首页> 外文会议>SPIE Conference on Ground-Based and Airborne Instrumentation for Astronomy >Design of a next generation synoptic solar observing network: solar physics research integrated network group (SPRING)
【24h】

Design of a next generation synoptic solar observing network: solar physics research integrated network group (SPRING)

机译:下一代天气太阳能观测网络设计:太阳能物理研究综合网络组(春季)

获取原文
获取外文期刊封面目录资料

摘要

Long-term synoptic observations of the Sun in different wavelength regions are essential to understand its secular behavior. Such observations have proven very important for discovery of 11 year solar activity cycle, 22 year magnetic cycle, polar field reversals, Hale's polarity law, Joy's law, that helped Babcock and Leighton to propose famous solar dynamo model. In more recent decades, the societal impact of the secular changes in Sun's output has been felt in terms of solar inputs to terrestrial climate-change and space-weather hazards. Further, it has been realized that to better understand the activity phenomena such as flares and coronal mass ejections (CMEs) one needs synoptic observations in multiple spectral lines to enable tomographic inference of physical parameters. Currently, there are both space and ground based synoptic observatories. However, given the requirements for the long-term stability and reliability of such synoptic datasets, ground-based facilities are more preferable. Also, the ground based observatories are easy to maintain or upgrade while detailed and frequent calibrations are easily possible. The only ground-based facility that currently provides full-disk velocity and magnetic field maps of the Sun around the clock and at good cadence, is the Global Oscillations Network Group (GONG) network of National Solar Observatory (NSO) which is operational since the mid 90s. Due to its aging instrumentation, operating for nearly three decades, and new requirements to obtain multi-wavelength observations, a need is felt in the solar community to build a next generation synoptic observatory network. A group of international observatories have come together under the auspices of SOLARNET program, funded by European Union (EU), to carryout a preliminary design study of such a synoptic solar observing facility called "SPRING", which stands for Solar Physics Research Integrated Network Group. In this article we will present concept of SPRING and the
机译:在不同波长区域中的太阳的长期偶数观察对于了解其世俗行为至关重要。这种观察结果已经证明了11年的42年太阳能活动周期,22年磁性循环,极地逆转,哈利的极性法,欢乐法,帮助Babcock和Leighton提出着名的太阳能发电机模型。在近几十年来,在太阳能投入到陆地气候变化和空间天气危害方面,感受到Sun产出的世俗变化的社会影响。此外,已经意识到,为了更好地理解诸如耀斑和冠状质量射血(CMES)的活动现象(CMES),一种需要多种光谱线的概要观察,以实现物理参数的断层监测推断。目前,有空间和地面的舞台观测。然而,鉴于对这种舞台数据集的长期稳定性和可靠性的要求,更优选基于地面设施。此外,基于地面的观察者易于维护或升级,而详细和频繁的校准很容易。目前唯一基于地面的设施,目前为时钟和良好的Cadence提供全磁盘速度和磁场地图,是全球振荡网络组(Gong)网络的国家太阳天文台(NSO),自于此90年代中期。由于其老化仪器,运行近三十年,并获得多波长观测的新要求,在太阳能社区中感受到了一种建立下一代揭练天文台网络的需求。一群国际观察者在Solarnet计划的主持下,由欧盟(欧盟)资助的Solarnet计划,进行了初步设计研究,该研究称为“Spring”,它代表太阳能研究综合网络组。在本文中,我们将呈现春季的概念和

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号