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Table 3
Impact energies.
| Observer | Effective | Full-disk | Jupiter reflected | Jupiter DNs | Flash DNs | 1DN (J) | Flash energy (J) |
| solar constant | albedo | power (W) | |||||
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|
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| A.W. | 6.6 W/m2 | 0.50 | 4.96 × 1016 | 2.51 × 109 | (18.1 ± 0.8) × 106 | 3.29 × 105 | (6.0 ± 0.3) × 1012 |
| C.G. | 6.2 W/m2 | 0.40 | 5.30 × 1016 | 5.92 × 106 | (4.9 ± 0.1) × 104 | 1.14 × 108 | (5.6 ± 0.2) × 1012 |
|
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| M.T. | 28 W/m2 | 0.45 | 1.89 × 1017 | 3.11 × 109 | (4.7 ± 0.4) × 104 | 1.9 × 109 | (88 ± 7.3) × 1012 |
| K.A. | 28 W/m2 | 0.45 | 1.89 × 1017 | 7.40 × 106 | (9.8 ± 1.2) × 104 | 1.6 × 109 | (16 ± 2.0) × 1012 |
| M.I. | 28 W/m2 | 0.45 | 1.89 × 1017 | 3.37 × 106 | (9.7 ± 1.0) × 103 | 3.6 × 109 | (35 ± 3.4) × 1012 |
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| G.H. | 4.8 W/m2 | 0.50 | 3.67 × 1016 | 2.16 × 109 | (17.0 ± 0.7) × 106 | 1.1 × 106 | (19 ± 0.6) × 1012 |
Notes. Uncertainties in the flash DN and flash energy columns are based solely on photometric uncertainties in Fig. 6. The order-of-magnitude variations in the total Jupiter DNs for different videos come from different image codifications in the original data.
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