中國(guó)科技網(wǎng)6月10日?qǐng)?bào)道（張微 編譯）能夠影響GPS和電網(wǎng)技術(shù)的，來(lái)自太陽(yáng)的大型磁暴，可能很快就會(huì)提前24小時(shí)得到預(yù)報(bào)。

　　日冕物質(zhì)拋射(CME)是從太陽(yáng)中噴發(fā)出的氣體和磁性物質(zhì)，有可能破壞衛(wèi)星和地面技術(shù)，干擾無(wú)線電傳輸，導(dǎo)致變壓器泄露和停電。

　　這些拋射物質(zhì)能夠引發(fā)GPS技術(shù)的諸多問(wèn)題，而GPS技術(shù)在包括汽車到油輪到拖拉機(jī)的各種交通工具上有著廣泛的應(yīng)用。例如，它們可以影響飛機(jī)系統(tǒng)在著陸時(shí)精確判斷飛機(jī)與地面距離的能力，導(dǎo)致飛機(jī)長(zhǎng)達(dá)一個(gè)小時(shí)沒(méi)法著陸。

　　但是，并不是從太陽(yáng)到地球的每種拋射物質(zhì)都能對(duì)地球造成這么多的干擾;這種力量取決于拋射物質(zhì)中的磁場(chǎng)方向。目前，衛(wèi)星只能在拋射物質(zhì)接近地球的時(shí)候，才能明確地辨識(shí)出日冕物質(zhì)拋射的磁場(chǎng)方向，發(fā)出一個(gè)30-60分鐘的通知。這點(diǎn)時(shí)間不足以減輕對(duì)電網(wǎng)和GPS操作系統(tǒng)的影響。

　　現(xiàn)在，一個(gè)新的測(cè)量和建模工具可以提前24小時(shí)通知對(duì)地球有害的拋射物質(zhì)到達(dá)地球的時(shí)間。倫敦帝國(guó)理工學(xué)院的校友和客座研究員，同時(shí)也是美國(guó)宇航局戈達(dá)德太空飛行中心的一位太空科學(xué)家尼爾 薩瓦尼博士領(lǐng)導(dǎo)的研究團(tuán)隊(duì)開(kāi)發(fā)了這項(xiàng)技術(shù)，研究成果發(fā)表在今天出版的《Space Weather》期刊上。

　　“當(dāng)越來(lái)越多的技術(shù)融合和集成在一起的時(shí)候，太空天氣事件的干擾就會(huì)越來(lái)越多地影響我們的日常生活，”薩瓦尼博士說(shuō)。“打破24小時(shí)預(yù)測(cè)瓶頸對(duì)于有效處理潛在的問(wèn)題非常重要。”

　　日冕物質(zhì)拋射的磁場(chǎng)方向取決于兩件事情：它們從太陽(yáng)噴發(fā)出來(lái)的最初形態(tài)，以及它們奔向地球過(guò)程中的演變。日冕物質(zhì)拋射來(lái)自于太陽(yáng)表面的兩個(gè)區(qū)域，在拋射向太空和太陽(yáng)表面之間形成一個(gè)牛角包狀的一團(tuán)日冕物質(zhì)。

　　隨著日冕物質(zhì)的移動(dòng)，里面的磁場(chǎng)方向也在發(fā)生改變。如果其中一個(gè)磁場(chǎng)與地球磁場(chǎng)的方向相同，那么兩個(gè)磁場(chǎng)就會(huì)連接，“打開(kāi)一扇門”讓這些物質(zhì)到達(dá)地球并引起地磁風(fēng)暴。

　　此前，預(yù)測(cè)依賴于測(cè)量初始CME的爆發(fā)，但是對(duì)于CME爆發(fā)和日冕物質(zhì)到達(dá)地球過(guò)程中的情況沒(méi)有有效地建模。這項(xiàng)新技術(shù)仔細(xì)調(diào)查了日冕物質(zhì)來(lái)自太陽(yáng)的具體位置，利用一系列的觀測(cè)來(lái)追蹤和建模日冕物質(zhì)的演變。

　　薩瓦尼博士和他的同事根據(jù)之前的八次日冕物質(zhì)拋射情況，對(duì)該模型進(jìn)行了測(cè)試，結(jié)果顯示，對(duì)于改善目前影響地球的太陽(yáng)風(fēng)暴預(yù)測(cè)系統(tǒng)帶來(lái)了巨大希望。如果美國(guó)宇航局支持進(jìn)行進(jìn)一步的測(cè)試，那么這個(gè)系統(tǒng)將很快在美國(guó)國(guó)家海洋和大氣管理局以及英國(guó)氣象局的地磁風(fēng)暴預(yù)測(cè)中得到應(yīng)用。

　　New tool could predict large solar storms more than 24 hours in advance

　　Large magnetic storms from the Sun, which affect technologies such as GPS and utility grids, could soon be predicted more than 24 hours in advance.

　　Coronal mass ejections (CMEs) are eruptions of gas and magnetised material from the Sun that have the potential to wreak havoc on satellites and Earth-bound technologies, disrupting radio transmissions and causing transformer blowouts and blackouts.

　　These mass ejections can cause problems with GPS technology - used by all kinds of vehicles, from cars to oil tankers to tractors. For example, they can affect the ability of aircraft systems to judge precisely a plane\'s distance from the ground for landing, leading to planes being unable to land for up to an hour.

　　However, not every mass ejection from the Sun that travels past the Earth causes this much disturbance; the power depends on the orientation of magnetic fields within the mass ejection. Currently, satellites can only tell the orientation of a mass ejection\'s magnetic field with any certainty when it is relatively close to the Earth, giving just 30-60 minutes\' notice. This is not enough time to mitigate the impacts on utility grids and systems operating on GPS.

　　Now, a new measurement and modelling tool could give more than 24 hours\' notice of mass ejections that could be harmful to systems on Earth. Details of the technique, developed by a team led by Dr Neel Savani, an alumnus and Visiting Researcher at Imperial College London and a space scientist at NASA\'s Goddard Space Flight Center, were published today in a paper in Space Weather.

　　"As we become more entwined with technology, disruption from large space weather events affects our daily lives more and more," said Dr Savani. "Breaking through that 24 hour barrier to prediction is crucial for dealing efficiently with any potential problems before they arise."

　　The orientations of magnetic fields within coronal mass ejections depend on two things: their initial form as they are erupted from the Sun, and their evolution as they travel towards Earth. Mass ejections originate from two points on the Sun\'s surface, forming a croissant-shaped cloud in between that discharges into space.

     This cloud is full of twisted magnetic fields that shift as they travel. If one of these magnetic fields meets the Earth\'s magnetic field at a certain orientation, the two will connect, \'opening a door\' that allows material to enter and cause a geomagnetic storm.

　　Previously, predictions had relied on measuring the initial CME eruption, but were not efficient modelling what happened between this and the cloud\'s arrival at Earth. The new technique takes a closer look at where mass ejections originate from on the Sun and makes use of a range of observatories to track and model the evolution of the cloud.

　　Dr Savani and colleagues have tested the model on eight previous mass ejections, with the results showing great promise at improving the current forecasting system for large Earth-directed Solar storms. If further testing at NASA supports these initial results, the system could soon be used by NOAA in the US and the Met Office in the UK for geomagnetic storm predictions.