solar flux

Parameterization of solar radiative flux calculation in the atmosphere

有云大气中太阳辐射通量的参数化计算

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There is high correlation between flux variations of the solar X-ray bursts and the recorded low freguency sudden phase anomalies ( LF-SPA).

相关分析表明，太阳X射线爆发的流量变化量与低频记录的突然相位异常（SPA）的变化量之间有好的相关性。

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In this paper, based on correlative analysis between observed SPA events for VLF signals and the flux density of solar X-ray bursts, a quantitative relation between the flux of the solar X-ray bursts and height variations of the ionosphere at the time of SPA events is found.

本文通过实测的VLF信号的SPA事件的数据和太阳X射线爆发通量密度之间的相关分析，建立了它们之间的数值关系。

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The results show that the ambient solar wind speed and the ICME transit time errors show little correlation, even after taking into account the angle of magnetic cloud flux tube to the ecliptic plane the correlation is still not obvious.

结果表明，背景太阳风速度和ICME渡越时间并没有明显的相关性，在考虑了磁云通量管轴相对黄道面夹角的影响后相关性仍然不明显。

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The calculation showed that the variation of solar absorptance with the angle of incidence must be considered to calculate precisely the absorbed solar flux for the satellites with second surface mirror or anodized aluminum coating.

计算结果表明，对采用二次表面镜或铝光亮阳极氧化涂层的卫星，在计算吸收的太阳热流量时，必须考虑太阳吸收比随人射角的变化。

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Most extreme high level of electron flux at geostationary orbit occurred during the geomagnetic storm recovery phase with the solar wind proton density lower than 4 cm-3 and strong substorm activity.

绝大多数高通量事件都是出现在磁暴恢复相期间，且太阳风质子密度低于4个/cm3并伴有亚暴时才会发生。

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Solar Atmospheric Responses to. Magnetic Flux Eruptions I. A Mechanism for Coronal Mass Ejections

磁通量喷发的大气响应Ⅰ.日冕物质喷射机制

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Low solar wind density and the strong substorm are the two key parameters leading to the 2 MeV electron flux at geostationary orbit reach very high level during the geomagnetic storm recovery phase.

在磁暴恢复相期间，低的太阳风密度和强的亚暴是导致地球同步轨道能量大于2MeV电子通量的达到极高值的两个关键参数。

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