Browse Topic: Radiation protection

Items (101)
Study on the Influence of the Magnetic Field and the Induced Electrical Field in Human Bodies by EV/PHEV Wireless Charging Systems2016-01-11584/5/2016
Wireless charging systems for electric vehicles (EVs) and plug-in hybrid electric vehicles (PHEVs) employing the resonant magnetic coupling method and using induction coils have been intensively studied in recent years. Since this method requires kW class high power to be transmitted using resonant magnetic coupling in the high frequency range, it is necessary to pay attention to the leakage of the magnetic field generated by the coil current, and to its influence on surrounding objects, particularly human bodies. Noting that acceptable values for human body exposure to electromagnetic fields have previously been issued by the International Commission on Non-Ionizing Radiation Protection (ICNIRP) as guidelines, we have developed a method for predicting product compliance with those guidelines at the basic design development stage. This method calculates the magnetic field generated by the induction coil current and predicts the value of the electric field induced in the human body. Once we calculate the surrounding magnetic field of the vehicle, this method makes it possible to evaluate induced electric field values when a human body is present in various locations. Using this method, we analyzed the magnetic field distribution and electric field of a 3.7 kW charging system operating at a resonant frequency of 85 kHz while taking into consideration induction coil positions under, at the rear, at the center, and in front of the vehicle. The results show that the induced electric field in the human body is much smaller than the basic restrictions imposed by the ICNIRP guidelines.
Watanabe, ToshiakiIshida, Masaya
A versatile, novel, multifunctional hybrid structural composite of a high-hydrogen epoxy matrix (UN-10) coupled with boron and carbon fibers (IM-7) has been developed. Prototype laminates of 18×18 in. (≈46×46 cm), with the nominal areal density of 0.35 g/cm2, were fabricated in this effort. The hydrogen atoms in the epoxy will provide shielding strength against high-energy protons, electrons, and heavy ionic species, while the boron fibers that have a high neutron cross-section will help shield against neutrons and reduce the buildup of high-energy photons from secondary reactions. The carbon fibers will provide improved mechanical strength.
Currently, lead and lead-based materials are used to fabricate shields not only for X-rays, but also for other types of radiation. With the growing environmental concern about the toxicity of lead, and the high costs associated with transporting heavy lead-based shields in spacecraft, alternatives are needed for fabricating X-ray shields that are less toxic and lighter.
Validation of an “Intelligent Mouthguard” Single Event Head Impact Dosimeter2014-22-000111/10/2014
Dating to Colonel John Paul Stapp MD in 1975, scientists have desired to measure live human head impacts with accuracy and precision. But no instrument exists to accurately and precisely quantify single head impact events. Our goal is to develop a practical single event head impact dosimeter known as “Intelligent Mouthguard” and quantify its performance on the benchtop, in vitro and in vivo. In the Intelligent Mouthguard hardware, limited gyroscope bandwidth requires an algorithm-based correction as a function of impact duration. After we apply gyroscope correction algorithm, Intelligent Mouthguard results at time of CG linear acceleration peak correlate to the Reference Hybrid III within our tested range of pulse durations and impact acceleration profiles in American football and Boxing in vitro tests: American football, IMG=1.00REF-1.1g, R2=0.99; maximum time of peak XYZ component imprecision 3.6g and 370rad/s2; maximum time of peak azimuth and elevation imprecision 4.8° and 2.9°; maximum average XYZ component temporal imprecision 3.3g and 390rad/s2. Boxing, IMG=1.00REF-0.9g, R2=0.99, R2=0.98; maximum time of peak XYZ component imprecision 3.9g and 390rad/s2, maximum time of peak azimuth and elevation imprecision 2.9° and 2.1°; average XYZ component temporal imprecision 4.0g and 440rad/s2. In vivo Intelligent Mouthguard true positive head impacts from American football players and amateur boxers have temporal characteristics (first harmonic frequency from 35Hz to 79Hz) within our tested benchtop (first harmonic frequency <180Hz) and in vitro (first harmonic frequency <100Hz) ranges. Our conclusions apply only to situations where the rigid body assumption is valid, sensor-skull coupling is maintained and the ranges of tested parameters and harmonics fall within the boundaries of harmonics validated in vitro. For these situations, Intelligent Mouthguard qualifies as a single event dosimeter in American football and Boxing.
