SDO HMI 2014-10-07 17:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.12 | 0.00 | 12.55 | -20.42 | 103.89 | 7.66 | 196.17 | 0.4830 | 258.3 | 278.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.64 | -17.58 | 110.33 | 14.10 | 209.96 | 0.4669 | 632.0 | 483.5 | |
| 0.00 | 1.58 | 0.00 | 0.87 | -15.53 | 110.08 | 13.85 | 211.95 | 0.4378 | 840.0 | 611.3 | |
| 0.00 | 1.49 | 0.00 | 0.80 | -12.41 | 109.32 | 13.10 | 214.74 | 0.3901 | 975.0 | 833.6 | |
| 0.00 | 0.96 | 0.00 | 0.58 | -25.07 | 109.41 | 13.18 | 201.70 | 0.5608 | 721.0 | 585.5 | |
| 0.00 | 3.07 | 0.00 | 1.78 | -22.60 | 108.89 | 12.66 | 202.78 | 0.5247 | 691.0 | 645.5 | |
| 0.00 | 1.14 | 0.00 | 0.67 | -23.27 | 108.32 | 12.09 | 201.35 | 0.5307 | 721.0 | 602.8 | |
| 0.00 | 1.23 | 0.00 | 0.72 | -23.40 | 108.06 | 11.83 | 200.84 | 0.5311 | 721.0 | 431.9 | |
| 0.00 | 1.23 | 0.00 | 0.67 | -15.93 | 106.82 | 10.60 | 205.09 | 0.4188 | 745.0 | 620.8 | |
| 0.00 | 1.67 | 0.00 | 0.91 | -15.99 | 106.51 | 10.28 | 204.37 | 0.4175 | 933.0 | 752.1 | |
| 0.00 | 2.46 | 0.00 | 1.43 | -23.65 | 105.56 | 9.33 | 196.57 | 0.5227 | 680.0 | 510.4 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -16.80 | 100.18 | 3.95 | 189.52 | 0.4004 | -841.0 | -615.9 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -18.32 | 94.21 | -2.01 | 175.43 | 0.4208 | -833.0 | -594.2 | |
| 0.00 | 1.32 | 0.00 | 0.74 | -22.45 | 94.06 | -2.17 | 175.84 | 0.4853 | -873.0 | -639.3 | |
| 0.00 | 1.58 | 0.00 | 0.87 | -19.38 | 93.50 | -2.73 | 174.10 | 0.4386 | -782.0 | -676.0 | |
| 0.00 | 1.05 | 0.00 | 0.68 | -31.07 | 81.72 | -14.51 | 160.47 | 0.6442 | -456.0 | -379.3 | |
| 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. | |