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Magnetospheric electric convection field Wikipedia audio article
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This is an audio version of the Wikipedia Article: • https://en.wikipedia.org/wiki/Magneto... • • • 00:00:56 1 Model Description • 00:01:25 2 Inner Magnetosphere • 00:01:36 3 Origin of Convection Field • 00:03:38 4 Polar Magnetosphere • 00:06:12 5 See also • 00:07:25 6 Literature • 00:10:14 See also • 00:10:26 Literature • • • • Listening is a more natural way of learning, when compared to reading. Written language only began at around 3200 BC, but spoken language has existed long ago. • • Learning by listening is a great way to: • increases imagination and understanding • improves your listening skills • improves your own spoken accent • learn while on the move • reduce eye strain • • Now learn the vast amount of general knowledge available on Wikipedia through audio (audio article). You could even learn subconsciously by playing the audio while you are sleeping! If you are planning to listen a lot, you could try using a bone conduction headphone, or a standard speaker instead of an earphone. • • Listen on Google Assistant through Extra Audio: • https://assistant.google.com/services... • Other Wikipedia audio articles at: • https://www.youtube.com/results?searc... • Upload your own Wikipedia articles through: • https://github.com/nodef/wikipedia-tts • Speaking Rate: 0.9087923329392681 • Voice name: en-US-Wavenet-A • • • I cannot teach anybody anything, I can only make them think. • Socrates • • • SUMMARY • ======= • The impact of the solar wind onto the magnetosphere generates an electric field within the inner magnetosphere (r 10 a; with a the Earth's radius) - the convection • field-. Its general direction is from dawn to dusk. The co-rotating thermal plasma within • the inner magnetosphere drifts orthogonal to that field and to the geomagnetic field Bo. The generation process is not yet completely understood. One possibility is viscous interaction between solar wind and the boundary layer of the magnetosphere (magnetopause). Another process may be magnetic reconnection. Finally, a hydromagnetic dynamo process in the polar regions of the inner magnetosphere may be possible. Direct measurements via satellites have given a fairly good picture of the structure of that field. A number of models of that field exists.A widely used model is the Volland-Stern model
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