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Table 2

Measured characteristics of S and L burst patterns at high resolution, and possible interpretations (see Table 1 for abbreviations used).

Date Time Δ f Source Structure df/dt Quasi- Mechanism? Fig.
(UT) (MHz) type or pattern (MHz/s) period. (Hz) (Ref. N°) No

14 Mar. 2005 01:30:40-41 23.527.5 Io-A QS 16 to 20 1015 1, 3, 6, 9 1a

14 Mar. 2005 01:30:40-41 2627.5 Io-A MS 20 to 32 3, 4, 8 1a, d
14 Mar. 2005 01:30:40-41 2627.7 Io-A QS within MS ~16 1, 3, 6, 9 1d
14 Mar. 2005 00:49:49-56 1732 Io-A L (FF) 7 1b
13 Mar. 2004 18:28:58-59 2024.3 Io-B QS, shadow edges (FF) 16 to 20 1015 1, 3, 6, 9? 1c
13 Mar. 2004 18:28:58-59 18.824 Io-B Shadows on L (FF) 16 to 20 ~10 2 1c
13 Mar. 2004 18:28:58-59 18.820 Io-B QS (FF) 10 to 20 6070 1, 3, 6, 9 1c
13 Mar. 2004 18:28:58-59 ~2024 Io-B Forking QS 16 to 20 ~100 ? 1c
at shadow edges
15 Mar. 2005 2:27:26-27 1624 Io-B LS (FF) ~5 6070 7 2a
14 Mar. 2005 1:27:41-43 1626 Io-A LS (FF) ~5 6070 7 2bd
14 Mar. 2005 1:27:41-43 ~24.530 Io-A QS (FF) 16 1030 1, 3, 6, 9 2bd
30 Oct. 2008 15:52:06-07 1420 Io-A QS (FF) 13 to 20 ~10 1, 3, 6, 9 3a
30 Oct. 2008 15:52:06-07 1420 Io-A Shadows on L (FF) 13 to 20 ~10 2 3a
30 Oct. 2008 15:52:06-07 1420 Io-A QS, shadow edges 13 to 20 ~100 ? 1, 3, 6, 9? 3a
30 Oct. 2008 15:52:06-07 2024.5 Io-B MS envelope (FF) 16 to 30 <10 3, 4, 8 3a
30 Oct. 2008 15:52:06-07 16.316.6 Io-B NB, LS 5 >100 3, 9? 3a, b
30 Oct. 2008 15:46:48-49 20.525.5 Io-B MS envelope (FF) 24 to 40 1015 3, 4, 8 5a
or >0
30 Oct. 2008 15:46:48-49 20.525.5 Io-B QS within MS 20 100 1, 3, 6, 9 5bd
30 Oct. 2008 16:00:32-34 16.529.5 IoB QS at shadow edges (FF) 16 2030 1, 3, 6, 9? 6a
30 Oct. 2008 16:00:32-34 16.529.5 Io-B Shadows on L (FF) 16 2030 2 6a
30 Oct. 2008 16:00:32-34 16.529.5 Io-B QS at shadow edges 19 >100 1, 3, 6, 9? 6b
30 Oct. 2008 16:26:0910 16.532.5 Io-B FS fat bursts (FF) 32 30 2, 5 7a
30 Oct. 2008 16:26:09-10 2731.5 Io-B Forking QS (FF) 17 to 19 ~30 ? 7a, b

Reference. (1) CMI + adiabatic keV electrons (Ellis 1965); (2) CMI absorption (Gopalswamy 1986); (3) Disruption of current filaments (Ryabov 1994); (4) Phase bunching and interaction region (Willes 2002); (5) CMI + Alfvén wave trains (Hess et al. 2007b); (6) CMI + Alfvén waves and potential drops (Hess et al. 2009b); (7) CMI in large-scale cavities (Mottez et al. 2010); (8) Wave propagation in disturbed medium (Shaposhnikov et al. 2011); (9) CMI in electron holes (Treumann et al. 2012). (FF) = Faraday fringes, is a simple modulation due to propagation, superimposed on the emissions.

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