Energetic proton observations at 1 and 5 AU 2. Rising phase of the solar cycle 23

Lario D.; Sanderson TR.; Maksimovic M.; Sanahuja B.; Plunkett SP.; Balogh A.; Forsyth RJ.; Lin RP.; Gosling JT.; Marsden RG.

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Energetic proton observations at 1 and 5 AU 2. Rising phase of the solar cycle 23

机译：在1和5 AU 2处的高能质子观测。太阳周期的上升阶段23

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The increasing level of solar activity at the end of 1997 coincides with the observation of solar energetic particle (SEP) events by the Wind and Ulysses spacecraft. The proximity of Ulysses to the ecliptic plane during this period allows us to study the effects of the solar activity at two different heliolongitudinal and heliocentric distances but at similar heliolatitudes. We identify the main transient proton enhancements seen by Wind and Ulysses from October 1997 to the end of December 1998, We compare their characteristics and suggest an interpretation in terms of their heliospheric location, the activity occurring at the Sun, and the conditions for particle propagation between the Sun and both spacecraft. Whereas at 1 RU different SEP events can be associated with individual coronal mass ejections (CMEs), at 5 AU long-lasting SEP events are observed while a sequence of CMEs takes place at the Sun, Continuous injection of particles from traveling CME-driven shocks, the effects of particle propagation along interplanetary magnetic field lines, acid the corotation of these field lines across the Ulysses location are the main factors responsible for these long-lasting periods of high particle intensity observed by Ulysses. [References: 45]

机译：1997年底太阳活动水平的增加与Wind和Ulysses航天器观测到的太阳高能粒子（SEP）事件相吻合。在此期间，尤利西斯（Elysses）与黄道平面的接近使我们能够研究太阳活动在两个不同的日向纵向距离和日向中心距离但在相似的日高纬度下的影响。我们确定了Wind和Ulysses从1997年10月到1998年12月底看到的主要瞬时质子增强，我们比较了它们的特征，并提出了关于它们的日球位置，太阳活动和粒子传播条件的解释。在太阳和两个航天器之间。在1 RU时，不同的SEP事件可能与单个冠状物质抛射（CME）相关，而在5 AU时，会观察到持久的SEP事件，而一系列CME在太阳下发生，CME驱动的震动不断注入粒子，粒子沿行星际磁场线传播的影响，酸化这些磁场线在尤利西斯位置上的共同旋转是造成尤利西斯观测到的这些高强度粒子长持续时间的主要因素。 [参考：45]

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《Journal of Geophysical Research. Biogeosciences》 |2000年第8期|共24页
作者
Lario D.; Sanderson TR.; Maksimovic M.; Sanahuja B.; Plunkett SP.; Balogh A.; Forsyth RJ.; Lin RP.; Gosling JT.; Marsden RG.;
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正文语种 eng
中图分类地球物理学;
关键词
Coronal mass ejection; Particle events; Interplanetary shocks; Driven shocks; Cosmic-rays; Ulysses; Wind; Flares; Propagation; Spacecraft;

机译：日冕物质抛射;粒子事件;行星际冲击;驱动冲击;宇宙射线;尤利西斯;风;耀斑;传播;航天器;

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1. Energetic proton observations at 1 and 5 AU 2. Rising phase of the solar cycle 23 [J] . Lario D., Sanderson TR., Maksimovic M., Journal of Geophysical Research. Biogeosciences . 2000,第A8期

机译：在1和5 AU 2处的高能质子观测。太阳周期的上升阶段23
2. The Solar Wind at 1 AU During the Declining Phase of Solar Cycle 23: Comparison of 3D Numerical Model Results with Observations [J] . Lee CO, Luhmann JG, Odstrcil D, Solar physics . 2009,第1期

机译：太阳周期23下降阶段1 AU处的太阳风：3D数值模型结果与观测值的比较
3. Solar energetic particle events during the rise phases of solar cycles 23 and 24 [J] . R. Chandra, N. Gopalswamy, P. Maekelae, Advances in space research . 2013,第12期

机译：太阳周期23和24上升阶段的太阳高能粒子事件
4. Multi-spacecraft observations of solar energetic electron events during the rising phase of solar cycle 24 [C] . WOLFGANG DROEGE, RAUL GOMEZ-HERRERO, YULIA KARTAVYKH, International Cosmic Ray Conference . 2011

机译：太阳周期上升阶段太阳能量电子事件的多航天器观测24
5. Connecting coronal holes and open magnetic flux through observation and models of solar cycles 23 and 24. [D] . Lowder, Christopher Alan. 2015

机译：通过太阳周期23和24的观测和模型连接日冕孔和开放的磁通量。
6. Solar origins of solar wind properties during the cycle 23 solar minimum and rising phase of cycle 24 [O] . Janet G. Luhmann, Gordon Petrie, Pete Riley 2013

机译：周期23的太阳风属性的太阳起源周期24的太阳最小和上升阶段
7. Solar origins of solar wind properties during the cycle 23 solar minimum and rising phase of cycle 24 [O] . Janet G. Luhmann, Gordon Petrie, Pete Riley 2013

机译：在周期24太阳能最小和周期24的上升阶段期间太阳能风能的太阳能起源

Energetic proton observations at 1 and 5 AU 2. Rising phase of the solar cycle 23

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