Inclusion of Radiation Environment Variability in Total Dose Hardness Assurance Methodology.

Variability of the space radiation environment is investigated with regard to parts categorization for total dose hardness assurance methods. It is shown that it can have a significant impact. A modified approach is developed that uses current environment models more consistently and replaces the radiation design margin concept with one of failure probability during a mission.

Solar particle event storm shelter requirements for missions beyond low Earth orbit.

Protecting spacecraft crews from energetic space radiations that pose both chronic and acute health risks is a critical issue for future missions beyond low Earth orbit (LEO). Chronic health risks are possible from both galactic cosmic ray and solar energetic particle event (SPE) exposures. However, SPE exposures also can pose significant short term risks including, if dose levels are high enough, acute radiation syndrome effects that can be mission- or life-threatening. In order to address the reduction of short term risks to spaceflight crews from SPEs, we have developed recommendations to NASA for a design-standard SPE to be used as the basis for evaluating the adequacy of proposed radiation shelters for cislunar missions beyond LEO. Four SPE protection requirements for habitats are proposed: (1) a blood-forming-organ limit of 250 mGy-equivalent for the design SPE; (2) a design reference SPE environment equivalent to the sum of the proton spectra during the October 1989 event series; (3) any necessary assembly of the protection system must be completed within 30 min of event onset; and (4) space protection systems must be designed to ensure that astronaut radiation exposures follow the ALARA (As Low As Reasonably Achievable) principle.

A spatially restricted linear energy transfer equation.

An analytical expression is developed for calculating the average energy deposited by an ion in a volume with dimensions less than the range of the secondary electrons produced. The expression is obtained by including two additional terms in an energy-restricted linear-energy-transfer equation. The usual energy-restricted expression accounts for energy deposited in the volume by energy transfers less than a certain cutoff value. The modified expression, due to the two additional terms, also accounts for energy deposited in the volume which results from energy transfers greater than the cutoff value. The additional terms therefore convert the energy-restricted equation to a distance- or spatially restricted equation. The method is used to obtain radial dose profile information on ion tracks and to calculate the energy deposited by an ion randomly incident upon spherical and hemispherical target sites. Results are in close agreement with more complex methods reported previously for ions with energies from 0.25 to 1000 MeV/amu in volumes of water vapor with dimensions from 1 nm to 10 microns. There are no fitted parameters in this general approach, and all the necessary input data are readily available.

Modeling the yield of double-strand breaks due to formation of multiply damaged sites in irradiated plasmid DNA.

Although double-strand breaks have long been recognized as an important type of DNA lesion, it is well established that this broad class of damage does not correlate well with indicators of the effectiveness of radiation at the cellular level. Assays of double-strand breaks do not distinguish the degree of complexity or clustering of singly damaged sites produced in a single energy deposition event, which is currently hypothesized to be key to understanding cellular end points. As a step toward this understanding, double-strand breaks that are formed proportionally to dose in plasmid DNA are analyzed from the mechanistic aspect to evaluate the yield that arises from multiply damaged sites as hypothesized by Ward (Prog. Nucleic Acid Res. Mol. Biol. 35, 95-125, 1988) and Goodhead (Int. J. Radiat, Biol. 65, 7-17, 1994) as opposed to the yield that arises from single hydroxyl radicals as hypothesized by Siddiqi and Bothe (Radiat. Res. 112, 449-463, 1987). For low-LET radiation such as gamma rays, the importance of multiply damaged sites is shown to increase with the solution's hydroxyl radical scavenging capacity. For moderately high-LET radiation such as 100 keV/micron helium ions, a much different behavior is observed. In this case, a large fraction of double-strand breaks are formed as a result of multiply damaged sites over a broad range of scavenging conditions. Results also indicate that the RBE for common cellular end points correlates more closely with the RBE for multiply damaged sites than with the RBE for total double-strand breaks over a range of LET up to at least 100 keV/micron.

Quantitative assessment of the contribution of clustered damage to DNA double-strand breaks induced by 60Co gamma rays and fission neutrons.

The induction of DNA strand breaks by fission neutrons was studied in aqueous plasmid (pBR322) DNA under aerobic conditions for a wide range of hydroxyl radical (*OH) scavenger concentrations and was compared to the induction of strand breaks by 6OCo gamma rays. Strand breaks were measured using agarose gel electrophoresis coupled with sensitive 32P-based phosphor imaging. Yields are reported for DNA single-strand breaks (SSBs) and double-strand breaks formed linearly with dose (alphaDSBs). The fraction of alphaDSBs that were dependent on the multiply damaged site (MDS) or clustered damage mechanism was also calculated using a model. G values for SSBs and alphaDSBs declined with increasing *OH scavenging capacity. However, with increasing *OH scavenging capacities, the decrease in yields of strand breaks for fission neutrons was not as pronounced as for gamma rays. The percentage of alphaDSBs for gamma rays was dependent on *OH scavenging capacity, appearing negligible at low scavenging capacities but increasing at higher scavenging capacities. In contrast, fission neutrons induced high percentages of alphaDSBs that were approximately independent of *OH scavenging capacity. The levels of alphaDSBs formed by the MDS mechanism after exposure to fission neutrons are consistent with the expected distinctive features of high-LET energy deposition events and track structure. The results also confirm observations made by others that even for low-LET radiation, the MDS mechanism contributes significantly to DNA damage at cell-like scavenging conditions.

