共查询到19条相似文献，搜索用时 125 毫秒
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姚进生 《紫金山天文台台刊》1992,11(3):250-254
本文介绍了一种不仅可以测定太阳。月亮,大、小行星和恒星的位置以及太阳的角直径,而且还能测定方位标方位角的多功能光电测微器。初步使用结果表明:其性能良好,系统稳定:获得了满意的方位标定位精度;达到了预期设计要求。 相似文献
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3月4日 木星冲日 木星冲日是指木星和太阳的视黄经相差180度的天文现象。行星在围绕太阳公转的过程中,太阳、地球和行星的位形随时变化。从地球看去,外行星和太阳间的方位在不断变化,当行星和太阳方位相同(黄经相等)时称为合日,当行星和太阳的黄经相差90度时称为方照。冲日时,行星和太阳的黄经差最大,方位刚好相反:太阳在东方,行星在西方,太阳落山之际,行星刚刚在东地 相似文献
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1m太阳望远镜的方位驱动控制系统采用液压轴承,液压系统正常工作时望远镜才能实现平稳旋转。可通过油压、油温监测液压系统的工作状态。针对原有液压系统不能提供其工作状态实时监测和自动化程度较低的缺陷,设计了液压监控系统并将其集成到望远镜控制系统中,可实现油压油温数据采集、油压异常报警、油泵自动启停等功能,保证液压轴承的安全运转。介绍了该监控系统的结构和工作原理,阐述了油压、油温数据采集系统的软硬件实现并给出了相应的实验数据和运行结果。理论分析和实验结果表明系统工作正常,数据采集速度快、分辨率高,精度可满足要求,能长期稳定运行。 相似文献
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分布式多CCD实时控制与图像采集系统软件的研制是1 m红外太阳塔进入常规观测的必要条件。重点讨论了太阳塔多CCD实时控制与图像采集软件系统的研制,包括软件系统采取的主控前置系统结构、工作流程,为了解决主控机和前置机之间通信而设计的通信协议,利用双缓存、双模数变换器(Analog-to-Digital Converter,ADC)、存储器直接访问(Direct Memory Access,DMA)技术提高图像处理和存储速度,利用多线程机制实现多CCD的同步图像采集,前置系统定时向主控系统发送心跳信息以增强系统的可靠性。经实际测试,系统达到了预定指标,初步满足1 m红外太阳塔的观测需求。 相似文献
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太阳磁像仪是开展太阳磁场观测研究的核心仪器,其中的稳像系统是空间太阳磁像仪的关键技术之一,针对深空探测卫星系统对载荷重量、尺寸限制严苛的要求,设计了基于图像自校正方法的稳像观测系统.介绍了一套基于现场可编程门阵列(Field-Programmable Gate Array, FPGA)和数字信号处理器(Digital Signal Processor, DSP),通过基于自相关算法的高精度稳像方法设计,并结合精确偏振调制、准确交替采样控制等系统软硬件设计,克服由于卫星平台抖动、指向误差等因素造成的图像模糊,实现实时相关、校正、深积分的稳像观测系统.针对像素尺寸为1 K×1 K、帧频为20 fps的CMOS (Complementary Metal Oxide Semiconductor)探测器,实现了1像元以内的实时稳像观测精度.在完成实验室测试后, 2021年6月18日在国家天文台怀柔太阳观测基地35 cm太阳磁场望远镜上开展了实测验证,结果表明该系统能够有效地完成太阳磁像仪自校正稳像观测,获得了更高分辨率的太阳磁场数据.稳像系统的成功研制不仅可以为深空太阳磁像仪的研制提供轻量化、高... 相似文献
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位于云南天文台凤凰山本部的10 m太阳射电望远镜是中国太阳射电物理界重要的观测设备之一,其设计之初,800~975 MHz频段受到移动电话的严重干扰,不能正常工作,因此缺失这一频段的观测资料。近年来,随着微波和数字器件性能的提升以及移动电话工作频段的改变,使得这一重要频段的观测变得可行。针对800~975 MHz频段的太阳射电天文信号,提出了一种基于现场可编程门阵列(Field Programmable Gate Array,FPGA)和千兆以太网的实时采集与处理方法。在数据采集和处理过程中,系统采用流水线方式,得到了太阳射电信号的实时频谱图;采用硬件描述语言Verilog实现了千兆以太网的数据传输,提高了传输效率;另外本系统采用分时传输机制,完成千兆以太网的UDP数据包的传输。最后还对所得数据进行了误差分析和结果分析,证明了本文提出的实时信号采集、分析和传输方法的正确性和可靠性。 相似文献
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在太阳耀斑区磁场和电流研究方面，文中将着重介绍太阳横向磁场方位的确定，太阳活动区磁场的非热性表示、太阳耀斑前后的活动区磁场变化、以及耀斑核块与活动区纵向电流密度极大点位置的关系等几个重要问题的研究现状。 相似文献
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《天文研究与技术》2020,(2)
观测技术及仪器的进步推动了太阳物理的研究,步进电机是各类观测仪器精密结构调整部件中经常采用的驱动源,步进电机控制系统的性能直接影响太阳望远镜的数据精度和时间分辨率。介绍了一套怀柔太阳观测基地自主研制的多轴步进电机控制系统。该系统以现场可编程门阵列为核心控制器,利用中断处理机制及输入/输出寄存器产生多路晶体管-晶体管逻辑电平(TTL)方波信号,结合驱动器实现多轴步进电机控制;通过周期信号化简处理算法缩短电机调整时间;以霍尔器件作为位置传感器实现系统闭环控制,通过对霍尔信号的软、硬件滤波处理,提高信号识别的准确率;设计了板载存储电路,实时保存系统关键参数,大幅提高系统整体的可靠性。同时,该系统设计了丰富的输入/输出接口、通讯接口,提高系统的可集成性。目前该系统已在多台太阳望远镜中投入使用。 相似文献
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Solar catalogs are frequently handmade by experts using a manual approach or semi-automated approach. The appearance of new tools is very useful because the work is automated. Nowadays it is impossible to produce solar catalogs using these methods, because of the emergence of new spacecraft that provide a huge amount of information. In this article an automated system for detecting and tracking active regions and solar flares throughout their evolution using the Extreme UV Imaging Telescope (EIT) on the Solar and Heliospheric Observatory (SOHO) spacecraft is presented. The system is quite complex and consists of different phases: i) acquisition and preprocessing; ii) segmentation of regions of interest; iii) clustering of these regions to form candidate active regions which can become active regions; iv) tracking of active regions; v) detection of solar flares. This article describes all phases, but focuses on the phases of tracking and detection of active regions and solar flares. The system relies on consecutive solar images using a rotation law to track the active regions. Also, graphs of the evolution of a region and solar evolution are presented to detect solar flares. The procedure developed has been tested on 3500 full-disk solar images (corresponding to 35 days) taken from the spacecraft. More than 75 % of the active regions are tracked and more than 85 % of the solar flares are detected. 相似文献
