Solar Storm Threat Analysis - Impact
Solar Storm Threat Analysis - Impact
Solar Storm Threat Analysis - Impact
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
<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