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Table 5

Parameters from thermal disruption model.

Name bulk density grain density Tlim (K) number of sizes number mass (kg)
(kg m-3) (kg m-3)

20101016_070052 7500 7500 1415 5 8000 2.0E-09
3000 6.0E-09
12000 1.0E-08
2000 3.0E-08
1400 5.0E-08
20101016_075031 2500 7000 1450 3 300 1.0E-08
10 7.0E-08
1 3.0E-06
20101020_094418 800 1000 1100 2 400 1.0E-08
10 1.0E-07
20101020_100214 2000 1800 1050 3 2000 8.0E-10
700 1.5E-09
170 1.5E-08
20101103_045928 4500 4500 1550 1 1 3.5E-07
20101103_053624 1000 1000 1080 3 300 8.0E-09
60 4.0E-08
3 3.0E-07
20101103_061856 1500 1500 900 1 60 2.0E-07
20101103_071855 1000 1000 1100 4 1000 5.0E-10
600 1.0E-09
200 5.0E-09
40 2.00E-08
20101106_065820 6500 6500 1400 3 400 1.0E-09
50 1.0E-08
12 1.0E-07
20101107_015015 6000 6000 1100 2 1001 9.0E-09
100 1.5E-08

Notes. Tlim is the temperature at which fragmentation occurs. The number of grain sizes is given for each meteor, and the size and total number of grains for each meteor.

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