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China's 12 Meters Aperture Optical Telescope

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Spat threatens China’s plans to build world’s largest telescope

Jun. 14, 2017 , 10:00 AM

China's astronomers are united in wanting a world-class giant optical telescope, one that would serve notice that they are ready to compete on the global stage. But a squabble has opened up over the telescope's design. On one side is an established engineering team, led by a veteran optics expert responsible for the nation's largest existing telescope, that is eager to push ahead with an ambitious design. On the other are astronomers reveling in a grassroots priority-setting exercise—unprecedented for China—who have doubts about the ambitious design and favor something simpler.

Now, a panel of international experts has reviewed the designs and come out squarely in favor of the simpler proposal, according to a copy of the review obtained by Science. But the conclusion has not ended what one Chinese astronomer calls "an epic battle" between the high-ranking engineers accustomed to top-down control over projects and the nascent grassroots movement.

At issue is a project that emerged in 2015, when the Chinese Academy of Sciences (CAS) set up a Center for Astronomical Mega-Science that polled senior astronomers on their priorities. Top was a desire to boost China's participation in the Thirty Meter Telescope (TMT), which is being developed by an international consortium. (Construction on Hawaii's Mauna Kea has been delayed by legal claims raised by Native Hawaiians.) Second was a giant telescope of the country's own.

For now, China's largest optical telescope is the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST), a 4-meter survey telescope completed in 2008 in Hebei province near Beijing. China's astronomers rallied around the idea of leapfrogging to a 12-meter telescope that, if completed quickly before other giants like the TMT, would for some years be the largest telescope on Earth. In early 2016, the National Development and Reform Commission (NDRC), responsible for funding large domestic projects, gave the megascience center approval to develop plans for what is now being called the Large Optical/Infrared Telescope (LOT), to be sited in western China. To secure NDRC funding for construction—an estimated 1.5 billion renminbi ($220 million)—the plans must be approved by the end of 2018.

Xiangqun Cui was ready. An optics specialist, Cui heads a group at CAS's Nanjing Institute of Astronomical Optics & Technology (NIAOT) that had developed LAMOST and was already working on a 12-meter telescope design.

In most large telescopes, a large primary mirror captures light and reflects it off one or two secondary mirrors to the telescope's instruments. The daring NIAOT design calls for four mirrors—one primary and three secondary. The fourth mirror allows for exquisite control of the streams of photons so that they fall almost perpendicular to the instrument's focal plane, ensuring "very good image quality," Cui says. She adds that, because the TMT and other telescopes would eventually surpass the LOT's sensitivity, the NIAOT design needed to provide a wide field of view that would enable the telescope to act as a spotter for the bigger scopes. "This is a new century, we need new optical systems," Cui says.

In an unusual step, the megascience center set up meetings, working groups, and a science advisory committee to solicit input from the wider astronomical community—"a first for Chinese astronomy," says Johannes Andersen, an astronomer at the University of Copenhagen. Astronomers who took part expressed concerns with the NIAOT design. "I found many scientific and engineering issues," says Donglin Ma, an optics scientist at Huazhong University of Science and Technology (HUST), in Wuhan, China.

One concern centers on the four-mirror design. Many astronomers fear the additional mirror will degrade sensitivity, or the ability to see faint objects, because photons are lost with each reflection. Cui counters that a new mirror coating developed in the United States promises 98% reflectivity. "There will be no problem" with the additional mirror, she says.

A second point of contention is how quickly the scope can shift from a wide-field survey mode to one that would focus on transient phenomena, such as gamma ray bursts and supernovae. With the complexity of the NIAOT design, astronomers worry the shift would be slow.

Finally, the astronomers want proven technology that will work reliably from the start. They note that LAMOST has fallen short of its primary goal: observing faint galaxies beyond the Milky Way. Cui says the issue is not with the telescope, but with increasing dust and humidity at the site, which now gets only 120 clear nights a year, down from more than 200 when LAMOST was being planned.

After reviewing the NIAOT design, Ma formed a group that began developing a rival design with just two secondary mirrors. The HUST team has received advice from outsiders like Jerry Nelson of the Lick Observatory at the University of California, Santa Cruz, an applied physicist who led the design of the 10-meter Keck telescopes in Hawaii and was the TMT project scientist. "We will be involved as consultants for the telescope and instruments to the extent we are asked," says Nelson, who passed away last week. But Cui, a senior scientist and CAS academician, refused to back down.

To resolve the impasse, the megascience center had an international panel weigh the two alternatives. The nine-member panel, led by Andersen, met in Beijing on 19 and 20 April. Their report, which has been circulated among key personnel but not publicly released, firmly sides with advocates of a simpler design. It calls the mirror coating proposed by the NIAOT team "not yet proven technology" and says that atmospheric turbulence would prevent the image quality in the NIAOT design from living up to hopes. It also says that the telescope would have a hard time switching quickly between surveys and targeting transient objects.

The panel report concludes that the NIAOT optical system "cannot compete" with more standard designs like the HUST approach, "in terms of meeting scientific objectives, providing operational flexibility and keeping within a limited budget." With the panel's recommendation in hand, the megascience center board decided on 19 May to proceed with the HUST design.

Cui is now reportedly lobbying CAS for a second review. But some astronomers are confident CAS will leave the matter in the hands of the megascience team. "We think the debate is over," says Suijian Xue, a vice director of CAS's National Astronomical Observatories in Beijing. He says that getting everyone to work on optimizing the three-mirror system is "the only way to unite the entire community." He also hopes that the bottom-up process the megascience center followed will set a precedent that will help future science projects avoid clashes.


