SSALMON——阿塔卡马大型毫米波观测阵网络太阳模拟
太阳与恒星天体物理
2016-01-20 v3
摘要
SSALMON (Solar Simulations for the Atacama Large Millimeter Observatory Network) 于2014年与两项ALMA发展研究相关联发起。Atacama Large Millimeter/submillimeter Array (ALMA) 是一个强大的新工具，也可以以高空间、时间和光谱分辨率观测太阳。国际SSALMONetwork旨在协调ALMA太阳观测模式的进一步发展，并促进太阳物理的科学机会，特别关注数值模拟，其可为观测模式提供重要约束并有助于未来观测的解释。ALMA探测的辐射主要源自太阳色球层——光球与日冕之间复杂而动态的层，在能量和物质传输以及太阳大气外层的加热中起重要作用。潜在目标包括活动区、日珥、宁静太阳区、耀斑。此处，我们简要概述该网络及未来ALMA太阳观测的潜在科学案例。
引用
@article{arxiv.1502.05601,
title = {SSALMON - The Solar Simulations for the Atacama Large Millimeter Observatory Network},
author = {S. Wedemeyer and T. Bastian and R. Brajsa and M. Barta and H. Hudson and G. Fleishman and M. Loukitcheva and B. Fleck and E. Kontar and B. De Pontieu and S. Tiwari and Y. Kato and R. Soler and P. Yagoubov and J. H. Black and P. Antolin and S. Gunar and N. Labrosse and A. O. Benz and A. Nindos and M. Steffen and E. Scullion and J. G. Doyle and T. Zaqarashvili and A. Hanslmeier and V. M. Nakariakov and P. Heinzel and T. Ayres and M. Karlicky and the SSALMON Group},
journal= {arXiv preprint arXiv:1502.05601},
year = {2016}
}
备注
15 pages, 3 figures, to appear in Advances in Solar Physics (special issue of Advances in Space Research, AdSR), proceedings of the 14th European Solar Physics Meeting (ESPM-14, Dublin, Ireland, September 2014); (resubmitted version after minor revision)