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首页> 外文期刊>Space Science Reviews >ULYSSES OBSERVATIONS OF A CORONAL ORIGIN PARTICLE EVENT AT 32-DEGREES SOUTH HELIOGRAPHIC LATITUDE
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ULYSSES OBSERVATIONS OF A CORONAL ORIGIN PARTICLE EVENT AT 32-DEGREES SOUTH HELIOGRAPHIC LATITUDE

机译:南斜度32度冠状起源颗粒事件的尤利西斯观测

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摘要

A remarkable streaming beam-like particle event of 60 keV-5 MeV ions and of 38-315 keV electrons has been reported previously. This event has been associated with the passage of a Coronal Mass Ejection (CME) over the Ulysses spacecraft on June 9-13, 1993. At this time, the spacecraft was located at 4.6 BU from the sun and at an heliolatitude of 32 degrees south. It was proposed (Armstrong et al., 1994) that the particle injection source could have been of coronal origin. In this study, we analyse the solar activity during this period. We identify a region of solar radio noise storms in the corona and in particular, a flare on June 7 that presents all the required characteristics to produce the hot plasma beam observed in the interplanetary medium. [References: 11]
机译:先前已报道了60 keV-5 MeV离子和38-315 keV电子的显着流束状粒子事件。此事件与1993年6月9日至13日在尤利西斯号航天器上进行日冕物质抛射(CME)有关。此时,该航天器位于距太阳4.6 BU处,向南32度。有人提出(Armstrong等,1994),粒子注入源可能是冠状的。在这项研究中,我们分析了这段时期的太阳活动。我们确定了日冕中的太阳无线电噪声风暴区域,尤其是6月7日的耀斑,该耀斑具有产生在行星际介质中观察到的热等离子体束所需的所有必要特性。 [参考:11]

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