Bartsch, AdamSamorezov, SergeyBenzel, EdwardMiele, VincentBrett, Daniel
The FAA, using its CARI-6 program, provides galactic cosmic radiation dosage rates for any location on the Earth from ground up to 60,000 ft (≈18,300 m). One way to protect astronauts from galactic cosmic radiation (GCR) on a Mars mission is to use material shielding. However, current radiation shielding code does not model shields thicker than about 100 to 200 gm/cm2, and it has been shown that this shield thickness is insufficient to provide protection for a trip to Mars. There is effort underway to extend the code to thicker shields, but there is a lack of experimental data to use to verify the code. The atmosphere represents a very thick and effective radiation shield, and that atmospheric radiation data might be used as a source of verification data.
Acute Radiation Risk and BRYNTRN Organ Dose Projection Graphical User InterfaceTBMG-107618/1/2011
The integration of human space applications risk projection models of organ dose and acute radiation risk has been a key problem. NASA has developed an organ dose projection model using the BRYNTRN with SUM DOSE computer codes, and a probabilistic model of Acute Radiation Risk (ARR). The codes BRYNTRN and SUM DOSE are a Baryon transport code and an output data processing code, respectively. The risk projection models of organ doses and ARR take the output from BRYNTRN as an input to their calculations. With a graphical user interface (GUI) to handle input and output for BRYNTRN, the response models can be connected easily and correctly to BRYNTRN. A GUI for the ARR and BRYNTRN Organ Dose (ARRBOD) projection code provides seamless integration of input and output manipulations, which are required for operations of the ARRBOD modules.The ARRBOD GUI is intended for mission planners, radiation shield designers, space operations in the mission operations directorate (MOD), and space biophysics researchers. BRYNTRN code operation requires extensive input preparation. Only a graphical user interface (GUI) can handle input and output for BRYNTRN to the response models easily and correctly. The purpose of the GUI development for ARRBOD is to provide seamless integration of input and output manipulations for the operations of projection modules (BRYNTRN, SLMDOSE, and the ARR probabilistic response model) in assessing the acute risk and the organ doses of significant Solar Particle Events (SPEs).
Effective Solar Absorptance of Multilayer Insulation2009-01-23927/12/2009
Multi Layer Insulation (MLI) is very commonly used in all spacecraft for heat conservation. In most instances one has to deal with MLI facing space or other cold surfaces while protecting the thermally controlled surface at more moderate temperatures than the heat sink. But in some instances, either in steady state or transient modes, one has to deal with the MLI facing the sun. Examples of such situations are during spacecraft turns, deliberate or inadvertent, when the MLI is exposed to solar insolation for short or extended periods. The effective emittance of MLI is commonly used to describe its heat loss behavior in the absence of solar incidence and is well documented in widespread literature based on measurements and rules of thumb from practice. However, when MLI faces the sun, its effective solar absorptance comes into play to determine its effectiveness in controlling the temperature of the object that it was designed to protect thermally. The heat loss from the controlled object is different when it is absorbing solar energy on the MLI's external surface versus when it is not. The effective absorptance of MLI then simply is this difference in the heat loss flux of the MLI as a fraction of the incident solar flux. This is where it is analogous to the effective emittance of MLI and provides a simple metric of the MLI's performance when exposed to the sun. Knowledge of the effective solar absorptance, just like the effective emissivity of MLI, allows for a simple accounting for the effect of solar incidence on the MLI's performance for thermal design and analysis. Since MLI is not simply a series of radiation shields with only radiation between them but also has heat transfer by conduction due to thermal contact between them, the effective absorptance cannot be easily characterized due to the non-linear complicated thermal coupling between the innermost and outermost layers. In this paper the effective solar absorptance of MLI is estimated analytically by utilizing the following three known properties of the MLI: effective emittance of the MLI blanket and the emissivity/absorptivity of the outermost surface of the blanket. Two ways of making these estimates are presented in this paper and discussed in detail. The first way is bounding in nature by using two extreme assumptions to bracket the estimates: pure radiation or pure conduction between the innermost and outermost layers. A generalized relationship between the two extreme estimates as a function of the MLI's intrinsic properties (effective emittance, external layer emissivity an absorptivity) is presented, along with range of applicability, general trends and rules of thumb. The second method is more rigorous which uses standard equations that break down the radiative and conductive components of heat flow through MLI which are based on measurements of MLI heat losses and effective emissivity as a function of temperature, layer density, number of layers and layer properties. The two approaches are compared and traded off in terms of simplicity vs. rigor, accuracy vs. expediency.
