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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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EOS MLS forward model polarized radiative transfer for Zeeman-Split oxygen lines
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Comparison of Thermal Radiation Damage Models and Parameters for Impact Risk Assessment
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Overview of Space Radiation Risk Modeling at NASA Langley
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A Multi-source Calibrated GOES Dataset and Solar Radiation Environment Model Update
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A Multi-source Calibrated GOES Dataset and Solar Radiation Environment Model Update
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Implementation of a New Scattering Database and a Radar Simulator into Community Radiative Transfer Model
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Responses of Microbes to Modeled Space Radiation
The built environment of spaceships is host to a microbial community that affects crew and craft alike. While the static composition of this community has been characterized and its temporal dynamics examined, the mechanisms controlling its make-up and evolutionary trajectory are not understood. Systematic analyses of microbial diversity show consistent patterns in community composition and function. Understanding these patterns' ecological origins remains a significant challenge, as it requires connecting processes at varying temporal and spatial scales. However, it is clear that the state and trajectories of microbial communities are in-part determined by their physical environment. In this regard, the spaceflight environment includes numerous interacting factors that differentiate it from Earth environments, including an altered atmospheric composition, reduced gravity (and thus altered fluid dynamics), and increased ionizing radiation. These factors impart selective pressures on microbial communities that affect their evolutionary trajectories and thus the risks and benefits these communities represent to crew and craft. The radiation environment of space leads to chronic exposure to low doses and is difficult to mimic on Earth. Thus, little is known about how microbial communities in spacecraft will respond and evolve. Therefore, given the limitations of existing studies, we aim to empirically determine how exposure to low doses of ionizing radiation for thousands of cell divisions affects rates of mutation accumulation in bacteria and the trajectory of their evolution. In this way, we will provide a critical set of data for designing safe and robust space missions. Here we discuss our progress towards this aim, including the construction of exposure facilities, our culturing and analysis approach, and preliminary data.
NAIRAS Atmospheric and Space Radiation Environment Model
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3D Radiative Hydrodynamics Modeling of Acoustic and Gravity Modes Excitation in Main-Sequence Stars with Shallow Outer Convection Zones
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3D Radiative MHD Modeling of Thermodynamical Coupling From Subsurface Layers of the Sun to Corona
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3D Radiative Hydrodynamic Modeling of Shallow Convection Zones of Main-Sequence Moderate-Mass Stars
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L-2 Charged Particle Environment (L2-CPE) Low Energy Radiation Fluence Model
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3D Radiative Hydrodynamic Modeling of Multi-Scale Flows Driven By Subsurface Turbulent Convection
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3D Radiative MHD Modeling of the Solar Transition Zone and Corona
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