Hydrogen- and Methane-Loaded Shielding Materials for Mitigation of Galactic Cosmic Rays and Solar Particle Events
und
01. Juli 2015
Über diesen Artikel
Artikel-Kategorie: Research Article
Online veröffentlicht: 01. Juli 2015
Seitenbereich: 59 - 81
DOI: https://doi.org/10.2478/gsr-2015-0006
Schlüsselwörter
© 2015 Kristina Rojdev et al., published by Sciendo
This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 3.0 License.
Figure 1.

Figure 2.

Figure 3.

Figure 4.

Figure 5.

Figure 6.

Figure 7.

Figure 8.

Figure 9.

Figure 10.

Figure 11.

Figure 12.

Figure 13.

Figure 14.

Figure 15.

Figure 16.

Figure 17.

Figure 18.

Figure 19.

Figure 20.

Figure 21.

Figure 22.

Figure 23.

UT1
CNT | = | Nanoporous Carbon Composites |
ESP | = | Energetic Solar Particle |
EVA | = | Extravehicular Activity |
GCR | = | Galactic Cosmic Ray |
GEO | = | Geostationary Orbit |
GLE | = | Ground Level Event |
GTO | = | Geostationary Transfer Orbit |
HDPE | = | High Density Polyethylene |
LEO | = | Low Earth Orbit |
MEO | = | Medium Earth Orbit |
MH | = | Metal Hydride |
MOF | = | Metal Organic Framework |
SPE | = | Solar Particle Event |
CNT material formulas and densities used for radiation transport calculations and the simulated space radiation environment (“Exposure”) used_ “Base” signifies the unaltered material, “H” is the hydrogen-loaded version, and “CH4” is the methane-loaded version_ The subscripts give the mole percent of each radical in the group_ This information was provided by Drs_ Daniel Liang, Matthew Hill, and Song Song_
CNT | |||
---|---|---|---|
Loading Condition | Chemistry | Density (g/cm 3) | Exposure |
Base | C2H4 | 0.95 | SPE, GCR |
Base | (C2H4)97.7C2.30 | 0.95 | SPE, GCR |
H | (C2H4)97.7(CH3)2.3 | 0.95 | SPE, GCR |
CH4 | (C2H4)97.7(CH4)0.32C1.98 | 0.95 | SPE, GCR |
Base | (C2H4)93.27C6.73 | 0.96 | SPE, GCR |
H | (C2H4)93.27(CH3)6.73 | 0.96 | SPE, GCR |
CH4 | (C2H4)93.27(CH4)0.93C5.8 | 0.96 | SPE, GCR |
Base | (C2H4)89.06C10.94 | 0.97 | SPE, GCR |
H | (C2H4)89.06(CH3)10.94 | 0.97 | SPE, GCR |
CH4 | (C2H4)89.06(CH4)1.51C9.43 | 0.97 | SPE, GCR |
Base | (C2H4)79.41C20.59 | 1.00 | SPE, GCR |
H | (C2H4)79.41(CH3)20.59 | 1.00 | SPE, GCR |
CH4 | (C2H4)79.41(CH4)2.84C17.75 | 1.00 | SPE, GCR |
Base | (C2H4)63.16C36.84 | 1.04 | SPE, GCR |
H | (C2H4)63.16(CH3)36.84 | 1.04 | SPE, GCR |
CH4 | (C2H4)63.16(CH4)5.08C31.76 | 1.04 | SPE, GCR |
Base | (C2H4)50C50 | 1.10 | SPE, GCR |
H | (C2H4)50(CH3)50 | 1.11 | SPE, GCR |
CH4 | (C2H4)50(CH4)6.9C43.1 | 1.10 | SPE, GCR |
Base | (C2H4)39.13C60.87 | 1.16 | SPE, GCR |
