Table 3
Mean geophysical parameters of the real meteor showers related to the predicted filaments of comet C/1963 A1.
cat.; | Dmin − Dmax | ⟨λ⊙ ⟩ | λ⊙,min − λ⊙,max | ⟨α⟩ | ⟨δ⟩ | ⟨Vg⟩ | ⟨Vh⟩ | ⟨Dmj⟩ |
---|---|---|---|---|---|---|---|---|
ref. | [deg] | [deg] | [deg] | [deg] | [km s−1] | [km s−1] | ||
Shower corresponding to Filament F1; ϑ-Leonids | ||||||||
S | 0.086−0.137 | 235.3 ± 9.0 | 224.2−251.8 | 161.4 ± 7.0 | 13.0 ± 3.3 | 70.2 ± 0.7 | 41.4 ± 0.5 | 0.092 ± 0.032 |
Shower corresponding to filament F3; November α-Sextantids, #483 | ||||||||
C | 0.115−0.166 | 222.9 ± 18.3 | 190.5−249.8 | 142.4 ± 13.4 | 1.4 ± 4.7 | 70.4 ± 1.1 | 42.6 ± 0.7 | 0.194 ± 0.059 |
S | 0.085−0.145 | 221.9 ± 5.9 | 211.1−232.3 | 140.6 ± 4.2 | 4.0 ± 2.0 | 69.9 ± 0.8 | 41.5 ± 0.7 | 0.098 ± 0.016 |
E | 0.185−0.227 | 215.3 ± 10.0 | 200.0−239.0 | 136.8 ± 7.4 | 1.2 ± 3.2 | 68.4 ± 1.5 | 41.5 ± 0.6 | 0.161 ± 0.069 |
[1] | 0.279−0.336 | 231.4 | 149.9 | − 3.4 | 71.1 | |||
[2] | 0.303−0.356 | 232.0 | 148.8 ± 0.91 | − 3.9 ± 0.34 | 69.0 | |||
Shower corresponding to filament F4; π-Hydrids, #101 | ||||||||
S | 0.036−0.078 | 314.2 ± 5.2 | 303.3−324.3 | 207.2 ± 4.1 | − 20.0 ± 1.7 | 70.6 ± 0.6 | 42.0 ± 0.5 | 0.090 ± 0.028 |
E | 0.115−0.138 | 315.6 ± 8.1 | 297.9−330.4 | 209.5 ± 6.2 | − 20.3 ± 2.6 | 69.5 ± 0.8 | 40.7 ± 0.6 | 0.101 ± 0.032 |
[3] | 0.083−0.115 | 317.1 | 210.3 ± 1.3 | − 23. ± 0.4 | 70.7 | |||
[4] | >0.4 | 319 | 215.2 ± 1.0 | − 26.2 ± 1.9 | 69.7 | |||
([5] | >0.4 | 271.0 | 179.0 | − 13.7 | 70.8) | |||
Shower corresponding to filament F5; δ-Corvids, #729 | ||||||||
S | 0.040−0.094 | 287.8 ± 6.1 | 278.5−297.7 | 189.0 ± 4.3 | − 14.8 ± 1.7 | 71.5 ± 0.4 | 42.1 ± 0.3 | 0.066 ± 0.014 |
[6] | 0.169 | 282.0 | 186.8 ± 0.93 | − 16.4 ± 0.39 | 71.8 | |||
[5] | >0.4 | 275.2 | 185.9 | − 10.7 | 72.0 |
Notes. The showers were separated from C, S, and E catalogs. In addition, we also give the mean parameters of the related showers in the IAU MDC list as published by various authors. Further symbols are used as follows: Dmin and Dmax are the minimum and maximum values of the Southworth-Hawkins D-discriminant, characterizing the similarity of the mean orbits of the given separated real shower (or shower in the IAU MDC list) and the predicted shower of a given filament (all predicted showers are considered, therefore there is a set of the D-discriminant values); ⟨λ⊙ ⟩ is mean solar longitude; λ⊙,min and λ⊙,max are the minimum and maximum solar longitudes of shower occurrence delimiting the shower activity; ⟨α⟩ and ⟨δ⟩ are the mean equatorial coordinates of geocentric radiant; ⟨Vg⟩ and ⟨Vh⟩ are the mean geocentric and heliocentric velocities; and ⟨Dmj⟩ is the mean value of the Southworth-Hawkins D-discriminant, characterizing the dispersion of meteor orbits in a given variant (see Sect. 4.2).
References. [1] Rudawska & Jenniskens 2014; [2] Jenniskens et al. 2016a; [3] Jenniskens 2006; [4] Molau & Rendtel 2009; [5] Jenniskenset al. 2018; [6] Jenniskenset al. 2016c.
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