Mashable 03月27日
Spacecraft films unprecedented view of sun shooting particles into space
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欧洲空间局的太阳轨道飞行器(Solar Orbiter)每六个月近距离观测太阳,捕捉到前所未有的太阳风景象。太阳风是太阳持续向太空释放的带电粒子流,对地球和我们的技术有重大影响。研究人员希望了解太阳风的形成和加速机制,从而更好地预测太阳风暴对地球的影响。通过Metis等仪器,科学家们能够观测到太阳内日冕的动态变化,这有助于我们预测潜在的日冕物质抛射(CME)和太阳耀斑,保护我们的电网、卫星和通信基础设施。

💨 太阳轨道飞行器(Solar Orbiter)是欧洲空间局的探测器,每六个月近距离观测太阳,捕捉太阳风的详细信息。通过Metis等仪器,可以观测到太阳风的动态变化。

🌀 太阳风是太阳不断释放的带电粒子流,其速度可超过每小时100万英里。研究太阳风有助于理解太阳活动对地球的影响。

🔥 太阳的日冕温度高达200万华氏度,而其表面温度仅为10,000华氏度。科学家们正试图揭示太阳11年活动周期的驱动因素。

🌍 了解太阳风有助于科学家预测日冕物质抛射(CME)和太阳耀斑何时何地影响地球,从而保护电网、卫星和通信基础设施。

🛡️ 地球的磁场和大气层保护我们免受太阳风暴的有害辐射。准确的太空天气预报可以帮助电力公司采取措施,避免因CME造成的电力激增。

Scientists are still unraveling the mysteries behind our torrid star.

The European Space Agency's Solar Orbiter — which makes a relatively close approach to the sun every six months — has captured an unparalleled view of the solar wind, a stream of charged particles the sun constantly streams into space. The solar wind has great implications for how solar storms impact Earth and our technologies, so researchers seek to understand how it forms and accelerates to speeds exceeding 1 million miles per hour.

"Watch particles whirl out from the Sun in giant, million-km twisters," ESA posted online.

The clip below, which zooms in on this stream of particles from an event in October 2022, was made possible by the spacecraft's coronagraph, called Metis. As you can see, a chronograph blocks the overpowering, luminous sun, allowing the Solar Orbiter to capture the whirling solar wind.

"Metis is currently the only instrument able to see the solar wind's twisting dance," the space agency explained. "No other imaging instrument can see — with a high-enough resolution in both space and time — the sun's inner corona where this dance takes place." The research has been published online in The Astrophysical Journal.

The Solar Orbiter's close observations of the sun also seek to reveal what drives its 11-year-cycle of activity, and why its outer atmosphere, or corona, heats up to some 2 million degrees Fahrenheit, while its surface is dramatically "cooler" at 10,000 F.

Improving our understanding of the solar wind will help scientists better forecast when and where a potent coronal mass ejection (an eruption of a mass of super hot gas) or solar flare may hit Earth and threaten our power grids, satellites, and communications infrastructure. For example, when a CME erupts from the sun's surface, it must travel over 92 million miles to reach Earth. Along the way, this hot gas will "pile up" the solar wind ahead of it, impacting its arrival time at Earth.

Knowledge about these space dynamics is critical: A good space weather forecast would allow power utilities to temporarily shut off power to avoid conducting a power surge from a CME, and potentially blowing out power to millions.

Thankfully, when these events do inevitably impact Earth, our planet's atmosphere and magnetic field protect our bodies from such dangerous radiation.

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太阳风 太阳轨道飞行器 日冕物质抛射 空间天气 太阳物理
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