Table A.1
Mean geophysical characteristics of the filaments crossing the Earth’s orbit which are regarded as the predicted meteor showers.
Filament | λ⊙ | α | δ | V g | V h | γ | Ns | Dlim | id. | |
---|---|---|---|---|---|---|---|---|---|---|
tev = 1 kyr, β = 0.005 | ||||||||||
01aI | 229.5 ± 2.0 | 59.4 ± 1.3 | 22.8 ± 0.6 | 29.4 ± 0.4 | 37.6 ± 0.1 | 167.0 | 713 | 0.06 | y | |
tev = 1 kyr, β = 0.007 | ||||||||||
xI | 229.4 ± 1.5 | 59.4 ± 1.0 | 22.8 ± 0.5 | 29.4 ± 0.3 | 37.5 ± 0.1 | 167.0 | 230 | 0.05 | y | |
xII | 103.0 ± 2.0 | 90.0 ± 1.1 | 20.8 ± 0.4 | 29.7 ± 0.6 | 36.8 ± 0.1 | 13.0 | 1360 | 0.06 | y | |
tev = 1 kyr, β = 0.009 | ||||||||||
01cII | 235.5 ± 0.6 | 64.3 ± 0.3 | 23.7 ± 0.3 | 28.7 ± 0.2 | 37.7 ± 0.1 | 169.0 | 30 | 0.06 | y | |
01cIII | 102.3 ± 0.4 | 91.2 ± 0.4 | 20.9 ± 0.2 | 28.6 ± 0.1 | 36.8 ± 0.1 | 11.0 | 143 | 0.05 | y | |
02cI | 253.2 ± 1.9 | 74.7 ± 1.2 | 25.7 ± 0.1 | 24.5 ± 0.4 | 38.1 ± 0.0 | 176.0 | 191 | 0.06 | y | |
02cII | 84.5 ± 0.7 | 81.1 ± 0.4 | 20.1 ± 0.1 | 24.5 ± 0.2 | 37.4 ± 0.0 | 4.0 | 155 | 0.05 | y | |
tev = 1 kyr, β = 0.011 | ||||||||||
01dI | 220.4 ± 7.8 | 53.9 ± 5.0 | 21.4 ± 1.7 | 31.4 ± 1.4 | 37.2 ± 0.4 | 164.0 | 1291 | 0.18 | y | |
01dII | 109.1 ± 6.4 | 93.7 ± 3.1 | 21.0 ± 0.7 | 31.3 ± 1.9 | 36.6 ± 0.3 | 16.0 | 577 | 0.16 | n | |
tev = 2 kyr, β = 0.00001 | ||||||||||
01eI | 101.0 ± 6.6 | 87.9 ± 1.9 | 20.4 ± 0.4 | 29.5 ± 0.5 | 36.8 ± 0.1 | 13.0 | 750 | 0.06 | y | |
tev = 2 kyr, β = 0.0001 | ||||||||||
01fI | 101.1 ± 1.5 | 88.2 ± 0.9 | 20.4 ± 0.3 | 29.6 ± 0.4 | 36.8 ± 0.0 | 13.0 | 852 | 0.06 | y | |
tev = 2 kyr, β = 0.001 | ||||||||||
01gI | 103.6 ± 1.3 | 89.7 ± 0.7 | 20.3 ± 0.2 | 30.2 ± 0.3 | 36.7 ± 0.0 | 14.0 | 908 | 0.08 | y | |
tev = 2 kyr, β = 0.003 | ||||||||||
01hI | 226.1 ± 3.1 | 57.0 ± 1.9 | 22.5 ± 0.7 | 29.8 ± 0.7 | 37.3 ± 0.1 | 166.0 | 297 | 0.11 | y | |
01hIII | 103.2 ± 4.0 | 89.8 ± 2.0 | 20.5 ± 0.5 | 29.9 ± 1.2 | 36.7 ± 0.1 | 14.0 | 1343 | 0.14 | y | |
tev = 2 kyr, β = 0.005 | ||||||||||
01iI | 224.0 ± 2.5 | 55.6 ± 1.6 | 22.7 ± 0.7 | 30.1 ± 0.5 | 37.2 ± 0.1 | 165.0 | 1060 | 0.10 | y | |
01iII | 104.4 ± 3.3 | 90.4 ± 1.7 | 20.3 ± 0.5 | 30.1 ± 1.0 | 36.5 ± 0.1 | 14.0 | 1781 | 0.17 | y | |