H | (C2H4)39.13(CH3)60.87 | 1.17 | SPE, GCR |
CH4 | (C2H4)39.13(CH4)8.4C52.49 | 1.16 | SPE, GCR |
Results of a preliminary study (Atwell et al_, 2014)_
MOFs | CNTs | MHs | Total | |
---|---|---|---|---|
1 | 7 | 1 | 9 | |
9 | 7 | 14 | 30 | |
0 | 0 | 25 | 25 |
MH material formulas and densities used for radiation transport calculations and the simulated space radiation environment (“Exposure”) used_ “Base” signifies the unaltered material and “H” is the hydrogen-loaded version_ This information was provided by Drs_ Daniel Liang, Matthew Hill, and Song Song_
Loading Condition | Chemistry | Density (g/cm3) | Exposure |
---|---|---|---|
Base | Li2.35Si | 1.67 | GCR |
H | 91% Li2.35Si and 9% H | 0.84 | GCR |
Base | LiB | 1.65 | GCR |
H | 91% LiB and 9% H | 0.67 | GCR |
Base | CaNi5 | 6.60 | GCR |
H | 96% CaNi5 and 4% H | 6.6 | GCR |
H | CaNi5H6 | 5.01 | GCR |
Base | LaNi4.7Al0.3 | 8.00 | GCR |
H | LaNi4.7Al0.3H6 | 6.08 | GCR |
H | 96% LaNi4.7Al0.3 and 4% H | 7.6 | GCR |
Base | LaNi4.8Sn0.2 | 8.40 | GCR |
H | LaNi4.8Sn0.2H6 | 6.38 | GCR |
H | 96% LaNi4.8Sn0.2 and 4% H | 8.4 | GCR |
Base | LaNi5 | 8.20 | GCR |
H | LaNi5H6 | 6.22 | GCR |
Base | Al2Cu | 5.83 | GCR |
H | Al2CuH | 5.39 | GCR |
Base | Al | 2.70 | GCR |
H | AlH3 | 2.5 | GCR |
H | BaAlH5 | 3.30 | GCR |
H | SrAl2H2 | 2.64 | GCR |
Base | Ti0.98Zr0.02V0.48Fe0.09Cr0.05Mn1.5 | 7.20 | GCR |
H | Ti0.98Zr0.02V0.48Fe0.09Cr0.05Mn1.5H3.3 | 5.80 | GCR |
Base | TiCr1.8 | 5.70 | GCR |
H | TiCr1.8H3.5 | 4.50 | GCR |
Base | TiFe0.9Mn0.1 | 6.50 | GCR |
H | TiFe0.9Mn0.1H2 | 5.20 | GCR |
H | LiAlH4 | 0.92 | GCR |
H | LiMg(AlH4)3 | 1.80 | GCR |
H | Mg(AlH4)2 | 2.24 | GCR |
H | NaAlH4 | 1.81 | GCR |
H | Y3Al2H6.5 | 4.10 | GCR |
Base | V | 6.00 | GCR |
H | VH | 5.60 | GCR |
H | VH2 | 2.30 | GCR |
Base | Li | 0.53 | GCR |
H | 80% Li and 20% H | 0.57 | GCR |
H | 85% Li and 15% H | 0.56 | GCR |
H | 90% Li and 10% H | 0.55 | GCR |
H | 95% Li and 5% H | 0.54 | GCR |
MOF material formulas and densities used for radiation transport calculations and the simulated space radiation environment (“Exposure”) used_ “Base” signifies the unaltered material, “H” is the hydrogen-loaded version, and “CH4” is the methane-loaded version_ This information was provided by Drs_ Daniel Liang, Matthew Hill, and Song Song_
Loading Condition | Chemistry | Density (g/cm 3) | Exposure |
---|---|---|---|
Base | C432H288Be48O144 | 0.42 | GCR |
H | C432H1120Be48O144 | 0.46 | GCR |
Base | Mg18O54H18C72 | 0.91 | GCR |
H | Mg18O54H141C72 | 0.95 | GCR |
Base | Al4O32C56H44 | 1.61 | GCR |
H | Al4O32C56H96 | 1.68 | GCR |
Base | C200H128 |
0.31 | GCR |
