Solar Coronal Loops Workshop V; Palma de Mallorca, Spain; June 2011
Solar Coronal Loops Workshop V; Palma de Mallorca, Spain; June 2011
批准号:
1102539
负责人:
Ignacio Ugarte-Urra
金额:
$1.0万
依托单位:
依托单位国家:
美国
项目类别:
Standard Grant
财政年份:
2011
资助国家:
美国
项目状态:
已结题
起止时间:
2011-03-01 至 2012-02-29
中文摘要
首席调查员将为8名学生和博士后参加2011年在西班牙马略卡岛举行的第五届日冕环路讲习班提供旅费。2011年的这次会议非常及时,是在2010年太阳动力学观测站(SDO)航天器发射一年后举行的。SDO极大地提高了我们观测日冕活动的能力,其数据现已广泛向公众开放。日冕环路研讨会将提供广泛的社区服务,为太阳物理理论家和观察者提供发展合作的机会,对抗反对的观点并对其进行测试,最终激发新的研究来解决公开的科学问题。自2002年日冕环Wokshop系列诞生以来,该场所已成为研究人员详细讨论太阳活动区日冕环形成、动力学和演化的基本物理过程的理想场所。由日冕环路研讨会社区开发的开放邮件列表与全球170多名科学家进行交流,使这些研究人员能够不断交流有关日冕环路研究的想法、新结果、出版物和信息。该研讨会传统上支持博士生和年轻博士后的出席和参与。因此,这次会议将为学生和青年科学家创造有意义的机会,让他们接触该领域的专家,并最终成为下一代太阳物理研究的主要参与者。
英文摘要
The Principal Investigator will provide travel support for eight students and postdocs to attend the Fifth Coronal Loops Workshop to be held in Mallorca, Spain in 2011. This 2011 meeting is very timely, coming about a year after the 2010 launch of the Solar Dynamics Observatory (SDO) spacecraft. SDO has dramatically improved our ability to observe activity in the solar corona, and its data are now widely available to the public. The Coronal Loops Workshop will provide a broad community service by giving solar physics theorists and observers the opportunity to develop collaborations, confront opposing views and test them, and ultimately inspire new investigations to address open scientific questions. Since 2002, when the Coronal Loops Wokshop series originated, the venue has become an ideal setting for researchers to discuss in detail the basic physical processes behing the formation, dynamics, and evolution of coronal loops in solar active regions. An open mailing list developed by the Coronal Loops Workshop community communicates with over 170 scientists worldwide, allowing those researchers to continuously exchange ideas, new results, publications, and information on coronal loops research. The workshop has traditionally been supportive of the attendance and participation of Ph.D. students and young postdocs. This meeting will therefore create meaningful opportunities for students and young scientists to engage experts in the field, and ultimately to become key participants in the next generation of solar physics research.
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