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Table 2

Physical properties of SPE fireballs.

Name minf Mabs vinf PE PE type hf p
(g) (mag) (km s−1) (km) (MPa)
SPE01 1.2 −5.7 65.55 −5.72 IIIA/IIIB
SPE02 0.7 −4.7 66.01 −5.25 II/IIIA
SPE03 1.7 −5.9 66.04 −5.05 II
SPE04 19.6 −10.2 65.81 −5.40 IIIA 88 0.0235
SPE05 96.4 −10.9 66.07 −5.36 IIIA 88 0.0236
SPE06 2.8 −6.4 65.75 −5.39 IIIA
SPE07 7.3 −9.0 65.8 −5.48 IIIA 85.5 0.0348
SPE08 90.2 −11.7 65.9 −5.54 IIIA 83.5 0.0468
SPE09 2.6 −7.8 65.8 −4.69 II 80 0.0796
SPE10 0.5 −5.6 65.9 −4.77 II 85.5 0.0349
SPE11 1.2 −5.8 65.69 −5.33 IIIA
SPE12 0.04 −2.6 65.2 −5.29 II/IIIA
SPE13 0.5 −5.0 66.01 −5.17 II 88 0.0236
SPE14 334.5 −12.7 65.87 −5.83 IIIB 84.5 0.0404
SPE15 2670 −15.0 66.44 −5.35 IIIA 81 0.0701
SPE16 2.1 −5.8 65.59 −5.05 II 89.5 0.0185
SPE17 0.1 −3.2 65.9 −5.26 II/IIIA
SPE18 0.3 −5.0 65.8 −5.20 II/IIIA 86 0.0322
SPE19 66.4 −11.7 65.94 −5.19 II/IIIA 79 0.0937
SPE20 0.2 −3.4 65.8 −5.20 II/IIIA
SPE21 9.4 −10.3 66.1 −5.36 IIIA 81.5 0.0642
SPE22 0.6 −4.4 65.75 −5.58 IIIA
SPE23 1.9 −6.7 65.84 −5.30 II/IIIA 85 0.0374
SPE24 3.4 −6.9 65.51 −5.16 II 86 0.0319
SPE25 1.6 −6.1 65.58 −5.72 IIIA/IIIB

Notes. minf is initial photometric mass determined on the basis of luminous efficiency from Revelle & Ceplecha (2001), Mabs absolute brightness (from 100 km distance), vinf initial velocity, PE is explained in Sect. 4.1, hf is the height where the first significant flare on a light curve was observed, p is dynamic pressure at hf.

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