tev = 2 kyr, β = 0.007 | ||||||||||
01jI | 224.6 ± 3.5 | 55.8 ± 2.2 | 22.9 ± 0.9 | 29.7 ± 0.7 | 37.1 ± 0.1 | 166.0 | 528 | 0.12 | y | |
01jII | 250.3 ± 1.8 | 75.5 ± 1.2 | 25.6 ± 0.2 | 26.2 ± 0.4 | 37.8 ± 0.1 | 173.0 | 208 | 0.06 | y | |
01jIII | 102.8 ± 4.2 | 89.9 ± 1.6 | 20.2 ± 0.5 | 29.3 ± 1.5 | 36.5 ± 0.3 | 13.0 | 1393 | 0.20 | y | |
tev = 2 kyr, β = 0.009 | ||||||||||
03cI | 213.4 ± 4.7 | 48.3 ± 2.9 | 21.8 ± 1.1 | 31.8 ± 1.0 | 36.6 ± 0.3 | 161.0 | 1164 | 0.19 | y | |
03cII | 110.6 ± 3.5 | 93.1 ± 2.0 | 19.6 ± 0.8 | 31.8 ± 0.9 | 36.0 ± 0.2 | 18.0 | 972 | 0.11 | n | |
tev = 2 kyr, β = 0.011 | ||||||||||
06cI | 214.4 ± 6.0 | 48.9 ± 3.7 | 22.0 ± 1.3 | 31.3 ± 1.2 | 36.4 ± 0.3 | 162.0 | 1337 | 0.23 | y | |
06cII | 110.7 ± 3.5 | 93.0 ± 2.0 | 19.5 ± 0.8 | 31.5 ± 0.9 | 35.8 ± 0.3 | 18.0 | 771 | 0.11 | n | |
tev = 4 kyr, β = 0.00001 | ||||||||||
01kI | 228.4 ± 2.7 | 58.3 ± 1.9 | 23.1 ± 0.6 | 29.3 ± 0.6 | 37.4 ± 0.1 | 167.0 | 614 | 0.07 | y | |
01kII | 101.3 ± 1.9 | 88.8 ± 1.1 | 20.7 ± 0.4 | 29.4 ± 0.6 | 36.8 ± 0.0 | 13.0 | 496 | 0.07 | y | |
tev = 4 kyr, β = 0.0001 | ||||||||||
01lI | 227.2 ± 3.1 | 57.5 ± 2.2 | 23.0 ± 0.7 | 29.5 ± 0.6 | 37.4 ± 0.1 | 167.0 | 582 | 0.08 | y | |
01lII | 101.7 ± 1.7 | 88.8 ± 0.9 | 20.7 ± 0.4 | 29.5 ± 0.6 | 36.7 ± 0.0 | 13.0 | 460 | 0.08 | y | |
tev = 4 kyr, β = 0.001 | ||||||||||
01mI | 226.3 ± 2.4 | 57.1 ± 1.5 | 22.5 ± 0.6 | 29.7 ± 0.6 | 37.3 ± 0.1 | 166.0 | 200 | 0.07 | y | |
01mII | 103.9 ± 1.4 | 90.0 ± 0.8 | 20.7 ± 0.4 | 30.1 ± 0.5 | 36.6 ± 0.0 | 14.0 | 933 | 0.09 | y | |
tev = 4 kyr, β = 0.003 | ||||||||||
01nI | 229.8 ± 2.5 | 60.2 ± 1.8 | 23.6 ± 0.7 | 29.1 ± 0.5 | 37.2 ± 0.1 | 167.0 | 53 | 0.07 | y | |
01nIII | 100.4 ± 4.9 | 89.8 ± 1.9 | 20.1 ± 0.4 | 28.0 ± 1.8 | 36.6 ± 0.2 | 11.0 | 415 | 0.18 | y | |
tev = 4 kyr, β = 0.005 | ||||||||||
01oII | 108.7 ± 1.6 | 92.8 ± 0.9 | 20.1 ± 0.5 | 30.5 ± 0.5 | 36.0 ± 0.1 | 16.0 | 306 | 0.07 | y | |
tev = 4 kyr, β = 0.007 | ||||||||||
04gI | 221.3 ± 3.3 | 54.6 ± 2.3 | 22.6 ± 1.0 | 29.9 ± 0.5 | 36.3 ± 0.2 | 163.0 | 818 | 0.08 | y | |
04gII | 109.1 ± 2.2 | 92.8 ± 1.4 | 20.4 ± 0.7 | 30.1 ± 0.6 | 35.5 ± 0.2 | 17.0 | 429 | 0.09 | y | |
tev = 4 kyr, β = 0.009 | ||||||||||