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▲ 取自苏 2017 的论文 The optical system of the proposed Chinese 12-m optical/infrared telescope


http://www.sciencemag.org/news/2017/06/spat-threatens-china-s-plans-build-world-s-largest-telescope
 

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National Astronomical Observatory has made progress in the development of very large CCD controller

After three years of efforts and two rounds of test, one of the key components developed by the ultra-large CCD controller, CCD controller bias and clock drive circuit ASIC, was recently successfully developed by the Chinese Academy of Sciences National Astronomical Optics and Infrared Detector Laboratory.

The National Astronomical Observatory achievements in the CCD controller development technology allows China to reach the international advanced level.

Thus making China independent in the development of ultra-large-scale CCD system.

With the development of optical telescopes of ever larger aperture and larger field of view, the size of the corresponding CCD detectors has increased to billions or even more pixels, which poses a huge challenge to the development of its controllers.

CDA chips development in China of of large-scale CCD controller technology, are now possible, in order to achieve the space station optical telescope, a large optical ground-based infrared telescope (12 meters aperture), the Antarctic large field optical infrared telescope, the ground-based international 30 meters optical infrared telescope and other large CCD control.


2017-09-04

经过历时三年的努力和两轮流片试验,超大型CCD控制器研制的关键元件之一,CCD控制器偏压及时钟驱动电路ASIC,日前在国家天文台天文光学与红外探测器实验室研制成功,从而使得国家天文台在CCD控制器的研制技术上位居国际先进水平,为我国独立研制超大规模的CCD系统奠定了基础。

随着光学望远镜向更大口径和更大视场发展,相应的CCD探测器的规模需求也提高到了十亿、数十亿像元甚至更大,这给其控制器的研制带来了巨大挑战。

CCD探测器要达到天文观测要求的优良性能,除了CCD器件本身性能优异以外,其工作所必需的控制器的性能指标至关重要。经过各国天文探测器技术人员多年努力,天文观测使用的CCD控制器在图像像质指标上已经达到目前技术的极限。然而当CCD像元规模达到数十亿量级时,传统CCD控制器技术却遇到了难以逾越的困难。这是因为以传统技术完成数十亿像元的CCD控制器,仅其体积就将达到数十立方米,更遑论众多模拟量数据通道之间的串扰控制、巨大的功耗以及观测环境的温控等问题。于是,支持数十亿像元及更大规模的CCD控制器技术成为国际上天文光学探测器研制的最大技术难题和技术发展方向。而增加电路的集成度以减小体积,是目前唯一的解决办法。于是,国际上各大天文CCD实验室纷纷开始研制CCD控制器专用集成电路ASIC。

为了满足我国大型天文光学红外望远镜的需要,在国家自然基金和天文财政专项的支持下,在国际知名CCD控制器电子学专家魏名智教授的强有力技术领导下,国家天文台光学与红外探测器实验室开展了CCD探测器ASIC技术的研究。研究方案是CCD控制器的主要电路研制成为两片ASIC芯片,即CCD控制器偏压及时钟驱动电路ASIC(简称CDA)和CCD信号处理电路ASIC(简称为SPA)。自2014年开始,经过三年的研究实验,日前新一轮的CDA流片經实验室测试已经证明完全符合设计要求,从而宣告国家天文台拥有自主知识产权的CCD控制器偏压及时钟驱动专用集成电路CDA研制成功。

CDA芯片提供CCD运行需要的所有电压和驱动脉冲,是CCD控制器必不可少的重要组成部分。此次研制成功的CDA芯片继承了天文CCD控制器中的经典——UCAM控制器的优良性能品质,同时是一个通用性很强的芯片,其灵活性使得它适用于目前世界上绝大多数的CCD芯片和CCD控制器。它可以和正在研制的SPA组成大规模集成化的多CCD系统或超小型的单CCD控制器,也可作为一个部件单独集成到任何一个CCD系统中去。高度集成化使得CCD控制器性能更可靠稳定,功耗,体积更小,並更容易研制。目前这个CDA芯片的版本已經是可供批量生产的版本,很容易进行低成本的重复生产。这就可为国内外科学级CCD系统的研制提供低成本、高性能、高集成度的专用芯片,开辟了新的研发手段。

CDA的研制成功,是我国大型CCD控制器的研制技术的重大进步,为实现空间站光学巡天望远镜、大型光学红外望远镜(12米口径)、南极大视场光学红外望远镜、国际30米光学红外望远镜等大型CCD控制器的研制目标展开了光明前景。


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▲ 此次研究成功的CDA2芯片及其性能测试电路

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▲ CDA和SPA各一片即可替代图中的三块电路板

http://www.bao.ac.cn/xwzx/kydt/201709/t20170904_4854433.html
 

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日前,航天科技集团五院508所承研的地球静止轨道超高分辨率相机进入联调阶段。

此次联调规模非常大,常规相机联调时,电子学设备及配套负载通常为 6~8 台,该次联调则需要同时联调25台电子学设备及其配套负载。

据了解,该型号研制难度非常大,创下多项国内首次,包括首次使用稳像控制技术、首次使用可见光拼接焦面等,其焦面规模是高分四号可见光焦面的9倍:enjoy:

http://www.spacechina.com/n25/n1 ... 725309/content.html

@Bussard Ramjet India? :lol::D
 
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