| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.06 | 96.74 | 28.71 | 104.98 | 12.84 | 50.64 | -59.98 | 71.53 | 0.8915 | -103.3 | -60.0 | |
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back to the solar disc SDO HMI 2014-03-02 16:00:28 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.44 | 45.05 | 10.81 | 46.57 | 12.67 | 52.15 | -58.47 | 71.28 | 0.8800 | -683.4 | -319.3 | |
| 3.28 | 5.01 | 3.47 | 5.30 | 13.39 | 51.64 | -58.98 | 70.66 | 0.8856 | -488.9 | -298.9 | |
| 0.00 | 0.86 | 0.00 | 0.93 | 13.61 | 51.07 | -59.55 | 70.59 | 0.8903 | -225.0 | -168.7 | |
| 0.60 | 1.90 | 0.65 | 2.04 | 12.95 | 51.09 | -59.53 | 71.30 | 0.8888 | -369.1 | -265.5 | |
| 0.86 | 2.42 | 0.92 | 2.58 | 12.66 | 51.14 | -59.48 | 71.59 | 0.8878 | -321.2 | -250.4 | |
| 0.00 | 2.59 | 0.00 | 2.81 | 13.14 | 50.77 | -59.85 | 71.18 | 0.8916 | -281.0 | -142.3 | |
| 0.00 | 1.29 | 0.00 | 1.39 | 12.34 | 50.90 | -59.72 | 72.01 | 0.8889 | -191.0 | -103.1 | |
| 0.00 | 2.85 | 0.00 | 3.09 | 12.81 | 50.66 | -59.97 | 71.57 | 0.8917 | 75.0 | 82.7 | |
| 1.21 | 10.10 | 1.36 | 11.27 | 13.32 | 49.76 | -60.86 | 71.28 | 0.8993 | -245.7 | 134.7 | |
| 0.00 | 0.60 | 0.00 | 0.69 | 13.38 | 49.23 | -61.40 | 71.36 | 0.9032 | 383.0 | 361.1 | |
| 0.95 | 3.37 | 1.07 | 3.77 | 12.47 | 49.55 | -61.08 | 72.25 | 0.8992 | 559.5 | 486.1 | |
| 0.00 | 2.50 | 0.00 | 2.81 | 11.99 | 49.35 | -61.27 | 72.82 | 0.8997 | 612.0 | 559.1 | |
| 0.00 | 0.60 | 0.00 | 0.68 | 11.64 | 49.17 | -61.46 | 73.25 | 0.9004 | 271.0 | 342.4 | |
| 0.00 | 1.55 | 0.00 | 1.82 | 13.09 | 48.51 | -62.11 | 71.87 | 0.9077 | 463.0 | 489.4 | |
| 3.62 | 5.44 | 4.27 | 6.40 | 12.59 | 48.20 | -62.43 | 72.48 | 0.9090 | 565.5 | 365.1 | |
| 2.42 | 10.61 | 2.92 | 12.83 | 13.28 | 47.62 | -63.01 | 71.90 | 0.9141 | 313.8 | 335.9 | |
| 2.68 | -16.00 | 3.24 | -16.00 | 13.04 | 47.52 | -63.10 | 72.18 | 0.9143 | 347.0 | 999999 | |
| 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. | |