01pII | 188.7 ± 0.7 | 33.2 ± 0.4 | 7.6 ± 0.1 | 29.1 ± 0.2 | 32.2 ± 0.2 | 155.0 | 53 | 0.16 | n | |
08aI | 188.7 ± 0.7 | 33.2 ± 0.4 | 7.6 ± 0.1 | 29.1 ± 0.2 | 32.2 ± 0.2 | 155.0 | 53 | 0.01 | y | |
tev = 4 kyr, β = 0.011 | ||||||||||
01qI | 206.0 ± 6.6 | 43.0 ± 4.2 | 20.6 ± 1.6 | 29.1 ± 0.5 | 34.0 ± 1.1 | 159.0 | 269 | 0.11 | y | |
01qII | 112.0 ± 3.9 | 91.0 ± 1.7 | 18.9 ± 1.1 | 29.2 ± 0.5 | 33.0 ± 1.2 | 22.0 | 378 | 0.12 | y | |
08bI | 186.1 ± 1.0 | 32.3 ± 0.4 | 7.2 ± 0.2 | 27.1 ± 0.2 | 30.5 ± 0.4 | 153.0 | 18 | 0.01 | y | |
10aI | 71.4 ± 6.8 | 72.4 ± 4.7 | 16.1 ± 1.6 | 20.7 ± 1.2 | 36.5 ± 0.3 | 7.0 | 13 | 0.15 | n | |
tev = 8 kyr, β = 0.00001 | ||||||||||
01rI | 229.0 ± 4.0 | 59.0 ± 3.0 | 23.2 ± 0.8 | 29.3 ± 0.7 | 37.4 ± 0.1 | 167.0 | 243 | 0.09 | y | |
01rII | 102.4 ± 2.1 | 89.6 ± 1.5 | 20.7 ± 0.4 | 29.5 ± 0.7 | 36.7 ± 0.0 | 13.0 | 290 | 0.09 | y | |
11aI | 217.7 ± 1.8 | 53.0 ± 1.1 | 15.1 ± 0.6 | 31.8 ± 0.5 | 37.3 ± 0.0 | 163.0 | 405 | 0.07 | y | |
11aII | 109.2 ± 1.6 | 92.9 ± 1.1 | 27.4 ± 0.6 | 32.2 ± 0.4 | 36.8 ± 0.0 | 17.0 | 584 | 0.07 | n | |
tev = 8 kyr, β = 0.0001 | ||||||||||
01sI | 226.0 ± 4.7 | 56.6 ± 3.8 | 22.8 ± 1.0 | 29.7 ± 0.6 | 37.3 ± 0.1 | 166.0 | 221 | 0.08 | y | |
01sII | 102.5 ± 1.8 | 89.5 ± 1.8 | 20.6 ± 0.4 | 29.7 ± 0.7 | 36.7 ± 0.0 | 13.0 | 262 | 0.08 | y | |
11bI | 219.7 ± 1.6 | 54.2 ± 1.0 | 15.1 ± 0.6 | 31.2 ± 0.4 | 37.4 ± 0.0 | 164.0 | 384 | 0.07 | y | |
11bII | 107.1 ± 1.7 | 91.5 ± 1.2 | 27.6 ± 0.6 | 31.6 ± 0.4 | 36.8 ± 0.0 | 16.0 | 520 | 0.07 | n | |
tev = 8 kyr, β = 0.001 | ||||||||||
05cI | 205.0 ± 2.2 | 41.0 ± 1.7 | 11.3 ± 0.6 | 30.7 ± 0.4 | 36.5 ± 0.1 | 162.0 | 1251 | 0.08 | y | |
05cII | 95.5 ± 0.6 | 76.9 ± 0.7 | 27.2 ± 0.6 | 30.9 ± 0.3 | 35.9 ± 0.0 | 18.0 | 1158 | 0.07 | y | |
tev = 8 kyr, β = 0.003 | ||||||||||
05dI | 197.8 ± 3.9 | 36.2 ± 2.6 | 9.3 ± 0.8 | 30.4 ± 0.6 | 35.4 ± 0.2 | 160.0 | 804 | 0.10 | y | |
05dIII | 96.9 ± 2.0 | 75.8 ± 1.2 | 27.9 ± 0.7 | 30.6 ± 0.5 | 34.7 ± 0.2 | 20.0 | 1118 | 0.09 | y | |
tev = 8 kyr, β = 0.005 | ||||||||||
05eI | 200.1 ± 3.6 | 38.4 ± 2.4 | 9.3 ± 0.5 | 28.6 ± 0.4 | 34.4 ± 0.4 | 160.0 | 80 | 0.07 | y | |
05eIII | 95.6 ± 2.5 | 74.5 ± 1.6 | 29.0 ± 0.7 | 28.7 ± 0.4 | 33.7 ± 0.5 | 20.0 | 217 | 0.08 | y | |
