Richard A. Shine; Thomas E. Berger; Alan M. Title; Luis R. Bellot Rubio; David Orozco Suarez

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FORMATION OF SOLAR MAGNETIC FLUX TUBES WITH KILOGAUSS FIELD STRENGTH INDUCED BY CONVECTIVE INSTABILITY

机译：对流不稳定性引起的具有KILOGAUSS场强的太阳磁通管的形成

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Convective instability has been a mechanism used to explain the formation of solar photospheric flux tubes with kG field strength. However, the turbulence of the Earth's atmosphere has prevented ground-based observers from examining the hypothesis with pr

机译：对流不稳定性一直是用来解释具有kG场强的太阳光球通量管形成的机制。但是，地球大气层的湍流使地面观测者无法通过pr检验假设

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《The Astrophysical journal》 |2008年第2期|p.145-147|共3页
作者
Shinichi Nagatal; Saku Tsuneta; Yoshinori Suematsu; Kiyoshi Ichimoto; Yukio Katsukawa; Toshifumi Shimizu; Takaaki Yokoyama; Theodore D. Tarbell; Bruce W. Lites; Richard A. Shine; Thomas E. Berger; Alan M. Title; Luis R. Bellot Rubio; David Orozco Suarez;
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Hida Observatory, Kyoto University, Takayama, Gifu 506-1314, Japan;

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正文语种 eng
中图分类天文学;
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1. FORMATION OF SOLAR MAGNETIC FLUX TUBES WITH KILOGAUSS FIELD STRENGTH INDUCED BY CONVECTIVE INSTABILITY [J] . Shinichi Nagatal, Saku Tsuneta, Yoshinori Suematsu, The Astrophysical journal . 2008,第2pa2期

机译：对流不稳定性引起的具有KILOGAUSS场强的太阳磁通管的形成
2. Thermal Relaxation of Very Small Solar Magnetic Structures in Intergranules: A Process That Produces Kilogauss Magnetic Field Strengths [J] . J. Sánchez Almeida1 The Astrophysical journal . 2008,第2期

机译：晶格间非常小的太阳磁结构的热弛豫：产生Kilogauss磁场强度的过程
3. Comparing Simulations of Rising Flux Tubes Through the Solar Convection Zone with Observations of Solar Active Regions: Constraining the Dynamo Field Strength [J] . M. A. Weber, Y. Fan, M. S. Miesch Solar Physics . 2013,第1a2期

机译：穿过太阳对流区的上升通量管的模拟与太阳活动区的观察结果的比较：约束发电机的场强
4. P-mode induced convective collapse in vertical expanding magnetic flux tubes? [C] . D. Utz, T. Van Doorsselaere, N. Magyar, International Astronomical Union., Symposium . 2017

机译：P模式诱导垂直膨胀磁通管中的对流塌陷？
5. The dynamic evolution of active-region-scale magnetic flux tubes in the turbulent solar convective envelope. [D] . Weber, Maria Ann. 2014

机译：湍流太阳对流包层中有源区尺度磁通管的动态演化。
6. Low geomagnetic field strength during End-Cretaceous Deccan volcanism and whole mantle convection [O] . Radhakrishna T., Asanulla R. Mohamed, Venkateshwarlu M., -1

机译：白垩纪末癸火山活动和整个地幔对流过程中地磁场强度低
7. Comparing Simulations of Rising Flux Tubes Through the Solar Convection Zone with Observations of Solar Active Regions: Constraining the Dynamo Field Strength [O] . M. A. Weber, C Springer 2016

机译：通过太阳对流区对太阳活动区上升通量管的模拟比较：抑制发电场强度

FORMATION OF SOLAR MAGNETIC FLUX TUBES WITH KILOGAUSS FIELD STRENGTH INDUCED BY CONVECTIVE INSTABILITY

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