Table A.1
Parameters of iron meteors.
| Meteor | v∞ | z | m∞ | τ | Ddr | Class | Quality | Source |
|---|---|---|---|---|---|---|---|---|
| (km s−1) | (deg) | (mg) | (%) | (μm) | ||||
| 09820028 | 19.1 | 34.5 | 80 ± 8 | 0.38 ± 0.06 | 10 ± 2 | A | 3 | Borovička et al. (2005) |
| 01C13024 | 14.6 | 38.2 | 52 ± 10 | 0.30 ± 0.12 | 65 ± 45 | B | 1 | Borovička et al. (2005) |
| 03422018 | 12.9 | 73.1 | 64 ± 7 | 0.72 ± 0.12 | 10 ± 2 | B | 1 | Borovička et al. (2005) |
| 03802071 | 17.9 | 70.4 | 135 ± 25 | 0.10 ± 0.03 | 15 ± 9 | B | 1 | Borovička et al. (2005) |
| 08728012 | 19.3 | 73.7 | 430 ± 43 | 0.22 ± 0.08 | 32 ± 7 | B | 1 | Vojáček et al. (2019) |
| 03422028 | 11.7 | 62.3 | 68 ± 7 | 0.71 ± 0.16 | 8 ± 2 | B | 1 | Borovička et al. (2005) |
| 17328029 | 15.8 | 78.8 | 150 ± 21 | 1.05 ± 0.16 | 15 ± 15 | B | 3 | This work |
| 07A08045 | 31.1 | 44.7 | 125 ± 18 | 0.24 ± 0.06 | 300 ± 63 | C | 1 | Vojáček et al. (2019) |
| 08505008 | 26.6 | 31.1 | 95 ± 15 | 0.34 ± 0.04 | 235 ± 40 | C | 1 | Vojáček et al. (2019) |
| 09B17008 | 23.8 | 28.6 | 90 ± 9 | 0.38 ± 0.04 | 190 ± 19 | C | 1 | Vojáček et al. (2019) |
| 10406008 | 14.4 | 37.8 | 37 ± 5 | 1.17 ± 0.42 | 50 ± 27 | C | 1 | Vojáček et al. (2019) |
| 18417511 | 17.8 | 35.3 | 54 ± 10 | 0.73 ± 0.21 | 103 ± 14 | C | 1 | This work |
| 18816562 | 24.9 | 43.9 | 25 ± 4 | 1.24 ± 0.18 | 220 ± 22 | C | 1 | This work |
| 18A08311 | 23.6 | 57.4 | 265 ± 43 | 0.16 ± 0.08 | 320 ± 54 | C | 1 | This work |
| 03505005 | 11.1 | 25.2 | 125 ± 13 | 0.29 ± 0.08 | 25 ± 11 | C | 2 | Borovička et al. (2005) |
| 03504018 | 19.3 | 18.1 | 10 ± 2 | 0.38 ± 0.10 | 120 ± 23 | D | 1 | Borovička et al. (2005) |
| 09421018 | 18.1 | 14.7 | 38 ± 4 | 1.25 ± 0.18 | 150 ± 15 | D | 1 | Vojáček et al. (2019) |
| 10406060 | 32.6 | 57.0 | 45 ± 10 | 1.38 ± 0.20 | 450 ± 45 | D | 1 | Vojáček et al. (2019) |
| 99A19136 | 21.5 | 49.9 | 6 ± 1 | 2.01 ± 0.83 | 300 ± 30 | D | 2 | Borovička et al. (2005) |
| 17328053 | 14.1 | 26.5 | 135 ± 30 | 0.82 ± 0.16 | 75 ± 24 | D | 2 | This work |
| 05728004 | 21.4 | 63.5 | 210 ± 21 | 0.31 ± 0.08 | 50 ± 16 | D | 3 | Vojáček et al. (2019) |
| 08505025 | 16.1 | 30.1 | 325 ± 38 | 0.48 ± 0.12 | 75 ± 13 | D | 3 | Vojáček et al. (2019) |
| 05403028 | 40.7 | 62.3 | 35 ± 9 | 1.51 ± 0.51 | 500 ± 50 | E | 2 | Vojáček et al. (2019) |
| 06406048 | 41.9 | 57.7 | 110 ± 11 | 0.31 ± 0.08 | 500 ± 50 | E | 3 | Vojáček et al. (2019) |
| 06725005 | 20.1 | 14.5 | 40 ± 4 | 1.77 ± 0.31 | 170 ± 28 | E | 3 | Vojáček et al. (2019) |
| 06C14187 | 12.7 | 39.5 | 125 ± 18 | 1.88 ± 0.26 | 400 ± 40 | E | 3 | Vojáček et al. (2019) |
| 12815084 | 43.4 | 24.0 | 95 ± 26 | 0.18 ± 0.03 | 250 ± 25 | E | 3 | Vojáček et al. (2019) |
| 18A10604 | 14.4 | 57.3 | 900 ± 200 | 0.20 ± 0.06 | 280 ± 28 | F | 2 | This work |