14aI | 167.9 ± 3.6 | 11.1 ± 1.6 | 10.3 ± 1.1 | 26.7 ± 0.5 | 30.2 ± 1.0 | 153.0 | 461 | 0.08 | y | |
15aI | 233.2 ± 3.5 | 65.1 ± 2.9 | 24.6 ± 0.8 | 28.2 ± 0.5 | 36.1 ± 0.2 | 165.0 | 127 | 0.09 | y | |
15aII | 111.5 ± 2.4 | 97.1 ± 2.0 | 20.1 ± 0.5 | 28.5 ± 0.6 | 35.2 ± 0.2 | 15.0 | 108 | 0.07 | y | |
tev = 8 kyr, β = 0.007 | ||||||||||
05fI | 205.6 ±.6 | 42.8 ± 3.1 | 10.5 ± 0.7 | 27.0 ± 0.4 | 33.9 ± 0.6 | 161.0 | 238 | 0.08 | y | |
05fII | 97.3 ± 3.3 | 75.6 ± 2.2 | 29.6 ± 0.8 | 26.9 ± 0.4 | 32.5 ± 0.9 | 21.0 | 176 | 0.08 | y | |
14bI | 151.6 ± 5.0 | 6.7 ± 6.7 | 12.2 ± 4.0 | 21.3 ± 3.7 | 24.0 ± 2.0 | 140.0 | 140 | 0.04 | n | |
18aI | 258.3 ± 4.8 | 87.4 ± 4.2 | 26.7 ± 0.3 | 26.0 ± 0.6 | 36.7 ± 0.2 | 170.0 | 125 | 0.08 | y | |
tev = 16 kyr, β = 0.00001 | ||||||||||
xI | 211.9 ± 1.5 | 45.2 ± 1.5 | 12.6 ± 0.5 | 30.0 ± 0.3 | 37.1 ± 0.0 | 165.0 | 604 | 0.08 | y | |
xII | 220.5 ± 2.2 | 56.8 ± 1.4 | 15.8 ± 0.8 | 32.4 ± 0.6 | 37.4 ± 0.0 | 162.0 | 120 | 0.08 | y | |
xIII | 229.8 ± 3.5 | 60.2 ± 2.7 | 23.5 ± 0.7 | 29.5 ± 0.8 | 37.4 ± 0.1 | 167.0 | 207 | 0.10 | y | |
xIV | 242.7 ± 1.4 | 74.6 ± 1.3 | 18.0 ± 0.4 | 29.5 ± 0.3 | 37.6 ± 0.0 | 167.0 | 290 | 0.09 | y | |
xV | 91.1 ± 0.6 | 75.2 ± 0.7 | 27.1 ± 0.6 | 30.1 ± 0.2 | 36.5 ± 0.0 | 15.0 | 599 | 0.08 | y | |
xV I | 97.9 ± 1.2 | 81.9 ± 0.9 | 26.9 ± 0.5 | 30.8 ± 0.5 | 36.6 ± 0.1 | 16.0 | 18 | 0.25 | n | |
xV II | 258.4 ± 2.1 | 89.9 ± 1.9 | 25.9 ± 0.4 | 29.1 ± 0.3 | 37.7 ± 0.0 | 168.0 | 25 | 0.05 | y | |
xV III | 104.4 ± 3.6 | 91.6 ± 3.0 | 20.7 ± 0.4 | 29.7 ± 0.7 | 36.7 ± 0.0 | 13.0 | 236 | 0.10 | y | |
xIX | 257.1 ± 1.7 | 91.4 ± 1.5 | 18.8 ± 0.5 | 30.9 ± 0.4 | 37.7 ± 0.0 | 165.0 | 16 | 0.07 | y | |
xX | 125.8 ± 2.2 | 115.8 ± 1.8 | 18.6 ± 0.4 | 29.3 ± 0.5 | 37.0 ± 0.0 | 12. | 37 | 0.06 | n | |
tev = 16 kyr, β = 0.005 | ||||||||||
xI | 163.0 ± 4.5 | 10.2 ± 2.1 | − 2.7 ± 1.0 | 22.3 ± 0.6 | 28.8 ± 1.1 | 154.0 | 104 | 0.19 | n | |
xII | 79.5 ± 5.0 | 38.5 ± 4.7 | 26.1 ± 0.7 | 20.6 ± 2.7 | 25.0 ± 2.2 | 36.0 | 93 | 0.12 | y | |
xIII | 93.3 ± 3.5 | 77.9 ± 4.1 | 17.4 ± 0.9 | 24.8 ± 0.5 | 33.3 ± 0.7 | 16.0 | 139 | 0.16 | n | |
xIV | 120.9 ± 4.7 | 116.3 ± 5.9 | 28.5 ± 1.1 | 24.4 ± 0.8 | 35.4 ± 0.4 | 11.0 | 119 | 0.19 | n | |
