SDO HMI 2013-03-29 18:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.15 | 253.48 | 24.67 | 135.51 | 14.85 | 255.31 | 4.66 | 347.91 | 0.3762 | -993.1 | -365.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.05 | 0.00 | 0.56 | 13.42 | 256.98 | 6.33 | 342.61 | 0.3605 | -874.0 | -660.1 | |
| 0.00 | 1.49 | 0.00 | 0.79 | 13.61 | 256.83 | 6.18 | 343.16 | 0.3628 | -791.0 | -659.1 | |
| 0.00 | 2.71 | 0.00 | 1.44 | 13.38 | 256.64 | 5.99 | 343.47 | 0.3584 | -848.0 | -729.9 | |
| 26.97 | 232.47 | 14.42 | 124.37 | 14.88 | 255.66 | 5.01 | 347.05 | 0.3778 | -1262.7 | -359.9 | |
| 0.00 | 1.58 | 0.00 | 0.83 | 13.02 | 255.37 | 4.72 | 346.60 | 0.3473 | -969.0 | -817.4 | |
| 0.00 | 2.98 | 0.00 | 1.58 | 14.20 | 255.02 | 4.37 | 348.27 | 0.3649 | -708.0 | -576.3 | |
| 19.18 | -4.00 | 10.25 | -4.00 | 15.06 | 254.98 | 4.33 | 348.86 | 0.3785 | -1273.6 | 999999 | |
| 0.00 | 2.89 | 0.00 | 1.52 | 12.16 | 254.80 | 4.15 | 347.63 | 0.3314 | -906.0 | -824.8 | |
| 0.00 | 1.66 | 0.00 | 0.88 | 12.92 | 254.44 | 3.79 | 349.11 | 0.3424 | -956.0 | -776.2 | |
| 0.00 | 1.31 | 0.00 | 0.69 | 11.77 | 253.47 | 2.82 | 351.32 | 0.3211 | -733.0 | -580.3 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 10.36 | 253.31 | 2.66 | 351.14 | 0.2973 | -682.0 | -521.2 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 16.12 | 252.51 | 1.85 | 355.41 | 0.3900 | 648.0 | 564.5 | |
| 0.00 | 1.58 | 0.00 | 0.84 | 15.05 | 251.50 | 0.85 | 357.78 | 0.3717 | 953.0 | 795.9 | |
| 0.00 | 1.66 | 0.00 | 0.90 | 17.29 | 251.08 | 0.42 | 359.00 | 0.4077 | 712.0 | 567.4 | |
| 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. | |