Solar cycle

It's like, no, you're going to be...

i mean there's solar activity these like these x-class solar flares and all this stuff those are solar flashes those like a like you could say there's a whole bunch of them happening but they're not that right they're just like these kind of like bumping up in consciousness and kind of like empowering things at an internal level more right right

yeah interestingly enough reina says we have a higher dimensional second son

I heard, I believe.

Well, that's

kind of what I've been telling everybody like, okay, well the solar cycle 25 is going to be peaking on, Say those years again, like that's exactly when.

So when we're supposed to be peaking.

So will it peak and just like peak and just keep just like expanding into some magenta color? chakra, like I'm up for it.

Like magenta, you say, like weird and huge, too.

Like when the when the stars do lose some of their energy.

gravity or whatever they do expand in size so that's a maturity thing I think when the like core starts to break down its strength and they've been trying to tell us it's losing its strength the sun I feel like and so I was wondering about the solar cycle like if the sun's losing strength it'll be less powerful than last solar cycle peak which was around 2017-18 I think so we'll see but it might just be it like that might just be it We might just be enjoying a few more Zoom calls just for funsies before 2024 comes around.

So enjoy 2023, everybody.

One thing is in the highest degree probable, namely, that electricity is largely concerned.

Going back to the question of sunspots, regarded in their possible or probable association with the corona, the present position of matters appears to be this, that there is a real connection between the general form of the corona and disturbances on the sun, taking sunspots as an indication of solar activity.

When sunspots are at or near their maximum, the corona has generally been somewhat symmetrical, with synclinal groups of rays making angles of 45 degrees with its general axis.

On the other hand, at the epochs of minimum sunspots, the corona shows polar rifts much more widely open, with synclinal zones making larger angles with the axis, and being, therefore, more depressed towards the equatorial regions, in which, moreover, there is usually a very marked extension of coronal matter in the form of elongated streamers reaching to several diameters of the sun.

This generalization is well borne out by the maximum epoch coronas of 1870 and 1871, and the minimum epoch coronas of 1867, 1874, 1875, 1878, and perhaps 1887 and certainly 1889.

On the other hand, the eclipses of 1883, 1885, and 1886 do not strikingly confirm this theory.

The eclipse of 1883 was at a time of rapidly decreasing solar activity, yet the corona had the features of a sunspot maximum.

The same, though in a somewhat less degree, may be said of the eclipses of 1885 and 1886.