image source: http://farm3.static.flickr.com/2386/1573364449_f54ed8f4e4.jpgThat must have been quite a spectacle.
There was a massive cme well over a decade ago and it was pure bright green.The Curtain sheet flapping effect was incredible.
Here are current facts about the Northern lights.
Letters to Nature
Nature 410, 557-560 (29 March 2001) | doi:10.1038/35069018; Received 7 June 2000; Accepted 12 December 2000
Rapid magnetic reconnection in the Earth's magnetosphere mediated by whistler waves
X. H. Deng and H. Matsumoto
[Quote]
Radio Science Center for Space and Atmosphere, Kyoto University, Uji, Kyoto 611-0011, Japan
Correspondence to: H. Matsumoto Correspondence and requests for materials should be addressed to H.M. (e-mail: Email:
matsumot@kurasc.kyoto-u.ac.jp).
Top of pageMagnetic reconnection has a crucial role in a variety of plasma environments1, 2, 3 in providing a mechanism for the fast release of stored
magnetic energy. During reconnection the plasma forms a 'magnetic nozzle', like the nozzle of a hose, and the rate is controlled by how fast plasma
can flow out of the nozzle. But the traditional picture of reconnection has been unable to explain satisfactorily the short timescales associated with
the energy release, because the flow is mediated by heavy ions with a slow resultant velocity. Recent theoretical work4, 5, 6 has suggested that the
energy release is instead mediated by electrons in waves called 'whistlers', (Whistle ) which move much faster for a given perturbation of the
magnetic field because of their smaller mass. Moreover, the whistler velocity and associated plasma velocity both increase as the 'nozzle' becomes
narrower. A narrower nozzle therefore no longer reduces the total plasma flow—the outflow is independent of the size of the nozzle. Here we report
observations demonstrating that reconnection in the magnetosphere is driven by whistlers, in good agreement with the theoretical
predictions.
