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	<title>Open Moon Project &#187; Rad hardening of equipment</title>
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		<title>Rad Hardening</title>
		<link>http://openmoonproject.com/electronics-in-space/rad-hardening/</link>
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		<pubDate>Sun, 13 Sep 2009 17:23:00 +0000</pubDate>
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				<category><![CDATA[Electronics in Space]]></category>
		<category><![CDATA[Rad hardening of equipment]]></category>

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		<description><![CDATA[When your computer behaves erratically, mauls your data, or just &#8220;crashes&#8221; completely, it can be frustrating. But for an astronaut trusting a computer to run navigation and life-support systems, computer glitches could be fatal. Unfortunately, the radiation that pervades space can trigger such glitches. When high-speed particles, such as cosmic rays, collide with the microscopic [...]]]></description>
			<content:encoded><![CDATA[<p>When your computer behaves erratically, mauls your data, or just &#8220;crashes&#8221; completely, it can be frustrating. But for an astronaut trusting a computer to run navigation and life-support systems, computer glitches could be fatal.</p>
<p>Unfortunately, the radiation that pervades space can trigger such glitches. When high-speed particles, such as cosmic rays, collide with the microscopic circuitry of computer chips, they can cause chips to make errors. If those errors send the spacecraft flying off in the wrong direction or disrupt the life-support system, it could be bad news.</p>
<p>To ensure safety, most space missions use radiation hardened computer chips. &#8220;Rad-hard&#8221; chips are unlike ordinary chips in many ways. For example, they contain extra transistors that take more energy to switch on and off. Cosmic rays can&#8217;t trigger them so easily. Rad-hard chips continue to do accurate calculations when ordinary chips might &#8220;glitch.&#8221;</p>
<p>NASA relies almost exclusively on these extra-durable chips to make computers space-worthy. But these custom-made chips have some downsides: They&#8217;re expensive, power hungry, and slow &#8212; as much as 10 times slower than an equivalent CPU in a modern consumer desktop PC.</p>
<p>With NASA sending people back to the moon and on to Mars&#8211;see the Vision for Space Exploration&#8211;mission planners would love to give their spacecraft more computing horsepower.</p>
<p>Having more computing power onboard would help spacecraft conserve one of their most limited resources: bandwidth. The bandwidth available for beaming data back to Earth is often a bottleneck, with transmission speeds even slower than old dial-up modems. If the reams of raw data gathered by the spacecraft&#8217;s sensors could be &#8220;crunched&#8221; onboard, scientists could beam back just the results, which would take much less bandwidth. </p>
<p>Objects, particularly spacecraft structures, antennas, solar arrays and other spacecraft equipment,  are shielded against damage from momentary exposure to high energy electromagnetic radiation in the form of high energy optical (laser) radiation or nuclear radiation by a radiation barrier or shield constructed of fibrous silica refractory composite material like that used for the heat shield tiles on the shuttle spacecraft.</p>
<h2><span>Major radiation damage sources</span></h2>
<p>Typical sources of exposure of electronics to ionizing radiation are <a title="Solar wind" href="http://en.wikipedia.org/wiki/Solar_wind">solar wind</a> and the <a title="Van Allen radiation belt" href="http://en.wikipedia.org/wiki/Van_Allen_radiation_belt">Van Allen radiation belts</a> for satellites, <a title="Nuclear reactor" href="http://en.wikipedia.org/wiki/Nuclear_reactor">nuclear reactors</a> in power plants for sensors and control circuits, residual radiation from <a title="Isotope" href="http://en.wikipedia.org/wiki/Isotope">isotopes</a> in <a title="Soft error" href="http://en.wikipedia.org/wiki/Soft_error#Alpha_Particles_from_Package_Decay">chip packaging materials</a>, <a title="Cosmic radiation" href="http://en.wikipedia.org/wiki/Cosmic_radiation">cosmic radiation</a> for both high-altitude airplanes and satellites, and <a title="Nuclear explosion" href="http://en.wikipedia.org/wiki/Nuclear_explosion">nuclear explosions</a> for potentially all military and civilian electronics.</p>
<ul>
