Some types of documents include conference papers, research reports, meeting papers, journal articles and more.

SEEs can occur at any time during the mission—they are just as probable at the beginning of the mission as at the end (known as Poisson processes). Earth’s geomagnetic field provides shielding against incident GCRs (and solar energetic particles) because it can effectively deflect the lower-energy particles.


Spacecraft must operate in an environment with pervasive radiation consisting of a mixture of particles that, depending on the location, can vary only negligibly in intensity over many years or change intensity by many factors in as fast as a few hours. Space Radiation Effects on Electronics presented by Kenneth A. LaBel at 2004 MRS Fall Meeting, Boston, MA – Nov 29, 2004 Radiation Effects on Electronics and the Space Environment • Three portions of the natural space environment contribute to the radiation hazard – Solar particles • Protons and heavier ions – SEE, TID, DD – Free-space particles

Images from our SDO show the flare in 3 different wavelengths: https://go.nasa.gov/3iZWEKo, A special type of aurora that drapes across the night sky like a glowing pearl necklace — called auroral beads — is helping scientists uncover complex processes in near-Earth space. https://www.intel.com/content/dam/www/programmable/us/en/pdfs/literature/wp/wp-01207-single-event-functional-interrupt.pdf, https://radhome.gsfc.nasa.gov/radhome/papers/SEEspec.pdf, Troubleshooting of a software running on satellites, Redundancy and its types in computer systems.

Figure 2.1 summarizes the general types of space radiation and where they are relevant.

As Box 2.1 explains, when a single particle passes through an electronic component, it ionizes atoms and generates small amounts of free charge.

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As a result, satellites may experience shortened lifetimes, major failures or even complete “destruction”. The results of these studies are then used to either modify the design or make use of mitigation techniques, such as radiation shielding to limit the impact of the environment. Total ionizing dose (TID) is mainly an issue at end of life for the spacecraft, and TID failures are often (although not always) preceded by gradual degradation. Lieferung verfolgen oder Bestellung anzeigen, Recycling (einschließlich Entsorgung von Elektro- & Elektronikaltgeräten). Bit flips are usually reversible by rewriting affected memory, but sometimes the damage is persistent – very small MOS transistors may be set by a single particle in the fixed state forever, the effect is named Single Event Hard (SEH) or stuck bit failure. cases revertible. ...or use these buttons to go back to the previous chapter or skip to the next one. 0000012301 00000 n When a MOSFET is turned off, the source has a high voltage. Anomalies can occur at any time in the solar cycle, and SEEs are a major root cause.

Turbulence in the field (such as that associated with solar maximum) makes propagation of GCRs into the inner solar system more difficult—the particles are scattered more effectively. Jump up to the previous page or down to the next one. If that charge collects within the component in a way that mimics or disrupts the normal operation of the device, then a spurious outcome is possible. 0000001443 00000 n A High voltage is a necessary condition for SEB. 0000011642 00000 n

Galactic cosmic rays are primarily protons and ionized heavy nuclei of galactic and/or extragalactic origin with energies ranging from ~1 MeV/nucleon to more than ~10,000 MeV/nucleon. Außerdem analysiert es Rezensionen, um die Vertrauenswürdigkeit zu überprüfen. In contrast, solar particle events (SPEs) are periods of significantly enhanced fluxes of particles (solar energetic particles, or SEPs) accelerated to high energies by solar electromagnetic fields and associated with periods of high solar activity. 0000014431 00000 n Failures caused by absorbed doses can be dealt with by component selection, layout adjustment and addition of absorber.

This applies especially to component selection and circuit design. Today I'll be talking about cosmic radiation effects on electronics, and how to pick the right parts for your space application. View our suggested citation for this chapter.

External electric field moves electrons and holes in opposite directions along the direction of the field. Having discussed the space radiation environment and its effect on electronics, in Chapter 3 the focus is on how spacecraft designers and component manufacturers assure the radiation hardening of electronics via testing at various facilities throughout the United States and a discussion of those facilities.
SEEs can occur at any point in a mission and in all space environments when a charged particle traverses a sensitive volume in an active semiconductor device, depositing sufficient charge to disrupt the normal functionality of that device (see Box 2.1). 0000001843 00000 n 0000004086 00000 n

First, beta radiation has little, if any, effect on electrical equipment because this type of ionizing radiation is easily shielded. The inner belt extends from hundreds of kilometers to ~6,000 km in altitude and is populated by high-energy protons (tens of MeV) and high-energy electrons (1–10 MeV), while the outer belt, up to 60,000 km in altitude, is predominately high-energy electrons. 9.3 How to find radiation and reliability reports on TI.com?

of the space radiation on electronic devices are the limits in shielding effectiveness for high-energy electrons, protons, and cosmic rays. Depending on the part’s technology and particular SEE mode, the result can be the following: Spacecraft depend on electronic components that must perform reliably over missions measured in years and decades. The Sun continually emits a “solar wind” of charged particles with kinetic energies largely between 1 eV to 10,000 electron volts (10 keV) that move radially away from the Sun at densities on the order of 10 particles per cubic centimeter superimposed on the background solar wind are high-energy particle bursts.

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