Length scales for September 14, 2005 solar noise storm |
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| Authors: | Adolfo L Méndez Berhondo Ramón E Rodríguez Taboada Paolo Zlobec Ana K Díaz Rodríguez |
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| Institution: | 1. Astronomy Department, Institute of Geophysics and Astronomy, Calle 212, No. 2906, La Lisa CP 11 600, La Habana, Cuba;2. INAF – Trieste Astronomical Observatory, Via G.B. Tiepolo 11, CP 34131 Trieste, Italy |
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| Abstract: | Source length scales are estimated for the September 14, 2005 solar noise storm from the spectral and temporal observed characteristics of the background continuum fluctuations and clusters of Type I bursts. The characteristic height of the magnetic structure where the noise storm source is located and the size of the source where Type I bursts clustering takes place were calculated. A lower limit for the height of the magnetic structure supporting the noise storm at 237 MHz was estimated too. |
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| Keywords: | Solar radio emission Solar noise storms Type I bursts |
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