brantc
Muse
- Joined
- Feb 14, 2009
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I looked at every single image you liked to. All of them. The photosphere is not visible at all in any of those images.
Are you sure?. Its this page right here.
http://www.nasa.gov/centers/marshall/news/news/releases/2010/10-052.html
And then from the corresponding paper.
"The Solar Optical Telescope (SOT) of Hinode (Tsuneta et al. 2008; Suematsu et al. 2008; Shimizu et al. 2008; Ichimoto et al. 2008) makes observations in white light. Its broadband filter imager (BFI) take images in red (668.40 nm, width 0.4 nm), green (555.05 nm, width 0.4 nm) and blue (450.45 nm, width 0.4 nm) continuum ranges. Radiation at these – 3 – wavelengths comes from the photosphere and hence reflects the broadband continuum emission well. However, SOT normally obtains only infrequent images in these filters. More frequently, SOT takes images in the G-band (430.50 nm, width 0.83 nm), formed mainly from CH line opacity. Carlsson et al. (2007) show contribution functions for these filters; the G-band has a photospheric and an upper-photospheric contribution. It therefore serves well to define the morphology of white-light flares and it was also used in the Yohkoh observations (Hudson et al. 1992; Matthews et al. 2003)."
http://arxiv.org/PS_cache/arxiv/pdf/1004/1004.4259v1.pdf
Not every flare has x-rays during the white light flare. Because of the wavelength that HINODE sees at, we know the location of the white light flares which take place on the "ghost limb". We know that the uncertainty is big enough to say that the white light flare could be happening under the photosphere. HINODE cannot place them with only a z observation. You need a limb observation.
The offset is 2 arcseconds not 2 degrees; I already corrected you on this once before (The Solar "Ghost Limb" Is An Optical Artifact IV).
Yep. I keep meaning to say arcseconds.
If the ghost limb is a ghosting of the 1500A band then it is an event taking place at 1500A below the transition layer bleeding into the 1216A channel.
If it is ghosting from the 2 degree wedge in the filter then its either from the upper limb or lower limb. Combine the 2 to get both effects..
Then the only issue with that is the the arc of the curve does not look like its from the transition layer or the true limb (solar surface). And it cant be the transition layer because thats ~192A.
But assuming that it is, if you correct down it is the solar surface, if you correct up then it is the transition layer.
HINODE says its below the transition layer if you consider all these events to be white light flares. So does TRACE at 1216A.
HINODE places such events lower in the solar atmosphere than TRACE does.
A white light flares by definition takes place in the area of the solar atmosphere where that wavelength is visible in "white light".
Right now it appears that the white light flares are very close to photosphere.
I have already said that the footprints of the loops should be visible in white light like an arc lamp. And once we have the ability to place the events on the limb with enough resolution we will see where they are; above or below the photosphere.