February 2007

Cosmic Rays, Solar Flux and Global Warming

A Danish scientist, Henrik Svensmark, Director of the Center for Sun-Climate Research of the Danish National Space Center in Copenhagen, has conducted experiments and studies to validate his theory that interstellar galactic cosmic rays may have a considerable effect on global climate.

Right: Cosmic rays affect global cloud cover

The theory is that when cosmic rays hit the Earth’s atmosphere, they speed up the process where ions combine with sulphuric acid. These combine to form condensation nucleii, or tiny specs of matter that allow water droplets to form. The widespread condensation of water droplets accumulate to form lower-atmospheric clouds, which serve to reflect sunlight back into space and allow the Earth’s surface to cool off. In the absence of heavy cosmic radiation, fewer clouds form and the surface of the planet heats up again.

The Sun affects cosmic rays entering into the Earth’s atmosphere by virtue of particle emission (solar winds) and solar magnetic flux — when particle emission and the magnetic field is strong due to high solar activity, cosmic rays are deflected away and thus allow fewer clouds to form.

Svensmark concludes “it now seems clear that stellar winds and magnetism are crucial factors in the origin and viability of life on wet earth-like planets,” as are “ever-changing galactic environments and star-formation rates.” When you consider the context of this galactic radiation effect, the impact of CO2 emissions caused by humanity literally fade away into climatic insignificance.”

References:

CO2 ScienceCosmoclimatology: A New Perspective on Global Warming

Telegraph.co.ukCosmic rays blamed for global warming

Thanks to my colleague Rick for bringing this to my attention.

Assymetrical Solar Polar Mystery

solar magnetic fieldTo see is to know — that’s an old science and engineering principle that has been around for most of the history of human technological progress. If you hypothesize you can develop a theory about a topic. If you have a theory, it isn’t much good unless you test it. Testing, it seems, isn’t always easy nor is it infallible. And once in a while, when testing your theories, you come up with a real head-scratcher. Like why is the Sun’s south pole cooler than it’s north pole? Why does that hold true regardless of the solar magnetic field’s north-south orientation?

Image: Ulysses and the Solar Magnetic Field (click image for full-size view) ESA Solar Image Gallery

I know, I know! It must be industrial pollution on planet Earth and greenhouse gasses . . . well, maybe Al Gore can explain it better.

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More Tulips

A couple of days ago I showed a photo of some crimson tulips. Today, I took this photo of a tulip indoors in a vase. The morning sunlight was muted by passing clouds to give this beautiful pastel pink over white effect.

pink tulip

Rapid Fire

Today was a fun day at the shooting range — Damsel is getting really good at emptying the magazine in her 20 gauge Remington 870 in just a couple of seconds. She maintains good accuracy also.

SOHO Captures First Complete Solar Cycle


2007 SOHO EIT IMAGE

1997 SOHO EIT IMAGE

SOHO moves around the Sun in step with the Earth, by slowly orbiting around the First Lagrangian Point (L1), where the combined gravity of the Earth and Sun keep SOHO in an orbit locked to the Earth-Sun line. The L1 point is approximately 1.5 million kilometers away from Earth (about four times the distance of the Moon), in the direction of the Sun. From that vantage point, SOHO’s Extreme ultraviolet Imaging Telescope (EIT) has enjoyed an uninterrupted view of our daylight star for the last eleven-plus years. All previous solar observatories have orbited the Earth, from where their observations were periodically interrupted as our planet `eclipsed’ the Sun.

SOHO’s Pick of the Week featured this remarkable milestone:

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