Timeline for Ion acoustic wave regime
Current License: CC BY-SA 3.0
10 events
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Mar 24, 2021 at 22:00 | history | bumped | CommunityBot | This question has answers that may be good or bad; the system has marked it active so that they can be reviewed. | |
Nov 24, 2020 at 15:11 | comment | added | honeste_vivere | I missed something the first time I read this. How do you get an IAW with immobile ions? IAWs are like Langmuir waves but where the ions oscillate in a longitudinal fashion. The electrons serve to counter the ion oscillations to prevent charge accumulation. If just the electrons oscillate, then the real part of the frequency would be near fpe not fpi. These would damp differently than an IAW too. | |
Nov 24, 2020 at 15:02 | history | bumped | CommunityBot | This question has answers that may be good or bad; the system has marked it active so that they can be reviewed. | |
Jun 11, 2020 at 9:33 | history | edited | CommunityBot |
Commonmark migration
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Dec 14, 2017 at 20:07 | history | edited | DanielSank | CC BY-SA 3.0 |
edited title
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Dec 14, 2017 at 18:53 | comment | added | Plasmaths | Thanks! This explains why the influence seen in my figures is almost negligible! | |
Dec 14, 2017 at 18:51 | history | edited | Plasmaths | CC BY-SA 3.0 |
added 87 characters in body
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Dec 14, 2017 at 13:29 | comment | added | honeste_vivere | The original idea behind IAWs was that $T_{e}/T_{i}$ needed to be greater than 3 otherwise the instability that radiates the waves would be suppressed. In the 1970s and 1980s, several authors (e.g., Christian Dum) did a lot of work on this topic and found that the instability dependence on $T_{e}/T_{i}$ could be reduced or even ignored in the presence of electron heat fluxes, temperature gradients, beams, etc. Note that the original concept is horribly flawed in that we never observe single, isotropic Maxwellians for either ions or electrons in space plasmas. | |
Dec 13, 2017 at 19:17 | answer | added | Quantum spaghettification | timeline score: 1 | |
Dec 13, 2017 at 18:04 | history | asked | Plasmaths | CC BY-SA 3.0 |