Flow Sources and Formation Laws of Solar Wind Streams

N.A. Lotova; V.N. Obridko; K.V. Vladimirskii; M.K. Bird; P. Janardhan

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Flow Sources and Formation Laws of Solar Wind Streams

机译：太阳风的流源和形成规律

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The large-scale stream structure of the solar wind flow is studied in the main acceleration zone from 10 to 40 solar radii from the Sun. Three independent sets of experimental data were used: radio astronomical observations of radio wave scattering using the large radio telescopes of the Lebedev Physical Institute; dual-frequency Doppler solar wind speed measurements from the Ulysses Solar Corona Experiment during the spacecraft's two solar conjunctions in summer 1991 and winter 1995; solar magnetic field strength and configuration computed from Wilcox Solar Observatory data. Both the experimental data on the position of the transonic region of the solar wind flow and the solar wind speed estimates were used as parameters reflecting the intensity of the solar wind acceleration process. Correlation studies of these data with the magnetic field strength in the solar corona revealed several types of solar wind flow differing in their velocities and the location of their primary acceleration region.

机译：在太阳从10到40的太阳半径的主要加速区中研究了太阳风的大尺度流结构。使用了三组独立的实验数据：使用列别捷夫物理研究所的大型射电望远镜进行的无线电波散射的射电天文观测； 1991年夏季和1995年冬季，在航天器的两次太阳活动期间，通过尤利西斯太阳电晕实验获得的双频多普勒太阳风速测量结果；根据Wilcox太阳观测站的数据计算得出的太阳磁场强度和结构。关于太阳风流的跨音速区域的位置的实验数据和太阳风速估计都用作反映太阳风加速过程强度的参数。这些数据与日冕中磁场强度的相关性研究表明，几种类型的太阳风流的速度和主要加速区域的位置不同。

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《Solar Physics》 |2002年第1期|149-163|共15页
作者
N.A. Lotova; V.N. Obridko; K.V. Vladimirskii; M.K. Bird; P. Janardhan;
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IZMIRAN;

IZMIRAN;

Lebedev Physical Institute;

Radioastronom. Institute University of Bonn;

Radioastronom. Institute University of Bonn;

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2. Diagnostics of solar wind streams and their sources in the solar corona [J] . Lotova N.A., Vladimirskii K.V., Obridko V.N. Geomagnetism and aeronomy . 2010,第6期

机译：太阳日冕中太阳风流及其来源的诊断
3. Solar Wind Sources in the Late Declining Phase of Cycle 23: Effects of the Weak Solar Polar Field on High Speed Streams [J] . J. G. Luhmann, C. O. Lee, Yan Li, Solar Physics . 2009,第1a2期

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5. Development of steady-state solar polar plume models in one and two dimensions to investigate solar wind sources. [D] . Peng, Beidi. 2008

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7. Solar Wind Sources in the Late Declining Phase of Cycle 23: Effects of the Weak Solar Polar Field on High Speed Streams [O] . 2009

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8. Solar Wind Sources in the Late Declining Phase of Cycle 23: Effects of the Weak Solar Polar Field on High Speed Streams [R] . Luhmann, J. G., Lee, C. O., Li, Y., 2009

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Flow Sources and Formation Laws of Solar Wind Streams

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