SDO HMI 2014-12-11 06:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 51.23 | 281.97 | 31.38 | 172.59 | -3.94 | 1.11 | 35.85 | 263.86 | 0.5900 | 873.4 | 345.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.77 | 0.00 | 0.51 | -2.44 | 7.31 | 42.05 | 266.81 | 0.6726 | 469.0 | 416.9 | |
| 0.77 | 2.73 | 0.47 | 1.67 | -1.46 | 1.37 | 36.11 | 268.09 | 0.5917 | -824.7 | -672.5 | |
| 33.07 | 257.32 | 20.32 | 157.72 | -4.12 | 1.38 | 36.12 | 263.59 | 0.5940 | 1110.4 | 364.6 | |
| 14.58 | -3.00 | 8.89 | -3.00 | -3.88 | 0.82 | 35.56 | 263.91 | 0.5858 | 1259.6 | 999999 | |
| 2.47 | 8.27 | 1.50 | 5.02 | -2.85 | 0.71 | 35.45 | 265.67 | 0.5832 | 804.2 | 586.8 | |
| 0.00 | 0.77 | 0.00 | 0.47 | -5.69 | 0.64 | 35.38 | 260.80 | 0.5859 | 555.0 | 494.1 | |
| 0.00 | 1.28 | 0.00 | 0.77 | -1.82 | 0.17 | 34.91 | 267.42 | 0.5749 | -552.0 | -435.3 | |
| 0.00 | 1.88 | 0.00 | 1.12 | -3.53 | 359.26 | 34.00 | 264.30 | 0.5630 | 847.0 | 745.4 | |
| 0.00 | 1.02 | 0.00 | 0.61 | -2.56 | 359.01 | 33.75 | 266.01 | 0.5585 | 654.0 | 461.8 | |
| 0.34 | 1.88 | 0.20 | 1.11 | -2.03 | 358.82 | 33.56 | 266.95 | 0.5554 | 950.2 | 794.8 | |
| 0.00 | 1.11 | 0.00 | 0.66 | -4.13 | 358.78 | 33.52 | 263.17 | 0.5570 | 661.0 | 498.2 | |
| 0.00 | 2.13 | 0.00 | 1.27 | -2.68 | 358.69 | 33.43 | 265.77 | 0.5540 | -561.0 | -408.7 | |
| 0.00 | 2.81 | 0.00 | 1.66 | -3.33 | 358.08 | 32.82 | 264.50 | 0.5457 | -827.0 | -685.5 | |
| 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. | |