| 17330039 | 18.0 | 39.2 | 4 | This work | ||||
| 17528031 | 16.5 | 56.0 | 4 | This work | ||||
| 18A08052 | 22.6 | 15.5 | 4 | This work | ||||
| 17527052 | 23.7 | 18.9 | 8 ± 2 | 0.80 ± 0.23 | 125 ± 18 | A | 1 | This work |
| 17528003 | 12.7 | 14.3 | 13 ± 2 | 0.94 ± 0.24 | 8 ± 5 | A | 1 | This work |
| 17328044 | 11.6 | 38.9 | 37 ± 7 | 0.91 ± 0.35 | 13 ± 12 | A | 2 | This work |
| 18418500 | 15.6 | 23.0 | 23 ± 4 | 0.21 ± 0.02 | 290 ± 40 | A | 2 | This work |
| 18417546 | 16.7 | 31.0 | 15 ± 2 | 0.29 ± 0.09 | 88 ± 23 | A | 3 | This work |
| 18419552 | 18.3 | 13.5 | 8 ± 3 | 1.39 ± 0.45 | 150 ± 15 | A | 3 | This work |
| 17528017 | 11.6 | 13.1 | 14 ± 3 | 0.40 ± 0.13 | 4 ± 1 | B | 1 | This work |
| 17328019 | 15.0 | 7.4 | 9 ± 1 | 5.84 ± 1.29 | 90 ± 20 | B | 2 | This work |
| 18417517 | 16.6 | 33.9 | 6 ± 1 | 0.66 ± 0.09 | 90 ± 20 | B | 2 | This work |
| 18419522 | 23.4 | 38.9 | 15 ± 4 | 0.10 ± 0.02 | 105 ± 16 | B | 3 | This work |
| 17527050 | 31.2 | 33.3 | 16 ± 5 | 0.53 ± 0.26 | 260 ± 26 | C | 1 | This work |
| 18414513 | 13.5 | 36.5 | 11 ± 3 | 1.44 ± 0.42 | 103 ± 41 | C | 1 | This work |
| 18418531 | 12.5 | 48.0 | 10 ± 2 | 2.21 ± 0.33 | 185 ± 46 | C | 1 | This work |
| 16831033 | 19.7 | 31.4 | 16 ± 4 | 2.02 ± 0.44 | 160 ± 16 | C | 2 | This work |
| 16908086 | 12.4 | 45.7 | 66 ± 7 | 0.31 ± 0.06 | 60 ± 12 | C | 2 | This work |
| 16908095 | 10.7 | 59.6 | 56 ± 8 | 0.29 ± 0.05 | 175 ± 23 | C | 2 | This work |
| 17528006 | 16.5 | 27.0 | 6 ± 2 | 0.54 ± 0.35 | 115 ± 28 | C | 2 | This work |
| 18417537 | 18.3 | 2.7 | 21 ± 5 | 0.57 ± 0.10 | 90 ± 9 | C | 2 | This work |
| 18418556 | 10.7 | 29.9 | 16 ± 2 | 0.68 ± 0.11 | 190 ± 19 | C | 2 | This work |
| 18420548 | 26.1 | 25.6 | 25 ± 4 | 0.08 ± 0.01 | 300 ± 85 | C | 2 | This work |
| 17527056 | 18.0 | 15.8 | 6 ± 2 | 0.36 ± 0.12 | 140 ± 25 | C | 3 | This work |
| 17527048 | 11.1 | 58.8 | 41 ± 6 | 0.23 ± 0.08 | 50 ± 16 | F | 2 | This work |
| 18418502 | 11.2 | 20.1 | 12 ± 3 | 0.30 ± 0.04 | 80 ± 8 | F | 2 | This work |
| 18420509 | 12.5 | 25.8 | 11 ± 3 | 0.32 ± 0.08 | 140 ± 58 | F | 2 | This work |
| 17328042 | 11.1 | 41.7 | 16 ± 3 | 0.31 ± 0.03 | 55 ± 22 | F | 3 | This work |
Notes. The first part lists meteors with iron spectra, the second part contains meteors without spectra. Initial velocity v∞ and zenith distance z come directly from observations. Initial mass m∞, luminous efficiency τ, and mean diameter of iron drops Ddr is determined by the model. A description of light curve classes A–F can be found in Sect. 5. The column “quality” means the quality of the fit; 1 is the best, 3 is the worst, and 4 means unsuccessful modeling. The cases of unsuccessful modeling are listed only for meteors with iron spectra.
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