SDO HMI 2014-11-29 16:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.36 | 24.11 | 2.76 | 15.01 | 16.47 | 152.41 | 34.49 | 296.34 | 0.6080 | 133.6 | 205.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.16 | 5.30 | 2.03 | 3.41 | 17.19 | 154.78 | 36.85 | 296.13 | 0.6405 | 819.0 | 603.8 | |
| 0.00 | 1.71 | 0.00 | 1.07 | 15.49 | 153.15 | 35.22 | 294.40 | 0.6126 | 923.0 | 714.4 | |
| 0.00 | 1.20 | 0.00 | 0.75 | 16.32 | 153.01 | 35.09 | 295.74 | 0.6148 | 598.0 | 459.9 | |
| 0.00 | 4.44 | 0.00 | 2.76 | 15.43 | 152.72 | 34.80 | 294.53 | 0.6070 | 810.0 | 682.5 | |
| 0.00 | 0.94 | 0.00 | 0.58 | 15.44 | 152.46 | 34.54 | 294.67 | 0.6037 | 888.0 | 747.7 | |
| 0.00 | 0.77 | 0.00 | 0.48 | 16.73 | 152.31 | 34.39 | 296.76 | 0.6080 | 538.0 | 436.1 | |
| 0.00 | 1.71 | 0.00 | 1.06 | 16.48 | 152.22 | 34.30 | 296.43 | 0.6057 | 507.0 | 465.5 | |
| 0.00 | 0.26 | 0.00 | 0.16 | 17.20 | 151.07 | 33.14 | 298.24 | 0.5951 | -757.0 | -654.3 | |
| 0.00 | 1.20 | 0.00 | 0.73 | 15.83 | 150.58 | 32.65 | 296.36 | 0.5816 | -617.0 | -480.4 | |
| 1.20 | 2.65 | 0.73 | 1.61 | 16.50 | 150.30 | 32.38 | 297.62 | 0.5817 | -717.2 | -597.2 | |
| 0.00 | 0.77 | 0.00 | 0.47 | 17.30 | 150.46 | 32.54 | 298.78 | 0.5881 | -720.0 | -618.2 | |
| 0.00 | 2.05 | 0.00 | 1.25 | 17.27 | 150.27 | 32.35 | 298.86 | 0.5856 | -845.0 | -659.4 | |
| 0.00 | 1.11 | 0.00 | 0.68 | 17.77 | 150.37 | 32.45 | 299.56 | 0.5896 | -625.0 | -514.0 | |
| 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. | |