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The corona we see during an eclipse is an overlap of the continuous,largely polarized, K-corona, the basically unpolarized F-corona, and in the inner corona an overlay of emission lines.
在日蚀期间我们所见到的日冕是连续的重叠，K-corona极化程度很大，F-corona基本上不极化，在日冕内部覆盖一组射线。
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Soil available N was positively correlated with spore density of Salvia miltiorrhiza and Dioscorea opposite, and hyphal and total percent colonization of Adenophora borealis, while negatively correlated with arbuscular colonization of Aster tataricus; Soil available P exhibited a positive correlation with arbuscular colonization of Salvia miltiorrhiza and vesicular colonization of Dioscorea opposite, while a negative correlation with spore density of Platycodon grandiflorus and vesicular colonization of Atractylodes macrocephala; Spore density of Bupleurum Chinense had a positive affection with soil organic matter; Soil pH was negatively correlated with hyphal and total colonization of Adenophora borealis and spore density of Bupleurum chinense, while positively correlated with spore density of Adenophora borealis.
土壤碱解N与丹参和麻山药的孢子密度、北沙参菌丝定殖率和总定殖率呈显著正相关，与紫苑丛枝定殖率呈显著负相关。土壤速效P与丹参丛枝定殖率、麻山药泡囊定殖率呈显著正相关，与桔梗孢子密度、白术泡囊定殖率呈显著负相关。土壤有机质与北柴胡孢子密度呈显著负相关。土坡pH与北沙参菌丝定殖率和总定殖率、北柴胡孢子密度呈显著负相关，与北沙参孢子密度呈显著正相关。
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Multiple wavelengths characteristics of dayside aurora activities were investigated with these keograms and in reference to all-sky images. It was found that there are three repeatedly appearing aurora activity regions along the dayside aurora oval. They are, Region A around 0900MLT in which aurora moves poleward while its intensity decreasing, and its form changingfrom arc to corona with time; Region B around 1330MLT in which aurora moves equatorward while its intensity increasing, and its form changing from corona to arc in time; Region C around 1330MLT in which aurora expands poleward while its intensity decreasing, and its forma evolving from arc to multiple arcs in time. There is a narrow belt of aurora activity in North-South direction between Regions A and B, which is dominated by weak and red corona aurora.
初步分析发现，沿日侧极光卵不论磁静日还是磁扰日，在三个波段上都同时观测到了四个重复出现的极光活动区，即0900MLT附近的A区、1330MLT的B区和1630MLT的C区以及1200MLT附近的G区。A区内的极光活动由低纬向高纬运动，强度逐渐变弱，形态由较宽的弧状极光向冕状极光演变；B区内的极光活动由高纬向低纬方向运动，形态呈现为冕状极光向较窄的极光弧的演变，极光强度逐渐增强；C区极光活动向高纬方向展宽，强度逐渐变弱，极光由单弧向多重弧演化；而在A与B之间存在一个纬度范围相对较窄的极光活动区G区，该区的极光呈现暗弱的冕状极光。
- 更多网络解释 与Corona Borealis相关的网络解释 [注：此内容来源于网络，仅供参考]
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Corona Borealis：北冕座
北冕座(Corona Borealis)是北天星座之一. 中心位置在赤经15时50分,赤纬33°. ...北 冕座位于牧夫座和武仙座之间. 在天琴座织女星和牧夫座大角连线靠近大角的地方, ...
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Corona Borealis：北冕星座
"我以勇气的名义呼唤北冕星座(Corona Borealis)的力量"穆迪举起了魔杖,发出绿色的光芒. "我以智慧的名义呼唤天鹰星座(Aquilae)的力量"从杰拉德魔杖发出的橙黄色光芒指向了天鹰座.
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Corona Borealis：北冕
南冕 Corona Austrina | 北冕 Corona Borealis | 乌鸦 Corvus
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Corona Borealis：北冕座Corvus 乌鸦座
Corona Australis 南冕座 | Corona Borealis 北冕座Corvus 乌鸦座 | Crater 巨爵座
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Corona Borealis CrB：北冕座
Corona Austrilis CrA 南冕座 128 25 | Corona Borealis CrB 北冕座 179 20 | Corvus Crv 乌鸦座 184 15
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