Table E.1
H/Si atomic number ratio comparison between this work and the literature.
| This study | ||||||||
|---|---|---|---|---|---|---|---|---|
| Mass Range T(K) ne(cm–3) | H/Si | N | Notes | |||||
| Combined | 10500 4.8 × 1013 | 10000 4.8 × 1013 | 11000 4.8 × 1013 | 10500 1.0 × 1014 | 10500 2.5 × 1013 | |||
| Smallest meteoroids (<0.01 kg) | 3.6 ± 1.5 | ![]() |
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6 | Cometary |
| Small meteoroids (0.01–0.1 kg) | 6.4 ± 3.0 | ![]() |
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14 | Cometary |
| Medium meteoroids (0.1–0.5 kg) | 8.7 ± 4.0 | ![]() |
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5 | Cometary |
| Large meteoroids (>0.5 kg) | 23 ± 10 | ![]() |
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6 | Cometary |
| Asteroidal | 4.5 ± 3.5 | ![]() |
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2 | asteroidal |
| Literature | ||||
|---|---|---|---|---|
| Category | H/Si | N | Source/Reference | Notes |
| Meteors - Perseids | 0.8 & 1.5 | 2 | Borovička & Betlem, 1997 | photographiC speCtra, Hβ |
| Meteors - Perseids and Leonids | 1.5–21.4 | 9 | Borovička et al., 2004 | photographiC speCtra |
| Meteors - Leonid | 4.4 | 1 | Jenniskens & Mandell, 2004 | video speCtrum |
| Comets - Halley’s dust | 10.95 ± 2.37 | – | Jessberger, 1988 | PUMA–1 mass speCtrometer |
| Comets - 67P/Churyumov –Gerasimenko dust | ![]() |
– | Engrand et al., 2024 | COSIMA instrument |
| Meteorites - CI chondrites | 5.308 | – | Wasson & Kallemeyn, 1988 | |
| Meteorites - CI chondrites | 5.29 | – | Anders & Grevesse, 1989 | Compilation |
| Meteorites - CI chondrites | 5.13 | – | Lodders et al., 2009 | |
| Meteorites - CI chondrites | 4.81 ± 0.94 | – | Lodders, 2020 | |
| Meteorites - CM chondrites | 3.024 | – | Wasson & Kallemeyn, 1988 | |
| Meteorites - CV chondrites | 0.50 | – | Wasson & Kallemeyn, 1988 | |
| Meteorites - CO chondrites | 0.12 | – | Wasson & Kallemeyn, 1988 | |
Notes. The combined values correspond to the adopted plasma parameters (10500 K, 4.8 × 1013 cm−3). Their quoted uncertainties combine the measurement and statistical errors of the adopted case with the variation across all tested plasma conditions. The uncertainties of the other values from this study are a combination of the measurement and statistical errors.
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