Free Access

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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.