Prominences a bit subdued this morning.
This is the last solar post for a while as we are off to Scotland for 2 1/2 weeks.
I have wondered about the resolution I get with my solar scope, so here are some fag-packet calculations:
Telescope diffraction limit (in radians)= 1.22 X wavelength in cm/scope dia. in cm
Telescope diffraction limit (in arcseconds)= 206265 X 1.22 X wavelength in cm/scope dia. in cm
Ha light wavelength = 6562 angstroms = 6562 X 10^-8 cm
Lunt LS35 THa is 3.5 cm dia
Diffraction limit = (206265 X 1.22 X 6562 X 10^-8)/3.5
= 4.7 seconds, or about 5
Solar diameter is around 30 arcminutes, or about 1800 arcseconds
In this image the distance between the 2 spots is around 0.135 X the solar diameter, or around 250 arcseconds
The lines or striations around spot 2620 at their thinnest, are around 1/50th of this distance, or around 5 arcseconds.
So. my Lunt LS35THa images could, in fact be diffraction limited!
The GONG cameras have an aperture of 2.8cm, so they are similar.
Conclusion, to get images like this one (http://spaceweathergallery.com/indiv_upload.php?upload_id=147458)
Of course, a Quark fitted to a 80mm scope should be pretty good! (Andy)
Sunspot 2720 has now appeared and seems to be developing quite rapidly.
“New sunspot AR2720 is not only large, but also strange. Its magnetic polarity is reversed. The North and South ends of its enormous magnetic field are backwards compared to the norm for sunspots in the current solar cycle, decaying Solar Cycle 24. Could AR2720 be the first big sunspot of the next solar cycle, Solar Cycle 25, popping up now in the middle of solar minimum? Stay tuned for more information about this intriguing possibility after the current geomagnetic storm is over.”!