<li><a title="Cosmic ray" href="http://en.wikipedia.org/wiki/Cosmic_ray">Cosmic rays</a> come from all directions and consist of approx. 85% <a title="Proton" href="http://en.wikipedia.org/wiki/Proton">protons</a>, 14% <a title="Alpha particle" href="http://en.wikipedia.org/wiki/Alpha_particle">alpha particles</a>, and 1% <a title="Heavy ion" href="http://en.wikipedia.org/wiki/Heavy_ion">heavy ions</a>, together with ultraviolet radiation and x-rays. Most effects are caused by particles with energies between 10<sup>8</sup> and 2*10<sup>10</sup> <a title="Electronvolt" href="http://en.wikipedia.org/wiki/Electronvolt">eV</a>, though there are even particles with energies up to <a title="Oh my god particle" href="http://en.wikipedia.org/wiki/Oh_my_god_particle">10<sup>20</sup> eV</a>. The atmosphere filters most of these, so they are primarily a concern for high-altitude applications like stratospheric jets and satellites.</li>
</ul>
<ul>
<li><a title="Coronal mass ejection" href="http://en.wikipedia.org/wiki/Coronal_mass_ejection">Solar particle events</a> come from the direction of the <a title="Sun" href="http://en.wikipedia.org/wiki/Sun">sun</a> and consist of a large flux of high-energy (several GeV) protons and heavy ions, again accompanied with UV and x-ray radiation. They cause a scale of problems for satellites, ranging from radiation damage to loss of altitude by heating up the upper regions of the atmosphere, causing them to raise up, and decelerating the low-orbit satellites by friction.</li>
</ul>
<ul>
<li><a title="Van Allen radiation belts" href="http://en.wikipedia.org/wiki/Van_Allen_radiation_belts">Van Allen radiation belts</a> contain electrons (up to about 10 MeV) and protons (up to 100s MeV) trapped in the <a title="Geomagnetic field" href="http://en.wikipedia.org/wiki/Geomagnetic_field">geomagnetic field</a>. The particle flux in the regions farther from the Earth can vary wildly depending on the actual conditions of the sun and the <a title="Magnetosphere" href="http://en.wikipedia.org/wiki/Magnetosphere">magnetosphere</a>. Due to their position they pose a concern for satellites.</li>
</ul>
<ul>
<li><a title="Secondary particle (page does not exist)" href="http://en.wikipedia.org/w/index.php?title=Secondary_particle&amp;action=edit&amp;redlink=1">Secondary particles</a> result from interaction of other kinds of radiation with structures around the electronic devices.</li>
</ul>
<ul>
<li><a title="Nuclear reactor" href="http://en.wikipedia.org/wiki/Nuclear_reactor">Nuclear reactors</a> produce <a title="Gamma radiation" href="http://en.wikipedia.org/wiki/Gamma_radiation">gamma radiation</a> and <a title="Neutron radiation" href="http://en.wikipedia.org/wiki/Neutron_radiation">neutron radiation</a> which can affect sensor and control circuits in <a title="Nuclear power plant" href="http://en.wikipedia.org/wiki/Nuclear_power_plant">nuclear power plants</a>.</li>
</ul>
<ul>
<li><a title="Nuclear explosion" href="http://en.wikipedia.org/wiki/Nuclear_explosion">Nuclear explosions</a> produce a short, extremely intense surge of the entire spectrum of electromagnetic radiation, <a title="Electromagnetic pulse" href="http://en.wikipedia.org/wiki/Electromagnetic_pulse">electromagnetic pulse</a> (EMP), <a title="Neutron radiation" href="http://en.wikipedia.org/wiki/Neutron_radiation">neutron radiation</a>, and flux of both primary and secondary charged particles. In case of a <a title="Nuclear warfare" href="http://en.wikipedia.org/wiki/Nuclear_warfare">nuclear war</a> they pose a potential concern for all civilian and military electronics.</li>
</ul>
<ul>
<li><a title="Soft error" href="http://en.wikipedia.org/wiki/Soft_error#Alpha_Particles_from_Package_Decay">Chip packaging materials</a> were an insidious source of radiation that was found to be causing <a title="Soft error" href="http://en.wikipedia.org/wiki/Soft_error">soft errors</a> in new <a title="DRAM" href="http://en.wikipedia.org/wiki/DRAM">DRAM</a> chips in the 1970s. Traces of radioactive elements in the packaging of the chips were producing alpha particles, which were then occasionally discharging some of the capacitors used to store the DRAM data bits. These effects have been reduced today by using purer packaging materials, and employing <a title="Error-correcting code" href="http://en.wikipedia.org/wiki/Error-correcting_code">error-correcting codes</a> to detect and often correct DRAM errors.</li>
</ul>
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