The Solar Wind is a torrent of space weather cruising past at 500 — 800 kilometers per second which is around 1.5 million miles per hour or, if you prefer, Mach 2,000.* It’s so powerful it erodes rocks on Mars, ejects particles up high and creates a kind of atmosphere of tiny rock particles which we can study. Then it blows that Martian atmosphere away.
In this new research people realized it was not just the rain of tiny high-speed protons fritzing Mars at 800 km per second that were carving up the rocks — the main role was from the heavy and highly charged He2+. (Now there’s a molecule you don’t see too often).
You might think that a variable torrent of charged particles that are constantly changing speed and direction might have an impact on our atmosphere, but you’d be wrong (or at least, politically incorrect). On Earth the solar wind “just causes the northern lights”. How do we know? We’ve got climate models. In all known GCMs the total global forcing for solar wind is “zero”. Must be true.
Thus and verily the IPCC can conclude that a flow […]
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