tev = 16 kyr, β = 0.007 | ||||||||||
xI | 186.0 ± 3.4 | 26.1 ± 1.9 | 2.5 ± 0.8 | 21.5 ± 0.3 | 30.9 ± 0.6 | 159.0 | 39 | 0.04 | n | |
xII | 79.0 ± 10.1 | 41.2 ± 8.8 | 28.8 ± 1.6 | 18.5 ± 2.4 | 26.0 ± 2.9 | 34.0 | 52 | 0.16 | n | |
xIII | 275.0 ± 3.5 | 98.6 ± 3.0 | 28.6 ± 0.4 | 21.4 ± 0.5 | 36.3 ± 0.1 | 174.0 | 21 | 0.05 | n | |
xIV | 101.5 ± 2.9 | 96.4 ± 2.5 | 17.6 ± 0.3 | 22.2 ± 0.8 | 35.1 ± 0.4 | 8.0 | 30 | 0.10 | n | |
tev = 16 kyr, β = 0.0001 | ||||||||||
xI | 163.3 ± 1.9 | 0.9 ± 1.4 | − 3.3 ± 0.6 | 31.2 ± 0.3 | 36.9 ± 0.0 | 163.0 | 184 | 0.04 | y | |
xIV | 52.8 ± 1.6 | 33.3 ± 1.7 | 17.4 ± 0.9 | 31.1 ± 0.6 | 36.8 ± 0.0 | 16.0 | 533 | 0.10 | n | |
tev = 16 kyr, β = 0.001 | ||||||||||
xI | 158.8 ± 3.6 | 2.3 ± 2.6 | − 3.6 ± 1.1 | 31.3 ± 0.4 | 34.5 ± 0.3 | 158.0 | 1152 | 0.10 | y | |
xIIb | 69.4 ± 1.2 | 43.4 ± 1.1 | 21.0 ± 0.5 | 31.3 ± 0.4 | 34.1 ± 0.2 | 23.0 | 565 | 0.09 | y | |
xIV | 82.2 ± 1.2 | 60.0 ± 1.1 | 17.1 ± 0.9 | 31.8 ± 0.4 | 34.9 ± 0.2 | 21.0 | 580 | 0.10 | n | |
tev = 16 kyr, β = 0.003 | ||||||||||
xI | 73.1 ± 1.9 | 30.7 ± 6.4 | 24.3 ± 0.6 | 20.3 ± 3.3 | 24.8 ± 2.6 | 38.0 | 150 | 0.06 | n | |
xII | 120.8 ± 8.3 | 335.9 ± 4.3 | − 0.5 ± 2.3 | 22.4 ± 2.6 | 24.7 ± 2.5 | 142.0 | 811 | 0.13 | n | |
xIII | 118.7 ± 4.4 | 357.0 ± 7.1 | 12.3 ± 3.6 | 14.6 ± 0.8 | 18.4 ± 1.2 | 116.0 | 161 | 0.003 | n |
Notes. tev: the period following the orbital evolution (the theoretical stream was modeled before this time); β: parameter characterizing the strength of P–R effect; λ⊙: mean solar longitude corresponding to the expected maximum of a shower; α and δ: equatorial coordinates of mean geocentric radiant; V g and V h: mean geocentric and heliocentric velocity; γ: angular distance of the mean radiant from the Sun at the time corresponding to the λ⊙ of maximum; Ns: the number of particles in the orbits approaching the Earth’s orbit within 0.05 au; Dlim: the threshold value of the Southworth-Hawkins DSH discriminant used to separate the meteors of the filament, id.: whether the predicted shower was identified with a real counterpart (y: yes, n: no). The angular quantities are given in degrees and velocities in km s−1.
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