Energy deposition and ionization fluctuations induced by ions in small sites--an analytical approach.

A concise, analytical approach is developed for calculating energy deposition and ionization fluctuations in volumes within ion-irradiated media which have dimensions as small as 1 nm. The method accounts for both direct ion interactions with the site and interactions of secondary electrons which are produced by ions in the surrounding medium. Particular attention is given to the way the contributions of the two types of events are combined. Since energy deposition fluctuations are simply related to the fundamental quantities ZD and yD employed in microdosimetry theory, this new approach provides a convenient means to obtain these parameters. Results obtained with the analytical method show good agreement with Monte Carlo charged-particle track-structure calculations of yD for 0.5 to 20 MeV protons incident on spherical sites of water vapor with diameters ranging from 1 nm to 10 microns. In contrast to Monte Carlo techniques, the analytical method does not depend on knowing the intricacies of single ion and electron interactions with the target and can therefore be adapted to calculations with heavier incident ions and different target materials, including those of the condensed state.

Energy deposition events produced by fission neutrons in aqueous solutions of plasmid DNA.

Using an agarose gel electrophoresis assay, single-strand breaks (ssb) induced by fission neutrons and 60Co gamma-rays in aerobic aqueous solutions of pBR322 plasmid DNA were studied. The energy-deposition events of the two radiations were characterized using a Rossi-type proportional counter to measure lineal-energy spectra. For neutrons, the dose-weighted lineal-energy mean, yD, is 63 keV micron-1--about 30 times that for gamma-rays. With increasing yD, hydroxyl radicals produced within spurs or tracks are less likely to survive due to recombination effects, resulting in decreased ssb yields. In TE buffer solution, the ssb yield induced by gamma-rays is 3.2 +/- 0.66 times that induced by neutrons at the same dose. Since the direct radiation effect is small under these conditions, we can estimate that the previously unknown G for hydroxyl radical production by fission neutrons is 0.088 mumol J-1. For glycerol concentrations that give the solution a hydroxyl radical scavenging capacity similar to that of cellular environments, the ssb yield induced by gamma-rays is about 2.0 +/- 0.24 times that induced by neutrons. Analysis shows that this trend with added scavenger is caused primarily by hydroxyl radical yields.

New techniques for predicting solar proton fluences for radiation effects applications.

At geosynchronous altitudes, solar proton events can be a significant source of radiation exposure for devices such as optical imagers, memories and solar cells. These events appear to occur randomly with respect to time and magnitude during the active period of each solar cycle. New probabilistic descriptions, including extreme value theory, are given in forms applicable to assessing mission risks for both single events and the cumulative fluence of multiple events. The analyses yield simpler forms than previous models, include more recent data, and can easily be incorporated into existing computer programs.

Validation of a comprehensive space radiation transport code.

The HZETRN code has been developed over the past decade to evaluate the local radiation fields within sensitive materials on spacecraft in the space environment. Most of the more important nuclear and atomic processes are now modeled and evaluation within a complex spacecraft geometry with differing material components, including transition effects across boundaries of dissimilar materials, are included. The atomic/nuclear database and transport procedures have received limited validation in laboratory testing with high energy ion beams. The codes have been applied in design of the SAGE-III instrument resulting in material changes to control injurious neutron production, in the study of the Space Shuttle single event upsets, and in validation with space measurements (particle telescopes, tissue equivalent proportional counters, CR-39) on Shuttle and Mir. The present paper reviews the code development and presents recent results in laboratory and space flight validation.

Implication of microdosimetry in estimation of radiation quality in space environment.

Errors introduced using a tissue equivalent proportional counter to estimate radiation quality of an arbitrary ion field as related to space radiations are examined. This is accomplished by using a generalized analytic model to calculate the effect of energy loss straggling, track structure, and pathlength distribution on the microdosimetric distribution. The error can be as large as a factor of two, but no systematic trend could be found.

An analysis of energy deposition in a tissue equivalent proportional counter onboard the space shuttle.

An improved prediction for space radiations in the lower earth orbits measured by the shuttle TEPC is obtained when energy loss straggling and chord length distribution of the detector are considered. A generalized analytic model is used to describe the energy deposition of direct ion interaction events in a micron-size detector. The transport calculation accounting for the shuttle configuration is accomplished by using a new version of HZETRN that has been extensively verified with laboratory and flight data. The agreement of predicted and measured lineal energy spectra is within 70% for the region above 2 keV/micrometer but within a factor of 2.3 underpredicted for the region below this value. The inclusion of indirect delta ray events in the model is needed before possible causes for the underprediction below 2 keV/micrometer can be assessed.