Bhandari, Pradeep
Structural and Radiation Shielding Properties of Non-parasitic, Multi-functional Microporous Carbon for Aerospace Applications2007-01-31117/9/2007
AFR, Inc. is developing a multifunctional Carbon material that, in addition to excellent radiation shielding characteristics, is appropriate for certain energy storage applications. As an excellent Hydrogen gas sorbent, it increases the usable storage capacity of a gas cylinder by ∼25% at 3500 PSI and by ∼150% at 500 PSI. Our ongoing NASA Langley funded study shows that when a sorbent-filled tank is charged with hydrogen, it provides shielding superior to polyethylene against most types of ionizing particles. Even as hydrogen is consumed, the carbon and tank ensure that significant radiation shielding capability is maintained. In addition to storing hydrogen, the carbon material also displays considerable strength. In this paper, we explore some of its mechanical properties that show this material is very versatile and highly multifunctional. Vastly improved radiation shielding is a clear requirement for a potential manned mission to Mars or a long-duration base on the surface of the Moon. However, current shielding technologies are predicated upon systems dedicated solely to the task of shielding. Such single-use material adds substantially to the mass, and therefore expense, of space operations, without otherwise helping to accomplish mission objectives. One approach to remedy these conflicting constraints is to modify other ship (or EVA suit) systems to maximize their radiation shielding properties, while still serving their primary purposes. Our carbon sorbent material takes this approach. Its performance in this key energy system application is excellent and the carbon itself is a better radiation shield against GCR's and SEP's than the excess Aluminum it can replace. As we explore its mechanical properties, additional functional roles such as micrometeorite protection or some structural applications may emerge.
Rubenstein, Eric P.Wójtowicz, Marek A.Florczak, ElizabethKroo, ErikGordon, JasonTownsend, Lawrence W.Wilkins, RichardGersey, BradAtwell, William
Improvement of Risk Assessment from Space Radiation Exposure for Future Space Exploration Missions2007-01-31167/9/2007
Protecting astronauts from space radiation exposure is an important challenge for mission design and operations for future exploration-class and long-duration missions. Crew members are exposed to sporadic solar particle events (SPEs) as well as to the continuous galactic cosmic radiation (GCR). If sufficient protection is not provided the radiation risk to crew members from SPEs could be significant. To improve exposure risk estimates and radiation protection from SPEs, detailed evaluations of radiation shielding properties are required. A model using a modern CAD tool ProE™, which is the leading engineering design platform at NASA, has been developed for this purpose. For the calculation of radiation exposure at a specific site, the cosine distribution was implemented to replicate the omnidirectional characteristic of the 4π particle flux on a surface. Previously, estimates of doses from SPEs to the blood forming organs (BFO) were made using an average body-shielding distribution for the bone marrow based on the computerized anatomical man (CAM) model. The development of an 82-point body-shielding distribution at BFOs made it possible to estimate the mean and variance of SPE doses in the major active marrow regions. Use of the detailed distribution of bone marrow sites and implementation of the cosine distribution of particle flux is shown to provide improved estimates of acute and cancer risks from SPEs.
Kim, M. Y.Ponomarev, A. L.Nounu, H.Hussein, H.Cucinotta, F. A.Atwell, William
A Comparison of the Radiation Environments in Deep Space2007-01-31147/9/2007
Both humans and onboard radiosensitive systems (electronics, materials, payloads and experiments) are exposed to the deleterious effects of the harsh space radiations found in the space environment. The purpose of this paper is to present the space radiation environment extended to deep space based on environment models for the moon, Mars, Jupiter, and Saturn and compare these radiation environments with the earth's radiation environment, which is used as a comparative baseline. The space radiation environment consists of high-energy protons and electrons that are magnetically “trapped” in planetary bodies that have an intrinsic magnetic field; this is the case for earth, Jupiter, and Saturn (the moon and Mars do not have a magnetic field). For the earth this region is called the “Van Allen belts,” and models of both the trapped protons (AP-8 model) and electrons (AE-8 model) have been developed. Trapped proton and electron models have been developed for Jupiter (GIRE model) and for Saturn (SATRAD model). The space radiation environment also consists of extremely energetic stripped elemental nuclei ranging from hydrogen (proton) to uranium; this environment is called the galactic cosmic radiation (GCR) environment. In addition to trapped and GCR particles, the space environment is sometimes dominated by the emission of high-energy solar protons; these sporadic occurrences or events are called solar proton events (SPE's). Particle spectra (flux vs. energy) and depth dose data for several shielding materials are presented for the moon, Mars, Jupiter, and Saturn and are compared with the particle spectra and radiation exposures for earth orbit.
Atwell, WilliamReddell, BrandonBoeder, Paul
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