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Searching for Photospheric Causes of Small-Scale Chromospheric Activity

Searching for Photospheric Causes of Small-Scale Chromospheric Activity
寻找小规模色球活动的光球原因
批准号:
1146896
负责人:
Vasyl Yurchyshyn
金额:
$39.78万
依托单位国家:
美国
项目类别:
Continuing Grant
财政年份:
2012
资助国家:
美国
项目状态:
已结题
起止时间:
2012-02-01 至 2016-01-31

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中文摘要
翻译
这个研究小组将使用大熊太阳天文台(BBSO)的新太阳望远镜(NST)来研究太阳色球层特征的起源,如针状体、“快速蓝移事件”和所谓的“海葵喷流”,以及最近由BBSO工作人员使用NST发现的微小的粒间喷流。特别是,这个团队将通过分析NST和航天器对日冕洞和“安静太阳”区域的高分辨率观测,来限制色球层上涌的驱动机制。他们将研究色球射流特性(如速度、与太阳磁场的关系和时间演化),以及色球对太阳光球动力学的响应。研究小组还将组织几次联合观测和数据分析活动,包括NST和选定的航天器,以前所未有的清晰度捕捉太阳表面现象的细节,揭示太阳光球层和色球层中小尺度磁场的动态。该团队希望他们的分析能够为日冕加热和太阳低层大气中的相关过程提供新的见解,并促进我们对太阳风加速的理解。团队成员将向更广泛的太阳能社区提供他们新的NST数据,并应外部研究人员的要求进行特定的太阳观测。他们注意到,NST最近的高质量图像已经引起了公众的极大兴趣(例如,列入《国家地理》“2010年最佳太空图片”的名单),他们预计这种形式的推广将继续下去。这项研究活动也将支持研究生的进一步教育和专业成长。
英文摘要
This research team will use the New Solar Telescope (NST) of the Big Bear Solar Observatory (BBSO) to investigate the origins of solar chromospheric features, such as spicules, "rapid blue shifted events," and so-called "anemone jets," as well as the tiny intergranular jets recently discovered by BBSO staff using the NST. In particular, this team will constrain the driving mechanisms of chromospheric upflows by analyzing high resolution NST and spacecraft observations of coronal holes and "quiet Sun" areas. They will study chromospheric jet properties (such as velocities, association with the solar magnetic field, and time evolution), as well as chromospheric response to solar photospheric dynamics. The research team will also organize several joint observational and data analysis campaigns involving NST and selected spacecraft for capturing the details of solar surface phenomena with unprecedented clarity, revealing the dynamics of small scale magnetic fields in the Sun's photosphere and chromosphere. This team expects their analysis to provide new insight into coronal heating and related processes in the lower solar atmosphere, as well as to advance our understanding of solar wind acceleration.The team members will provide their new NST data to the wider solar community and perform specific solar observations upon request from outside researchers. They note that recent high quality NST imagery has already generated significant interest among the general public (for example, making the list of National Geographic's "Best Space Pictures of 2010") and they anticipate that this form of outreach will continue. This research activity will also support the further education and professional growth of a graduate student.
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SHINE: Prediction of Coronal Mass Ejections and Interplanetary Magnetic Fields Using Advanced Artificial Intelligence Techniques
  • 批准号:
    2300341
  • 项目类别:
    Standard Grant
  • 资助金额:
    $57.32万
  • 财政年份:
    2023
  • 负责人:
    Vasyl Yurchyshyn
  • 依托单位:
High-resolution studies of dynamic processes in the sunspot umbra: Preparing for the era of the Daniel K. Inouye Solar Telescope
  • 批准号:
    1614457
  • 项目类别:
    Standard Grant
  • 资助金额:
    $28.5万
  • 财政年份:
    2016
  • 负责人:
    Vasyl Yurchyshyn
  • 依托单位:
Space Weather: Short-term Prediction of Solar Flares and Geoeffectiveness of Solar Coronal Mass Ejections
  • 批准号:
    0205157
  • 项目类别:
    Continuing Grant
  • 资助金额:
    $13.6万
  • 财政年份:
    2002
  • 负责人:
    Vasyl Yurchyshyn
  • 依托单位:
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