SDO HMI 2013-10-18 00:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.03 | 58.62 | 13.20 | 61.96 | -22.29 | 153.92 | 56.45 | 240.83 | 0.8819 | 199.8 | 102.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.94 | 39.95 | 11.30 | 45.58 | -22.42 | 156.51 | 59.05 | 241.73 | 0.9020 | 593.6 | 138.7 | |
| 0.00 | 0.61 | 0.00 | 0.68 | -22.54 | 155.90 | 58.43 | 241.40 | 0.8981 | 556.0 | 646.0 | |
| 1.13 | 3.05 | 1.04 | 2.79 | -21.32 | 149.03 | 51.56 | 240.15 | 0.8435 | 537.8 | 494.6 | |
| 0.00 | 3.05 | 0.00 | 2.78 | -21.46 | 148.68 | 51.22 | 239.85 | 0.8411 | 587.0 | 526.0 | |
| 0.00 | 1.57 | 0.00 | 1.40 | -20.94 | 148.08 | 50.61 | 240.16 | 0.8343 | -396.0 | -290.3 | |
| 0.44 | 1.48 | 0.40 | 1.36 | -22.34 | 148.51 | 51.04 | 238.80 | 0.8429 | 562.4 | 497.1 | |
| 0.52 | 1.57 | 0.46 | 1.37 | -20.65 | 147.24 | 49.77 | 240.13 | 0.8261 | -391.0 | -371.3 | |
| 0.00 | 1.22 | 0.00 | 1.07 | -20.93 | 147.07 | 49.60 | 239.74 | 0.8258 | -598.0 | -454.6 | |
| 0.00 | 1.05 | 0.00 | 0.91 | -22.39 | 146.16 | 48.69 | 237.70 | 0.8239 | -592.0 | -452.6 | |
| 0.00 | 1.83 | 0.00 | 1.49 | -22.04 | 142.91 | 45.44 | 236.49 | 0.7945 | -409.0 | -343.8 | |
| 0.00 | 1.05 | 0.00 | 0.85 | -24.55 | 141.73 | 44.27 | 233.05 | 0.7967 | -286.0 | -293.4 | |
| 0.00 | 0.79 | 0.00 | 0.62 | -23.63 | 140.39 | 42.92 | 233.31 | 0.7804 | -422.0 | -425.2 | |
| 0.00 | 0.70 | 0.00 | 0.54 | -24.18 | 138.53 | 41.07 | 231.58 | 0.7672 | -426.0 | -369.0 | |
| 0.00 | 0.70 | 0.00 | 0.52 | -23.65 | 136.79 | 39.32 | 231.06 | 0.7486 | -464.0 | -298.1 | |
| 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. | |