SDO HMI 2014-03-10 14:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.82 | 71.87 | 15.27 | 36.78 | 6.66 | 10.88 | 4.56 | 341.89 | 0.2545 | 98.7 | 76.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.91 | 3.03 | 0.98 | 1.56 | 5.84 | 14.30 | 7.97 | 328.46 | 0.2649 | -950.8 | -778.5 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 6.02 | 14.06 | 7.73 | 329.58 | 0.2655 | -828.0 | -590.6 | |
| 0.00 | 1.56 | 0.00 | 0.80 | 6.10 | 13.48 | 7.16 | 331.62 | 0.2620 | -1125.0 | -776.9 | |
| 0.00 | 2.69 | 0.00 | 1.38 | 6.56 | 13.46 | 7.14 | 332.51 | 0.2687 | -1068.0 | -826.7 | |
| 10.75 | 16.21 | 5.52 | 8.33 | 7.13 | 11.99 | 5.67 | 338.37 | 0.2671 | -1103.5 | -674.2 | |
| 0.00 | 0.87 | 0.00 | 0.44 | 6.78 | 10.78 | 4.46 | 342.27 | 0.2547 | 777.0 | 629.4 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 7.82 | 10.64 | 4.32 | 343.93 | 0.2709 | -611.0 | -448.3 | |
| 0.87 | 1.82 | 0.44 | 0.93 | 5.31 | 10.56 | 4.24 | 341.24 | 0.2297 | 955.3 | 810.8 | |
| 0.00 | 1.56 | 0.00 | 0.80 | 6.77 | 10.54 | 4.22 | 343.17 | 0.2534 | 901.0 | 757.6 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 4.79 | 10.41 | 4.08 | 341.14 | 0.2205 | 881.0 | 671.1 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 5.49 | 10.35 | 4.03 | 342.34 | 0.2316 | 1007.0 | 848.2 | |
| 0.00 | 0.87 | 0.00 | 0.44 | 5.61 | 10.23 | 3.91 | 342.99 | 0.2329 | 745.0 | 558.1 | |
| 2.34 | 9.62 | 1.20 | 4.93 | 7.45 | 10.10 | 3.78 | 345.53 | 0.2624 | -834.6 | -239.6 | |
| 3.12 | 8.67 | 1.59 | 4.41 | 5.88 | 9.82 | 3.49 | 345.02 | 0.2355 | 1035.9 | 755.6 | |
| 10.83 | 17.59 | 5.54 | 9.00 | 6.80 | 9.64 | 3.32 | 346.64 | 0.2499 | 1043.1 | 690.3 | |
| 0.00 | 0.35 | 0.00 | 0.18 | 6.49 | 8.83 | 2.51 | 349.60 | 0.2419 | 431.0 | 492.2 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 6.33 | 8.71 | 2.39 | 349.98 | 0.2389 | 806.0 | 591.6 | |
| 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. | |