SDO HMI 2013-10-17 16:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.22 | 81.63 | 17.19 | 75.97 | -22.20 | 153.51 | 51.63 | 239.05 | 0.8455 | 207.6 | 163.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.56 | 49.09 | 12.58 | 49.25 | -22.46 | 156.52 | 54.64 | 240.13 | 0.8712 | 692.6 | 199.2 | |
| 0.00 | 1.74 | 0.00 | 1.72 | -22.83 | 155.85 | 53.97 | 239.46 | 0.8673 | 252.0 | 256.1 | |
| 0.00 | 1.31 | 0.00 | 1.22 | -23.87 | 152.99 | 51.11 | 237.16 | 0.8492 | 290.0 | 283.1 | |
| 2.96 | 12.91 | 2.45 | 10.69 | -21.38 | 148.63 | 46.74 | 237.87 | 0.8030 | 749.6 | 513.8 | |
| 0.00 | 1.05 | 0.00 | 0.85 | -20.90 | 147.92 | 46.03 | 238.07 | 0.7945 | -579.0 | -485.3 | |
| 0.00 | 3.14 | 0.00 | 2.61 | -22.33 | 148.42 | 46.54 | 236.70 | 0.8055 | 668.0 | 542.1 | |
| 2.18 | 4.97 | 1.74 | 3.98 | -20.71 | 147.20 | 45.32 | 237.92 | 0.7872 | -794.4 | -559.0 | |
| 0.00 | 0.44 | 0.00 | 0.35 | -20.91 | 147.19 | 45.30 | 237.68 | 0.7880 | -586.0 | -541.4 | |
| 0.00 | 1.22 | 0.00 | 0.98 | -21.14 | 147.18 | 45.30 | 237.42 | 0.7891 | -583.0 | -484.9 | |
| 0.52 | 1.40 | 0.42 | 1.11 | -22.32 | 146.06 | 44.18 | 235.47 | 0.7848 | -517.2 | -449.5 | |
| 0.00 | 1.22 | 0.00 | 0.91 | -22.36 | 142.30 | 40.42 | 233.23 | 0.7509 | -464.0 | -360.7 | |
| 0.00 | 1.40 | 0.00 | 1.03 | -22.36 | 141.33 | 39.45 | 232.61 | 0.7419 | -533.0 | -534.0 | |
| 0.00 | 0.96 | 0.00 | 0.69 | -21.44 | 140.08 | 38.20 | 232.86 | 0.7244 | -420.0 | -401.6 | |
| 0.00 | 0.78 | 0.00 | 0.58 | -23.91 | 140.82 | 38.94 | 230.50 | 0.7469 | -625.0 | -547.7 | |
| 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. | |