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 | 23.5−27.5 | Io-A | QS | −16 to −20 | 10−15 | 1, 3, 6, 9 | 1a |
|
||||||||
14 Mar. 2005 | 01:30:40-41 | 26−27.5 | Io-A | MS | −20 to −32 | – | 3, 4, 8 | 1a, d |
14 Mar. 2005 | 01:30:40-41 | 26−27.7 | Io-A | QS within MS | ~−16 | – | 1, 3, 6, 9 | 1d |
14 Mar. 2005 | 00:49:49-56 | 17−32 | Io-A | L (FF) | 7 | 1b | ||
13 Mar. 2004 | 18:28:58-59 | 20−24.3 | Io-B | QS, shadow edges (FF) | −16 to −20 | 10−15 | 1, 3, 6, 9? | 1c |
13 Mar. 2004 | 18:28:58-59 | 18.8−24 | Io-B | Shadows on L (FF) | −16 to −20 | ~10 | 2 | 1c |
13 Mar. 2004 | 18:28:58-59 | 18.8−20 | Io-B | QS (FF) | −10 to −20 | 60−70 | 1, 3, 6, 9 | 1c |
13 Mar. 2004 | 18:28:58-59 | ~20−24 | Io-B | Forking QS | −16 to −20 | ~100 | ? | 1c |
at shadow edges | ||||||||
15 Mar. 2005 | 2:27:26-27 | 16−24 | Io-B | LS (FF) | ~−5 | 60−70 | 7 | 2a |
14 Mar. 2005 | 1:27:41-43 | 16−26 | Io-A | LS (FF) | ~−5 | 60−70 | 7 | 2b−d |
14 Mar. 2005 | 1:27:41-43 | ~24.5−30 | Io-A | QS (FF) | −16 | 10−30 | 1, 3, 6, 9 | 2b−d |
30 Oct. 2008 | 15:52:06-07 | 14−20 | Io-A | QS (FF) | −13 to −20 | ~10 | 1, 3, 6, 9 | 3a |
30 Oct. 2008 | 15:52:06-07 | 14−20 | Io-A | Shadows on L (FF) | −13 to −20 | ~10 | 2 | 3a |
30 Oct. 2008 | 15:52:06-07 | 14−20 | Io-A | QS, shadow edges | −13 to −20 | ~100 ? | 1, 3, 6, 9? | 3a |
30 Oct. 2008 | 15:52:06-07 | 20−24.5 | Io-B | MS envelope (FF) | −16 to −30 | <10 | 3, 4, 8 | 3a |
30 Oct. 2008 | 15:52:06-07 | 16.3−16.6 | Io-B | NB, LS | −5 | >100 | 3, 9? | 3a, b |
30 Oct. 2008 | 15:46:48-49 | 20.5−25.5 | Io-B | MS envelope (FF) | −24 to −40 | 10−15 | 3, 4, 8 | 5a |
or >0 | ||||||||
30 Oct. 2008 | 15:46:48-49 | 20.5−25.5 | Io-B | QS within MS | −20 | ≫100 | 1, 3, 6, 9 | 5b−d |
30 Oct. 2008 | 16:00:32-34 | 16.5−29.5 | Io−B | QS at shadow edges (FF) | −16 | 20−30 | 1, 3, 6, 9? | 6a |
30 Oct. 2008 | 16:00:32-34 | 16.5−29.5 | Io-B | Shadows on L (FF) | −16 | 20−30 | 2 | 6a |
30 Oct. 2008 | 16:00:32-34 | 16.5−29.5 | Io-B | QS at shadow edges | −19 | >100 | 1, 3, 6, 9? | 6b |
30 Oct. 2008 | 16:26:09−10 | 16.5−32.5 | Io-B | FS fat bursts (FF) | −32 | 30 | 2, 5 | 7a |
30 Oct. 2008 | 16:26:09-10 | 27−31.5 | 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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