03-12-2023

财政部

美联储理事会

联邦存款保险公司

美东时间下午 6:15 发布 

华盛顿特区——财政部长珍妮特·耶伦、联邦储备委员会主席杰罗姆·H·鲍威尔和 FDIC 主席马丁·J·格伦伯格发表了以下声明:

今天,我们正在采取果断行动,通过增强公众对我们银行系统的信心来保护美国经济。 此步骤将确保美国银行系统继续发挥其保护存款的重要作用,并以促进强劲和可持续经济增长的方式为家庭和企业提供信贷渠道。

在收到 FDIC 和美联储董事会的建议并与总统协商后,耶伦国务卿批准采取行动,使 FDIC 能够以充分保护所有储户的方式完成其对加利福尼亚州圣克拉拉硅谷银行的决议 . 从 3 月 13 日星期一开始,储户将可以使用他们所有的钱。与硅谷银行的决议相关的损失不会由纳税人承担。

我们还宣布纽约 Signature Bank 的类似系统性风险情况,该银行今天已被其州特许机构关闭。 该机构的所有存款人都将不受影响。与硅谷银行的决议一样,纳税人不会承担任何损失。

股东和某些无担保债务人将不受保护。 高级管理人员已被免职。 根据法律要求,存款保险基金为支持未投保的存款人而遭受的任何损失,将通过对银行进行特别评估来弥补。

最后,美国联邦储备委员会周日宣布,它将向符合条件的存款机构提供额外资金,以帮助确保银行有能力满足所有存款人的需求。

美国银行体系保持弹性且基础稳固,这在很大程度上归功于金融危机后为确保银行业获得更好保障而进行的改革。 这些改革与今天的行动相结合,表明我们承诺采取必要措施确保储户的储蓄安全。

17,547 thoughts on “国际视角(14)《财政部、美联储和 FDIC 的联合声明》 ”
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    The authors of the study, published May 6 in the journal Monthly Notices of the Royal Astronomical Society, specifically set out to search for Dyson spheres, in the form of infrared heat near stars that couldn’t be explained in any other way.
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    Using historical data from telescopes that pick up infrared signatures, the research team looked at stars located within less than 1,000 light-years from Earth: “We started with a sample of 5 million stars, and we applied filters to try to get rid of as much data contamination as possible,” said lead study author Matias Suazo, a doctoral student in the department of physics and astronomy of Uppsala University in Sweden.

    “So far, we have seven sources that we know are glowing in the infrared but we don’t know why, so they stand out.”
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    There is no conclusive evidence that the seven stars have Dyson spheres around them, Suazo cautioned.

    “It’s difficult for us to find an explanation for these sources, because we don’t have enough data to prove what is the real cause of the infrared glow,” he said. “They could be Dyson spheres, because they behave like our models predict, but they could be something else as well.”

    Among the natural causes that could explain the infrared glow are an unlucky alignment in the observation, with a galaxy in the background overlapping with the star, planetary collisions creating debris, or the fact that the stars may be young and therefore still surrounded by disks of hot debris from which planets would later form.
    The data used by the researchers comes from two active space telescopes — the Wide-field Infrared Survey Explorer, or WISE, from NASA and Gaia from the European Space Agency — as well as an astronomical survey of the sky in infrared light called The Two Micron All Sky Survey. Also known as 2MASS, the collaboration between the University of Massachusetts and the US space agency’s Jet Propulsion Laboratory took place between 1997 and 2001.

  2. Possibilities
    The authors of the study, published May 6 in the journal Monthly Notices of the Royal Astronomical Society, specifically set out to search for Dyson spheres, in the form of infrared heat near stars that couldn’t be explained in any other way.
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    Using historical data from telescopes that pick up infrared signatures, the research team looked at stars located within less than 1,000 light-years from Earth: “We started with a sample of 5 million stars, and we applied filters to try to get rid of as much data contamination as possible,” said lead study author Matias Suazo, a doctoral student in the department of physics and astronomy of Uppsala University in Sweden.

    “So far, we have seven sources that we know are glowing in the infrared but we don’t know why, so they stand out.”
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    There is no conclusive evidence that the seven stars have Dyson spheres around them, Suazo cautioned.

    “It’s difficult for us to find an explanation for these sources, because we don’t have enough data to prove what is the real cause of the infrared glow,” he said. “They could be Dyson spheres, because they behave like our models predict, but they could be something else as well.”

    Among the natural causes that could explain the infrared glow are an unlucky alignment in the observation, with a galaxy in the background overlapping with the star, planetary collisions creating debris, or the fact that the stars may be young and therefore still surrounded by disks of hot debris from which planets would later form.
    The data used by the researchers comes from two active space telescopes — the Wide-field Infrared Survey Explorer, or WISE, from NASA and Gaia from the European Space Agency — as well as an astronomical survey of the sky in infrared light called The Two Micron All Sky Survey. Also known as 2MASS, the collaboration between the University of Massachusetts and the US space agency’s Jet Propulsion Laboratory took place between 1997 and 2001.

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