HELIOSPHERIC IMAGES OF THE SOLAR WIND AT EARTH

N. R. Sheeley Jr.; A. D. Herbst; C. A. Palatchi; Y.-M. Wang; R. A. Howard; J. D. Moses; A. Vourlidas; J. S. Newmark; D. G. Socker; S. P. Plunkett; C. M. Korendyke; L. F. Burlaga; J. M. Davila; W. T. Thompson; O. C. St Cyr; R. A. Harrison; C. J. Davis

首页> 外文期刊>The Astrophysical journal >HELIOSPHERIC IMAGES OF THE SOLAR WIND AT EARTH

【24h】

HELIOSPHERIC IMAGES OF THE SOLAR WIND AT EARTH

机译：太阳风的地球球面影像

获取原文

获取原文并翻译 | 示例

掌桥外文数据库（机构版） >>

开具论文收录证明 >>

文献代查 >>

页面导航

摘要
著录项
相似文献
相关主题

摘要

During relatively quiet solar conditions throughout the spring and summer of 2007, the SECCHI HI2 white-light telescope on the STEREO B solar-orbiting spacecraft observed a succession of wave fronts sweeping past Earth. We have compared these heliospheric images with in situ plasma and magnetic field measurements obtained by near-Earth spacecraft, and we have found a near perfect association between the occurrence of these waves and the arrival of density enhancements at the leading edges of high-speed solar wind streams. Virtually all of the strong corotating interaction regions are accompanied by large-scale waves, and the low-density regions between them lack such waves. Because the Sun was dominated by long-lived coronal holes and recurrent solar wind streams during this interval, there is little doubt that we have been observing the compression regions that are formed at low latitude as solar rotation causes the high-speed wind from coronal holes to run into lower speed wind ahead of it.

机译：在2007年春季和夏季相对安静的太阳条件下，STEREO B太阳轨道航天器上的SECCHI HI2白光望远镜观测到一系列波阵面掠过地球。我们将这些日球图像与近地航天器获得的原位等离子体和磁场测量值进行了比较，并且我们发现了这些波的出现与高速太阳前缘密度增强的到达之间的近乎完美的联系。风。几乎所有的强同向相互作用区域都伴随着大范围的波浪，而它们之间的低密度区域则没有这种波浪。因为在此间隔期间，太阳由长寿命冠冕孔和反复出现的太阳风所控制，所以毫无疑问，我们一直在观察低纬度形成的压缩区域，因为太阳旋转会导致冠冕孔产生高速风在它前面遇到低速风。

著录项

来源
《The Astrophysical journal》 |2008年第1期|p.853-862|共10页
作者
N. R. Sheeley Jr.; A. D. Herbst; C. A. Palatchi; Y.-M. Wang; R. A. Howard; J. D. Moses; A. Vourlidas; J. S. Newmark; D. G. Socker; S. P. Plunkett; C. M. Korendyke; L. F. Burlaga; J. M. Davila; W. T. Thompson; O. C. St Cyr; R. A. Harrison; C. J. Davis;
展开▼
作者单位

展开▼
收录信息
原文格式 PDF
正文语种 eng
中图分类天文学;
关键词

相似文献

外文文献
中文文献
专利

1. Predicting the arrival of high-speed solar wind streams at Earth using the STEREO heliospheric imagers [J] . C. J. Davis, J. A. Davies, M. J. Owens, Space Weather . 2012,第2期

机译：使用STEREO日球成像仪预测高速太阳风在地球上的到达
2. HELIOSPHERIC IMAGES OF THE SOLAR WIND AT EARTH [J] . N. R. Sheeley Jr., A. D. Herbst, C. A. Palatchi, The Astrophysical journal . 2008,第1Pa1期

机译：太阳风的地球球面影像
3. Extracting inner-heliosphere solar wind speed information from heliospheric imager observations [J] . Barnard L. A., Owens M. J., Scott C. J., Space Weather . 2019,第6期

机译：从日球成像仪观测中提取太阳内层风速信息
4. Stray Light Analysis and Testing of the SoloHI (Solar Orbiter Heliospheric Imager) and WISPR (Wide Field Imager for Solar Probe) Heliospheric Imagers [C] . Arnaud F. R. Themisien, Russell A. Howard, Clarence Korendyke, SPIE Astronomical Telescopes + Instrumentation Conference . 2018

机译：SoloHI（太阳轨道宽视场成像仪）和WISPR（太阳探头的宽场成像仪）太阳系成像仪的杂散光分析和测试
5. Heliospheric x-rays due to solar wind charge exchange. [D] . Robertson, Ina Piket. 2003

机译：由于太阳风电荷交换而产生的日光X射线。
6. Modeling observations of solar coronal mass ejections with heliospheric imagers verified with the Heliophysics System Observatory [O] . C. Möstl, A. Isavnin, P. D. Boakes, -1

机译：由日光物理学系统天文台验证的日冕层成像仪对太阳日冕物质抛射的模拟观测
7. Predicting the arrival of high-speed solar wind streams at Earth using the STEREO Heliospheric Imagers [O] . Davis Chris J., Davies J. A., Owens Matt, 2012

机译：使用STEREO日球成像仪预测高速太阳风在地球上的到达
8. Analysis of Supergranule Sizes and Velocities Using Solar Dynamics Observatory (SDO)/Helioseismic Magnetic Imager (HMI) and Solar and Heliospheric Observatory (SOHO)/Michelson Doppler Imager (MDI) Dopplergrams. [R] . Williams, P. E., Pesnell, W. D., Beck, J. G., 2013

机译：使用太阳动力学观测台（sDO）/地震磁成像仪（HmI）和太阳和日光层观测台（sOHO）/迈克尔逊多普勒成像仪（mDI）多普勒图分析超粒径和速度。

HELIOSPHERIC IMAGES OF THE SOLAR WIND AT EARTH

摘要

著录项

相似文献

相关主题

期刊订阅