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全日面矢量磁像仪(Full-disk vector MagnetoGraph, FMG)是先进天基太阳天文台(Advanced Space-based Solar Observatory, ASO-S)卫星的3台主载荷之一,为开展FMG全系统性能测试和定标试验,已搭建用于FMG外场测试的地面试观测平台.利用该平台模拟FMG在轨跟踪状态,研制了基于全日面太阳图像的望远镜导行系统.该系统通过大面阵CCD (Charge Coupled Device)采集太阳像、多重逻辑条件判定、微调恒动跟踪速度校正偏移等策略,实现了RMS (Root Mean Square)优于1′′/30 min的跟踪精度.通过分析FMG方案阶段试观测的太阳纵向磁图,开启导行30 min后磁图特征点在赤经方向的偏移比恒动条件下减少17.5′′,提升了磁图空间分辨率.测试过程中该系统达到设计指标且工作稳定,为FMG地面试观测提供了良好的技术支撑. 相似文献
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Based on a set of 11 CME events we study the impact of projection effects by tracking CME leading edge features in the plane of sky (traditional CME tracking) from combined STEREO-SECCHI and SOHO-LASCO observations up to 20R ⊙. By using CME observations from two vantage points and applying triangulation techniques, the source region location of the CME on the solar surface was determined (heliospheric longitude and latitude) to correct for projection effects. With this information, the directivity and “true” speed of a CME can be estimated in a simple way. The comparison of the results obtained from the spacecraft pairs SOHO-LASCO/STEREO-A and SOHO-LASCO/STEREO-B allows us to study the reliability of the method. The determined CME source region is generally coincident within ?10°. 相似文献
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Local correlation tracking (LCT) is a commonly used motion tracking technique, particularly in solar physics. When used to track motions smaller than one pixel per time sample, interpolation of the original data is required. We demonstrate that it is possible to introduce large systematic errors by using an inappropriate interpolation method, and describe how to avoid these errors. The effect of these errors on the calculated velocity field is demonstrated on simulated solar granulation data. 相似文献
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V. M. Gogod 《Astronomische Nachrichten》1992,313(2):97-100
The potential possibilities of RATAN-600 for solar studies are considered which are going on to be realized during the present maximum of solar activity. Different methods of an improvement of the characteristics of the antenna-receiver system are analyzed. These are: – realization of tracking the Sun during about 4 hours for a day and attaining temporal resolution up to some msec, – realization of radio-heliographic observations, – realization of a full spectral coverage of the radio telescope from 1,5 to 18 GHz with a frequency reslution up to 1–2 MHz, – combination of all possibilities mentioned above in an adaptable solar observing complex. 相似文献
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A 48 GHz five-radiometer front end was installed at the Cassegrain focus of the 13.7-m Itapetinga antenna for the observation of solar bursts. The system works with five beam patterns partly overlapping. The five antenna temperatures are recorded with a temporal resolution of 1 millisecond, including time and antenna position. The ratios of the incoming antenna signals are used to determine the centroid of burst emission. Its coordinates are determined from groups of three receivers by using a least-square fit. In favourable observing conditions we obtain an angular accuracy of about 2 arc sec (r.m.s.), with a time resolution of 1 ms and a sensitivity of 0.05 s.f.u. The accuracy of the antenna tracking, the absolute pointing and the quality of radio seeing at Itapetinga are discussed. A preliminary analysis of an impulsive solar burst event is used to illustrate the capabilities of the method described here. 相似文献