H | C200H325 |
0.35 | GCR |
Base | C27H31NO22Sc3 | 1.03 | GCR |
H | C27H66NO22Sc3 | 1.07 | GCR |
Base | Zn216C3132O702H1242 | 0.25 | SPE, GCR |
H | Zn216C3132O702H14814 | 0.30 | SPE, GCR |
CH4 | Zn216C4189O702H5470 | 0.31 | SPE, GCR |
Base | C1536H864Cu96N32O480 | 0.47 | SPE, GCR |
H | C1536H2734Cu96N32O480 | 0.50 | SPE, GCR |
CH4 | C1908H2352Cu96N32O480 | 0.55 | SPE, GCR |
Base | C288H96Cu48O240 | 0.95 | SPE, GCR |
H | C288H531Cu48O240 | 0.99 | SPE, GCR |
CH4 | C362H392Cu48O240 | 1.06 | SPE, GCR |
Base | H112C192O128Zr12Ti12 | 1.10 | SPE, GCR |
H | H260C192O128Zr12Ti12 | 1.33 | SPE, GCR |
CH4 | H208C216O128Zr12Ti12 | 1.17 | SPE, GCR |
Base | H112C192O128Zr24 | 1.20 | SPE, GCR |
H | H260C192O128Zr24 | 1.22 | SPE, GCR |
CH4 | H208C216O128Zr24 | 1.27 | SPE, GCR |
Aggregated data of materials exposed to a GCR and how they compare with a typical spacecraft material (aluminum) and the standard radiation shielding material (HDPE)_
GCR | |||||||||
---|---|---|---|---|---|---|---|---|---|
MOFs | CNTs | MHs | |||||||
non-loaded | H-loaded | CH4-loaded | non-loaded | H-loaded | CH4-loaded | non-loaded | H-loaded | Total | |
0 | 1 | 0 | 0 | 7 | 0 | 1 | 7 | 16 | |
7 | 9 | 5 | 7 | 0 | 7 | 2 | 4 | 41 | |
3 | 0 | 0 | 0 | 0 | 0 | 9 | 16 | 28 |
The percent increase in dose for the methane-loaded MOF materials compared with the hydrogen-loaded equivalents for both the SPE and GCR cases_ The comparisons were made for a thickness of 30 g/cm 2_
MOF | ||
---|---|---|
Base Material | CH4 dose higher than H | |
SPE | GCR | |
Zn216C3132O702H1242 | 34% | 12% |
C1536H864Cu96N32O480 | 3% | 2% |
C288H96Cu48O240 | 0% | 2% |
H112C192O128Zr12Ti12 | 2% | 1% |
H112C192O128Zr24 | 1% | 1% |
The percent increase in dose for the methane-loaded CNT materials compared with the hydrogen-loaded equivalents for both the SPE and GCR cases_ The comparisons were made for a thickness of 30 g/cm 2_
CNT | ||
---|---|---|
Base Material | CH4 dose higher than H | |
SPE | GCR | |
(C2H4)97.7C2.30 | 0% | 0% |
(C2H4)93.27C6.73 | 1% | 0% |
(C2H4)89.06C10.94 | 2% | 1% |
(C2H4)79.41C20.59 | 4% | 2% |
(C2H4)63.16C36.84 | 8% | 3% |
(C2H4)50C50 | 12% | 5% |
(C2H4)39.13C60.87 | 17% | 6% |
Aggregated data of materials exposed to a SPE and how they compare with a typical spacecraft material (aluminum) and the standard radiation shielding material (HDPE)_
SPEs | |||||||
---|---|---|---|---|---|---|---|
MOFs | CNTs | ||||||
non-loaded | H-loaded | CH4-loaded | non-loaded | H-loaded | CH4-loaded | Total | |
0 | 1 | 0 | 0 | 7 | 0 | 8 | |
5 | 4 | 5 | 7 | 0 | 7 | 28 | |
0 | 0 | 0 | 0 | 0 | 0 | 0 |