SDO HMI 2014-09-11 21:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.82 | 29.64 | 2.50 | 19.06 | -20.00 | 106.26 | 29.08 | 225.79 | 0.6386 | 263.0 | 217.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.44 | 1.51 | 0.30 | 1.02 | -20.15 | 110.65 | 33.48 | 229.62 | 0.6821 | 706.0 | 619.5 | |
| 0.44 | 1.78 | 0.30 | 1.19 | -20.39 | 109.78 | 32.61 | 228.61 | 0.6756 | 826.8 | 666.8 | |
| 0.00 | 2.67 | 0.00 | 1.74 | -18.97 | 108.41 | 31.24 | 229.12 | 0.6509 | 742.0 | 643.5 | |
| 1.87 | 3.20 | 1.21 | 2.08 | -18.73 | 108.21 | 31.04 | 229.24 | 0.6469 | 808.6 | 652.3 | |
| 0.00 | 1.07 | 0.00 | 0.70 | -20.38 | 107.36 | 30.19 | 226.48 | 0.6524 | 672.0 | 495.2 | |
| 1.07 | 2.14 | 0.69 | 1.39 | -20.17 | 107.17 | 30.00 | 226.55 | 0.6487 | 813.7 | 722.8 | |
| 0.00 | 1.25 | 0.00 | 0.81 | -19.96 | 107.09 | 29.92 | 226.73 | 0.6461 | 702.0 | 643.9 | |
| 0.00 | 1.16 | 0.00 | 0.75 | -20.36 | 107.02 | 29.85 | 226.19 | 0.6490 | 675.0 | 631.8 | |
| 0.00 | 2.58 | 0.00 | 1.67 | -20.08 | 106.93 | 29.76 | 226.43 | 0.6457 | 953.0 | 773.0 | |
| 0.00 | 2.14 | 0.00 | 1.44 | -23.83 | 107.39 | 30.21 | 222.61 | 0.6823 | 808.0 | 615.2 | |
| 0.00 | 0.89 | 0.00 | 0.56 | -18.88 | 106.03 | 28.86 | 227.02 | 0.6264 | 664.0 | 500.8 | |
| 0.00 | 1.69 | 0.00 | 1.04 | -18.56 | 103.17 | 26.00 | 224.47 | 0.5954 | -687.0 | -537.3 | |
| 0.00 | 1.78 | 0.00 | 1.09 | -18.65 | 102.33 | 25.16 | 223.44 | 0.5881 | -824.0 | -725.2 | |
| 0.00 | 1.07 | 0.00 | 0.68 | -22.24 | 102.72 | 25.55 | 219.70 | 0.6271 | -593.0 | -523.8 | |
| 0.00 | 1.33 | 0.00 | 0.81 | -18.73 | 102.00 | 24.82 | 222.96 | 0.5856 | -617.0 | -598.1 | |
| 0.00 | 1.60 | 0.00 | 0.97 | -18.21 | 101.64 | 24.46 | 223.19 | 0.5769 | -770.0 | -686.7 | |
| 0.00 | 1.78 | 0.00 | 1.12 | -21.96 | 102.16 | 24.99 | 219.39 | 0.6196 | -655.0 | -507.4 | |
| 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. | |