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How to view the Northern Lights in the U.S. this week
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本周,北极光再次光临,为美国和加拿大边境地区带来了美丽的灯光秀。根据美国国家海洋和大气管理局(NOAA)太空天气预测中心(SWPC)的说法,预计6月1日北极光将出现在美国北部各州。虽然可能持续到6月2日,但届时强度会减弱。观赏极光的机会取决于您所在的地理位置,越往北机会越大。SWPC表示,周日北极光在纽约、威斯康星州和华盛顿州等地都可能可见。本周的北极光是周五太阳表面发生的日冕物质抛射的结果,预计地磁暴将减弱。为了获得最佳观赏效果,建议在晚上10点至凌晨2点之间,在光污染较少的地方观看。

🌌 **极光预测与可见区域**:美国国家海洋和大气管理局(NOAA)预测,6月1日北极光将在美国北部各州出现,并可能持续到6月2日,但强度会减弱。观赏极光的最佳地点是靠近美国和加拿大边境的地区。

💥 **地磁暴的影响**:本次北极光是由周五太阳表面发生的日冕物质抛射引起的。美国国家海洋和大气管理局(NOAA)发布了G4级严重地磁暴警报,预计到周一晚将减弱至G1级。G4级地磁暴可能导致电力系统广泛干扰,而G1级地磁暴的影响较小。

🕰️ **最佳观赏时间和地点**:观赏北极光的最佳时间是晚上10点到凌晨2点,此时地磁活动增强,也是夜间最黑暗的时刻。选择光污染较少的地方观看,例如靠近美国和加拿大边境的认证黑暗天空场所。

The Northern Lights are back once more, heralding summer with a beautiful light show along the U.S.-Canadian border. Here's how to watch the aurora borealis this week.

According to the U.S. National Oceanic and Atmospheric Administration's (NOAA) Space Weather Prediction Center (SWPC), the Northern Lights are expected to appear across northern U.S. states on June 1. The display may linger until June 2, but will be much weaker by then.

As always, your chances of viewing the aurora are better the further north you are. The SWPC states that the Northern Lights may be visible "as low as New York to Wisconsin to Washington state" on Sunday. Those along the U.S.-Canadian border may still be able to catch it on Monday if they're very lucky, however the aurora's area of visibility will have shrunk considerably.

Credit: The National Oceanic and Atmospheric Administration's Space Weather Prediction Center

This aurora borealis is the result of a coronal mass ejection which took place on the Sun's surface on Friday. The SWPC subsequently issued a severe G4 geomagnetic storm alert on Sunday, with conditions expected to weaken to minor G1 storm levels by Monday evening.

According to the NOAA Space Weather Scales, G4 geomagnetic storms can cause issues such as widespread interference with power systems, as well as prolonged disruption of radio and satellite navigation. In contrast, G1 storms may only cause weak power grid fluctuations, and might have a minor impact on satellite operations. Fortunately, the SWPC's warnings give us time to prepare for and mitigate disruptions. 

However, auroras caused by G1 geomagnetic storms can't be seen in as many areas as those caused by more severe storms. While G4 storms have previously produced auroras visible as low as Alabama and northern California, auroras from G1 storms are typically only seen at higher latitudes such as northern Michigan and Maine.

How to get the best view of the Northern Lights

People in the southern hemisphere have already gotten to enjoy their own aurora this week. Credit: Sanka Vidanagama / AFP via Getty Images

As always, you could just head outside at night and look up. Even if you're slightly outside the predicted visible zone, you may as well check since auroras can be visible from over 600 miles away in the right conditions. However, if you would like to optimise your chances of catching the aurora, there are a few factors to consider.

The SWPC states that the best time to see the Northern Lights is between 10 p.m. and 2 a.m., as the level of geomagnetic activity increases during this period. It's also the darkest time of night, which creates a strong contrast with the lights to make the aurora borealis become more visible.

Viewing the aurora borealis from an area with as little light pollution as possible will also help. Some of the best places to view the Northern Lights are likely to be Certified Dark Sky Places close to the U.S.-Canadian border, all of which have been assessed and recognised for having minimal light pollution.

What causes the Northern Lights?

The only difference between the aurora borealis and aurora australis is where they're located. Credit: Sanka Vidanagama / AFP via Getty Images

Auroras are caused by activity on the surface of the Sun, specifically solar flares and coronal mass ejections. During these events, significant amounts of plasma and magnetic field are expelled from the corona, the outermost layer of the Sun's atmosphere.

Such expulsions create a solar wind, which travels through space to reach Earth. How long this takes depends on the type of event it was. While radiation from solar flares is capable of reaching Earth within eight minutes in some circumstances, winds from coronal mass ejections can take hours to days for the same trip.

Once the solar wind reaches Earth, the planet's magnetic field deflects the majority of it back into space. However, some charged ion particles enter the magnetic field instead, travelling to Earth's polar regions where this field is weakest.

These charged ions then collide with oxygen and nitrogen atoms, causing chemical reactions that create the spectacular coloured lights we know as auroras. Both the aurora borealis and aurora australis are caused the same way, the only difference being that the former is in the Northern Hemisphere and the latter is in the Southern Hemisphere.

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北极光 极光观测 地磁暴
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