SDO HMI 2014-12-01 02:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.97 | 250.32 | 57.32 | 279.15 | 3.25 | 162.80 | 63.58 | 273.20 | 0.8969 | -255.8 | -185.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.87 | 223.57 | 17.18 | 254.33 | 2.48 | 163.88 | 64.66 | 272.31 | 0.9055 | -526.6 | -214.3 | |
| 21.62 | -1.00 | 24.38 | -1.00 | 3.38 | 163.15 | 63.93 | 273.32 | 0.9001 | -568.0 | 999999 | |
| 1.28 | -1.00 | 1.42 | -1.00 | 3.38 | 162.55 | 63.32 | 273.33 | 0.8954 | -775.9 | 999999 | |
| 1.28 | -1.00 | 1.39 | -1.00 | 4.01 | 162.17 | 62.94 | 274.05 | 0.8925 | -563.9 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.86 | 3.60 | 159.72 | 60.49 | 273.63 | 0.8723 | -545.0 | -426.2 | |
| 4.44 | 6.50 | 4.45 | 6.50 | 4.50 | 159.53 | 60.30 | 274.66 | 0.8709 | 381.0 | 145.6 | |
| 0.00 | 0.26 | 0.00 | 0.25 | 3.06 | 158.41 | 59.19 | 273.02 | 0.8609 | 322.0 | 302.3 | |
| 0.00 | 0.85 | 0.00 | 0.79 | 3.97 | 156.96 | 57.74 | 274.12 | 0.8479 | 362.0 | 287.5 | |
| 0.00 | 1.45 | 0.00 | 1.33 | 5.55 | 156.40 | 57.17 | 276.02 | 0.8431 | 415.0 | 346.1 | |
| 1.45 | 2.91 | 1.32 | 2.64 | 5.76 | 156.10 | 56.87 | 276.29 | 0.8404 | 535.4 | 426.4 | |
| 0.00 | 0.34 | 0.00 | 0.31 | 3.98 | 155.81 | 56.58 | 274.18 | 0.8370 | 254.0 | 402.8 | |
| 7.09 | 10.34 | 6.35 | 9.26 | 6.28 | 155.53 | 56.31 | 276.94 | 0.8353 | 719.1 | 553.9 | |
| 0.00 | 0.94 | 0.00 | 0.84 | 6.63 | 155.59 | 56.37 | 277.36 | 0.8361 | 341.0 | 308.7 | |
| 0.94 | 2.31 | 0.83 | 2.04 | 4.05 | 155.06 | 55.84 | 274.29 | 0.8299 | 564.0 | 472.6 | |
| 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. | |