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Solar Storm Threat Analysis - Impact

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<strong>Impact</strong>, 2007 James A. Marusek<br />

Figure 1 attempts to answer the above<br />

question. Using proxy data derived from<br />

nitrate spikes in ice cores on Earth and data<br />

derived from moon rocks, the figure<br />

compares the size of a solar storm (based on<br />

the fluence of high-energy nuclear particles)<br />

with the probability of such an event.<br />

Fluence is a measure of flux rate covering<br />

the complete timeline of a solar storm event.<br />

[As an analogy, fluence would be similar to<br />

the amount of rainfall during a rainstorm,<br />

where flux rate would be similar to the<br />

amount of rainfall per hour.] The diamond<br />

symbol closest to the middle of the graph is<br />

the fluence from the Carrington solar storm<br />

of 1859. The data point on the lowest right<br />

portion of the graph is the largest event<br />

measured using Aluminum and Beryllium<br />

dating from moon rocks. The graph implies<br />

that solar storms with a fluence a million<br />

time greater than the Carrington solar storm<br />

are possible on a scale of approximately<br />

once every million years.<br />

SPEs in solar storms leave behind a nitrate<br />

signature in Polar and Greenland ice cores.<br />

Figure 1. Estimate of the magnitude and<br />

probability of solar storms based on direct observation<br />

from satellites, nitrate spikes in Earth’s ice cores and<br />

analysis of inducted radioactivity in moon rocks. 8<br />

But the burst of Galactic Cosmic Rays (GCRs) from a nearby supernova also leaves behind a nitrate spike in the ice<br />

cores. These two types of signatures are distinct in the ice cores because supernovas produce nitrate spikes of<br />

greater intensity and width (time duration). The induced radioactivity in moon rocks could be caused by SPEs or by<br />

nearby supernovas. It is my opinion that nearby supernovas (within 2,000 light years from Earth) predominate<br />

moon rock signatures and that the sun is fairly limited in its peak intensity range.<br />

C. <strong>Analysis</strong> Structure<br />

An outline of solar storm effects analysis is provided below with a detailed discussion following.<br />

• Induced Currents<br />

o Extensive Power Plant Outages<br />

� Homes<br />

� Transportation<br />

� Banking<br />

� Commerce and Industry<br />

� Other <strong>Impact</strong>s<br />

o Oil and Gas Pipelines<br />

o Long Distant Communication Lines<br />

• Geomagnetic Field Distortion<br />

o Transient Distortions<br />

o Magnetic Pulses<br />

• Nuclear Radiation Exposure<br />

o Individuals<br />

� Scope of <strong>Threat</strong> to Humans<br />

o Spacecraft Electronics<br />

o Air and Ground Based Electronics<br />

• Ionospheric Reflectivity and Scintillation<br />

o Communications<br />

o Radar<br />

o Navigation<br />

5

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