Debrecen 2000-10-12 07:29:14 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 56 | 353 | 35 | 217 | -16.61 | 171.45 | -29.40 | 128.40 | 0.6023 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 0 | 1 | 0 | 1 | -18.63 | 172.27 | -28.59 | 131.79 | 0.6104 | |
| 2 | 231 | 1 | 142 | -16.78 | 173.15 | -27.70 | 130.21 | 0.5851 | |
| 16 | -2 | 10 | -2 | -17.24 | 172.63 | -28.22 | 130.31 | 0.5946 | |
| 14 | -2 | 8 | -2 | -16.44 | 172.68 | -28.17 | 129.28 | 0.5873 | |
| 5 | -2 | 3 | -2 | -16.80 | 172.41 | -28.45 | 129.51 | 0.5933 | |
| 1 | -2 | 1 | -2 | -16.50 | 172.06 | -28.80 | 128.76 | 0.5946 | |
| 0 | 2 | 0 | 1 | -14.41 | 173.04 | -27.81 | 126.77 | 0.5663 | |
| 0 | 2 | 0 | 1 | -15.80 | 172.03 | -28.82 | 127.78 | 0.5891 | |
| 0 | 1 | 0 | 0 | -14.33 | 172.84 | -28.02 | 126.45 | 0.5680 | |
| 0 | 1 | 0 | 0 | -16.42 | 170.80 | -30.06 | 127.49 | 0.6078 | |
| 0 | 1 | 0 | 1 | -17.16 | 170.19 | -30.67 | 127.93 | 0.6202 | |
| 12 | 107 | 8 | 67 | -16.12 | 169.78 | -31.09 | 126.18 | 0.6168 | |
| -12 | -12 | -12 | -12 | -16.02 | 169.48 | -31.37 | 125.80 | 0.6192 | |
| 2 | -12 | 1 | -12 | -16.09 | 169.04 | -31.82 | 125.51 | 0.6246 | |
| 4 | -12 | 3 | -12 | -16.05 | 168.60 | -32.26 | 125.09 | 0.6292 | |
| 0 | 0 | 0 | 0 | -17.41 | 167.61 | -33.25 | 126.10 | 0.6499 | |
| 0 | 5 | 0 | 3 | -17.43 | 167.19 | -33.67 | 125.80 | 0.6544 | |
| 0 | 1 | 0 | 0 | -16.54 | 166.71 | -34.15 | 124.26 | 0.6534 | |
| 0 | 1 | 0 | 1 | -17.41 | 162.11 | -38.75 | 122.17 | 0.7080 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |