SDO HMI 2014-11-28 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 |
| 10.79 | 34.20 | 5.99 | 18.86 | 17.12 | 151.99 | 20.89 | 308.92 | 0.4403 | 255.0 | -59.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.03 | 2.57 | 0.58 | 1.44 | 18.07 | 153.93 | 22.83 | 308.32 | 0.4721 | 538.5 | 446.6 | |
| 6.50 | 9.32 | 3.64 | 5.22 | 17.94 | 153.65 | 22.54 | 308.43 | 0.4676 | 922.4 | 506.5 | |
| 0.00 | 1.20 | 0.00 | 0.66 | 17.74 | 152.68 | 21.58 | 309.21 | 0.4540 | 849.0 | 663.4 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 17.95 | 152.61 | 21.50 | 309.69 | 0.4551 | 669.0 | 620.5 | |
| 0.00 | 1.28 | 0.00 | 0.69 | 10.75 | 151.78 | 20.68 | 295.71 | 0.3868 | 849.0 | 674.9 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 16.94 | 152.21 | 21.11 | 308.33 | 0.4411 | 572.0 | 522.2 | |
| 0.77 | 2.65 | 0.42 | 1.45 | 15.78 | 151.85 | 20.75 | 306.56 | 0.4262 | 909.1 | 724.6 | |
| 0.43 | 1.71 | 0.23 | 0.94 | 15.99 | 151.87 | 20.77 | 306.95 | 0.4284 | 770.4 | 597.3 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 16.24 | 150.75 | 19.65 | 308.90 | 0.4167 | -902.0 | -717.3 | |
| 1.20 | 3.93 | 0.65 | 2.14 | 16.37 | 150.41 | 19.30 | 309.62 | 0.4136 | -1069.0 | -854.7 | |
| 0.00 | 1.71 | 0.00 | 0.93 | 17.35 | 150.51 | 19.41 | 311.35 | 0.4243 | -905.0 | -713.5 | |
| 0.86 | 3.93 | 0.47 | 2.16 | 18.28 | 150.52 | 19.42 | 313.02 | 0.4336 | -888.4 | -661.5 | |
| 0.00 | 2.48 | 0.00 | 1.35 | 17.42 | 149.77 | 18.66 | 312.54 | 0.4162 | -962.0 | -759.0 | |
| 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. | |