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Energy Storage and Release through the Solar Activity Cycle: Models Meet Radio Observations
For nearly sixty years, radio observations have provided a unique insight into the physics of the active and quiescent solar atmosphere. Thanks to the variety of emission mechanisms and to the large altitude range available to observations, fundamental plasma parameters have been measured from the l...
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| Lenguaje: | eng |
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Springer
2012
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| Acceso en línea: | https://dx.doi.org/10.1007/978-1-4614-4403-9 http://cds.cern.ch/record/1481603 |