The magnetic fields and dynamical processes in the solar polar regions play a crucial role in the solar magnetic cycle and in supplying mass and energy to the fast solar wind,ultimately being vital in controlling sola...The magnetic fields and dynamical processes in the solar polar regions play a crucial role in the solar magnetic cycle and in supplying mass and energy to the fast solar wind,ultimately being vital in controlling solar activities and driving space weather.Despite numerous efforts to explore these regions,to date no imaging observations of the Sun's poles have been achieved from vantage points out of the ecliptic plane,leaving their behavior and evolution poorly understood.This observation gap has left three top-level scientific questions unanswered:How does the solar dynamo work and drive the solar magnetic cycle?What drives the fast solar wind?How do space weather processes globally originate from the Sun and propagate throughout the solar system?The Solar Polarorbit Observatory(SPO)mission,a solar polar exploration spacecraft,is proposed to address these three unanswered scientific questions by imaging the Sun's poles from high heliolatitudes.In order to achieve its scientific goals,SPO will carry six remote-sensing and four in-situ instruments to measure the vector magnetic fields and Doppler velocity fields in the photosphere,to observe the Sun in the extreme ultraviolet,X-ray,and radio wavelengths,to image the corona and the heliosphere up to 45 R_(s),and to perform in-situ detection of magnetic fields,and low-and high-energy particles in the solar wind.The SPO mission is capable of providing critical vector magnetic fields and Doppler velocities of the polar regions to advance our understanding of the origin of the solar magnetic cycle,providing unprecedented imaging observations of the solar poles alongside in-situ measurements of charged particles and magnetic fields from high heliolatitudes to unveil the mass and energy supply that drive the fast solar wind,and providing observational constraints for improving our ability to model and predict the three-dimensional(3D)structures and propagation of space weather events.展开更多
【目的】对热压干燥过程中杨木锯材芯层温度和压力进行测试,探究热压板温度对热压干燥过程中杨木锯材芯层温度和压力等参数及水分状态的影响,为热压干燥机理研究提供依据。【方法】采用集成探针同步测量并记录热压干燥过程中杨木锯材芯...【目的】对热压干燥过程中杨木锯材芯层温度和压力进行测试,探究热压板温度对热压干燥过程中杨木锯材芯层温度和压力等参数及水分状态的影响,为热压干燥机理研究提供依据。【方法】采用集成探针同步测量并记录热压干燥过程中杨木锯材芯层温度和压力,通过对杨木锯材芯层压力测量值与测量温度对应的饱和蒸汽压力值(压力理论值)进行对比分析,进而推测热压板温度对热压干燥过程中杨木锯材水分状态的影响。【结果】当热压板温度从120℃升高到140℃时,杨木锯材芯层压力峰值从146.4 k Pa增大到213.1 k Pa,相应温度峰值从102.8℃升高到123.7℃,温度和压力同时达到峰值,到达峰值时间从17.5 min缩短到11.6 min。当热压板温度为120和130℃时,含水率高于纤维饱和点的杨木锯材芯层水分为过压的未饱和水,热压干燥后杨木锯材芯层终含水率(48.55%和49.88%)高于纤维饱和点;当热压板温度升高到140℃时,杨木锯材芯层自由水受热汽化形成水蒸气,并随着蒸汽温度的升高由饱和状态转化为过热状态,热压干燥后杨木锯材芯层终含水率(27.70%)低于纤维饱和点。【结论】热压干燥过程中热压板温度越高,杨木锯材芯层温度和压力达到的峰值越高,峰值持续时间越短。热压干燥过程中含水率高于纤维饱和点的杨木锯材水分状态根据热压板温度不同,可为液态水(过压的未饱和水)、饱和水蒸气或过热蒸汽状态。展开更多
文摘The magnetic fields and dynamical processes in the solar polar regions play a crucial role in the solar magnetic cycle and in supplying mass and energy to the fast solar wind,ultimately being vital in controlling solar activities and driving space weather.Despite numerous efforts to explore these regions,to date no imaging observations of the Sun's poles have been achieved from vantage points out of the ecliptic plane,leaving their behavior and evolution poorly understood.This observation gap has left three top-level scientific questions unanswered:How does the solar dynamo work and drive the solar magnetic cycle?What drives the fast solar wind?How do space weather processes globally originate from the Sun and propagate throughout the solar system?The Solar Polarorbit Observatory(SPO)mission,a solar polar exploration spacecraft,is proposed to address these three unanswered scientific questions by imaging the Sun's poles from high heliolatitudes.In order to achieve its scientific goals,SPO will carry six remote-sensing and four in-situ instruments to measure the vector magnetic fields and Doppler velocity fields in the photosphere,to observe the Sun in the extreme ultraviolet,X-ray,and radio wavelengths,to image the corona and the heliosphere up to 45 R_(s),and to perform in-situ detection of magnetic fields,and low-and high-energy particles in the solar wind.The SPO mission is capable of providing critical vector magnetic fields and Doppler velocities of the polar regions to advance our understanding of the origin of the solar magnetic cycle,providing unprecedented imaging observations of the solar poles alongside in-situ measurements of charged particles and magnetic fields from high heliolatitudes to unveil the mass and energy supply that drive the fast solar wind,and providing observational constraints for improving our ability to model and predict the three-dimensional(3D)structures and propagation of space weather events.
文摘【目的】对热压干燥过程中杨木锯材芯层温度和压力进行测试,探究热压板温度对热压干燥过程中杨木锯材芯层温度和压力等参数及水分状态的影响,为热压干燥机理研究提供依据。【方法】采用集成探针同步测量并记录热压干燥过程中杨木锯材芯层温度和压力,通过对杨木锯材芯层压力测量值与测量温度对应的饱和蒸汽压力值(压力理论值)进行对比分析,进而推测热压板温度对热压干燥过程中杨木锯材水分状态的影响。【结果】当热压板温度从120℃升高到140℃时,杨木锯材芯层压力峰值从146.4 k Pa增大到213.1 k Pa,相应温度峰值从102.8℃升高到123.7℃,温度和压力同时达到峰值,到达峰值时间从17.5 min缩短到11.6 min。当热压板温度为120和130℃时,含水率高于纤维饱和点的杨木锯材芯层水分为过压的未饱和水,热压干燥后杨木锯材芯层终含水率(48.55%和49.88%)高于纤维饱和点;当热压板温度升高到140℃时,杨木锯材芯层自由水受热汽化形成水蒸气,并随着蒸汽温度的升高由饱和状态转化为过热状态,热压干燥后杨木锯材芯层终含水率(27.70%)低于纤维饱和点。【结论】热压干燥过程中热压板温度越高,杨木锯材芯层温度和压力达到的峰值越高,峰值持续时间越短。热压干燥过程中含水率高于纤维饱和点的杨木锯材水分状态根据热压板温度不同,可为液态水(过压的未饱和水)、饱和水蒸气或过热蒸汽状态。
