SDO HMI 2013-10-17 15:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.11 | 92.79 | 22.83 | 84.95 | -22.18 | 153.42 | 50.98 | 238.81 | 0.8403 | 290.6 | 147.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.17 | 55.90 | 13.00 | 55.23 | -22.45 | 156.57 | 54.13 | 239.94 | 0.8674 | 677.7 | 203.9 | |
| 0.87 | -1.00 | 0.85 | -1.00 | -22.53 | 155.95 | 53.52 | 239.61 | 0.8630 | 749.6 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.88 | -23.87 | 153.02 | 50.59 | 236.93 | 0.8452 | 332.0 | 299.9 | |
| 0.00 | 0.44 | 0.00 | 0.37 | -22.49 | 149.23 | 46.80 | 236.65 | 0.8084 | 308.0 | 277.8 | |
| 7.59 | 15.70 | 6.22 | 12.86 | -21.39 | 148.71 | 46.28 | 237.64 | 0.7989 | 652.0 | 443.6 | |
| 0.00 | 0.78 | 0.00 | 0.63 | -20.90 | 147.92 | 45.48 | 237.79 | 0.7895 | -526.0 | -448.2 | |
| 0.00 | 4.10 | 0.00 | 3.37 | -22.33 | 148.41 | 45.97 | 236.42 | 0.8006 | 631.0 | 474.9 | |
| 2.96 | 7.24 | 2.35 | 5.73 | -20.68 | 147.19 | 44.76 | 237.67 | 0.7819 | -792.0 | -544.9 | |
| 0.00 | 1.22 | 0.00 | 0.97 | -21.14 | 147.14 | 44.71 | 237.11 | 0.7837 | -408.0 | -397.2 | |
| 0.00 | 0.87 | 0.00 | 0.72 | -24.04 | 147.80 | 45.37 | 234.20 | 0.8035 | 235.0 | 263.4 | |
| 0.52 | 1.74 | 0.41 | 1.37 | -22.35 | 145.99 | 43.56 | 235.10 | 0.7794 | -566.0 | -412.7 | |
| 0.00 | 1.83 | 0.00 | 1.35 | -22.12 | 142.22 | 39.79 | 233.11 | 0.7436 | -706.0 | -551.9 | |
| 0.00 | 0.96 | 0.00 | 0.70 | -22.37 | 141.43 | 38.99 | 232.31 | 0.7377 | -621.0 | -514.0 | |
| 0.00 | 1.05 | 0.00 | 0.77 | -23.92 | 140.87 | 38.44 | 230.16 | 0.7425 | -548.0 | -505.8 | |
| 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 | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |