I had wondered if there was a typical size for the filaments based on density or some other parameter.Solar wrote:Perhaps you're confusing the Cosmic version of Intracloud Lightning with the Cosmic version of Clound-to-Ground lightning. On Earth, Intracloud lightning is by far actually the most common form of lighting. Not to be confused with cloud-to-ground lightning.upriver wrote:I found this image of the sun moving through the local chimney. I was looking for the filament connecting the sun to the whatever. If there was a filament connecting from the solar heliosphere what would it connect to? The wall??
http://elpub.wdcb.ru/journals/ijga/gi04 ... 70-o04.gif
http://elpub.wdcb.ru/journals/ijga/gi04 ... #fig04hook
The text for reference you posted is telling you where they think filament is located. The filaments appear to be in the "wall" of The Loop I Superbubble in the first cartoon graphic of your link. There it lay via P. Firsch above - with a question mark - as to whether the filament that the Sun “APPEARS” to be “embedded” within is, or isn’t, a part of the Loop I Superbubble Shell:In this case,the LIC cloud column density towards the star Sirius led to the conclusion that the Sun has entered the LIC cloud within the last 2,000-8,000 years, and that the Sun is about ~0.1 pc from the surface in the downwind direction (Frisch, 1994) When the upper limits of the Ca II column density towards Aql (Vallergra et al., 1993) and the LIC Fe II column density towards Cen (Lallement et al., 1995) are included, then we are forced to conclude that the Sun is located in a filament of difuse interstellar gas with a total thickness <0.7 pc. This filament is illustrated in Figure 4. - LISM STRUCTURE-FRAGMENTED SUPERBUBBLE SHELL?
Obviously, we can't see ourselves like the images assessed in "Characterizing interstellar filaments with Herschel in IC 5146" and nowhere therein is the question being asked "What does it connect to?" The cosmic version of Intracloud Lightning are electric discharges between Cosmic "clouds".
From the article:
"One merit of this scenario is that it provides an explanation for the typical ~0.1 pc width of the filaments as measured with Herschel (Sect. 4 and Fig. 7)"
"In this picture, the postshock thickness of the filaments effectively corresponds to the sonic scale λs at which the 3D turbulent velocity dispersion equals the sound speed (i.e., ℳ(λs) = 1), leading to λ ≈ λs ~ 0.05–0.15 pc according to recent determinations of the linewidth-size relationship in molecular clouds (e.g. Heyer et al. 2009; Federrath et al. 2010)."
So is the filament that the solar system is traveling in, above or below this size?
"the Sun is located in a filament of diffuse interstellar gas with a total thickness <0.7 pc"
So we are in a bigger filament. If it was dual then you could say that each filament was about 3pc with a 1pc space between them... I dont know what spacing is required for Roberts analysis...
Here is a 3D rendering of the Local Bubble..
https://en.wikipedia.org/wiki/Local_Bub ... Bubble.png
Heres an oldy but a goody.
Rotating Elephant Trunks.
http://www.aanda.org/articles/aa/pdf/20 ... 494-05.pdf
If the sun is traveling is a particular direction, for the scenario that Robert is talking about you would want the direction of travel to be axial along the filament. And you would also want a dual filament with a specific twist to
produce the 11(22) year solar cycle. I am thinking that also means that the filament pair has a specific spacing etc..
And probably that the solar cycle has changed many times.
So in trying to find that information out you have to rule out other scenarios. Like a filament going from the wall to the sun.
The position of stars in the local bubble. Not just in filaments. And does each of these have a filament that it travels through or that is connected to it?? What if the sun was traveling across a filament.... What would you expect the light curve to be as it crossed each boundary... Is that even a possibility in EU.
Galaxies embedded in walls have different characteristic than galaxies in bubbles or molecular clouds...
And so what if stars do as well. That luminosity and color depend on its position in the local bubble..
Its almost better to have a model that only depends on the density of the local plasma for its luminosity than to try to depend on the specific geometry of a dual filament. Kind of like a Langmuir Probe heliosphere..