ESO/ALMA会议“ALMA 2019:科学成果和跨设施协同效应”报告

IF 0.3 Q4 COMMUNICATION
C. Kemper
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引用次数: 1

摘要

阿塔卡马大型毫米/亚毫米阵列(ALMA)是地球上最大、最灵敏的毫米/亚毫米阵列,具有最高的空间分辨率。自开始运行以来,ALMA一直处于该波长范围的科学前沿,提供突破性的发现。ALMA 2019科学会议是全球ALMA社区定期举行的一系列会议之一,上一届会议于2016年在美国印第安维尔斯举行。在观测周期7开始之际,ALMA 2019会议为科学界提供了一个反思该设施所取得的众多科学成果的机会,特别强调了ALMA大型计划第一轮的结果、长基线和高频能力、新的太阳和甚长基线干涉测量(VLBI)模式,以及ALMA与其他天文台之间的协同作用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Report on the ESO/ALMA Conference “ALMA 2019: Science Results and Cross-Facility Synergies”
The Atacama Large Millimeter/submillimeter Array (ALMA) is the largest and most sensitive millimetre/submillimetre array on the planet, with the highest spatial resolution. Since it began operating, ALMA has routinely been at the forefront of science in this wavelength regime, delivering groundbreaking discoveries. The ALMA 2019 science conference was organised as one of a series of meetings held at regular intervals for the worldwide ALMA community, the previous one being held in Indian Wells, USA in 2016. At the start of Cycle 7 of observations, the ALMA 2019 conference provided an opportunity for the community to reflect on the multitude of scientific results from the facility, with special emphasis on the results from the first rounds of ALMA Large Programmes, the long baselines and high-frequency capabilities, the new solar and very long baseline interferometry (VLBI) modes, as well as the synergy between ALMA and other observatories.
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来源期刊
Jurnal The Messenger
Jurnal The Messenger COMMUNICATION-
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