"Remember, if you don't stand up for something, you'll fall for just about anything..."
207 posts
Latest Posts by rapalixi - Page 8
The Star Goddess Nuit
Popping out a butt-plug...
Rapalixi riding a Sky Raft
Safely, far below.
Arcturian Observer, journal & reports
The Four Horsemen of the Apocalypse:
The "Perfect Storm" of stress, oppression & death... squeezing-out that Resurrection, like "gloryfied" toothpaste!
Sonofagun, here we are!
roxy music - avalon
-ax and TOS
The revigorating Novelties of Creativity
Reprise Life's persistently diverse genesis.
Some kind of crows, on the Otherside of the Tree.
Experiential literature as Special FX... to alter consciousness
From a distance, he could see her wallowing in a lifetime of memory meat...
He sobbed silently: "Reason is crazy..."
Crystal Skull,
the "Galactic Signature" of AO Spare
Not only will one get hairy palms, there's the threat of blindness too...
"CIRs are transition zones between fast- and slow-moving streams of solar wind. They contain magnetic fields and shock waves akin to those of CMEs. While CMEs require some sort of explosion on the sun, CIRs do not. They form gently from the sandwiching of solar wind streams--no solar flare required.
The arrival of the CIR on March 8th immediately caused a G1-class (Minor) storm, intensifying to category G2 (Moderate) on March 9th. Sky watchers in Iceland, Canada and multiple US states from New York to Utah saw the geomagnetic glow.
A fast-moving solar wind stream has arrived on the heels of the CIR. This is the same stream that created the CIR in the first place by compressing a region of slower solar wind ahead of it. Blowing almost 600 km/s, the fast stream could cause additional category G1 (Minor) storms on March 10th.. "
Whatever happened to Barnes & Barnes, the "polly polly fish head" guys, from the Dr. Demento Radio Show?
CO-ROTATING INTERACTION REGION: A co-rotating interaction region (CIR) hit Earth on March 8th, setting the stage for a possible G1-class geomagnetic storm. CIRs are transition zones between fast- and slow-moving streams of solar wind. They contain magnetic fields and shock waves akin to those of CMEs.
