SDO HMI 2014-03-10 22:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.45 | 78.95 | 16.26 | 40.84 | 6.50 | 11.20 | 9.29 | 326.14 | 0.2879 | 51.7 | 18.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.78 | 3.03 | 0.41 | 1.58 | 5.71 | 14.70 | 12.78 | 315.11 | 0.3134 | -971.0 | -748.0 | |
| 0.00 | 1.13 | 0.00 | 0.59 | 7.58 | 14.57 | 12.65 | 319.33 | 0.3347 | 707.0 | 525.6 | |
| 0.00 | 2.17 | 0.00 | 1.13 | 5.98 | 14.28 | 12.36 | 316.67 | 0.3117 | -766.0 | -632.4 | |
| 0.00 | 1.65 | 0.00 | 0.86 | 6.15 | 13.94 | 12.03 | 317.84 | 0.3101 | -877.0 | -673.2 | |
| 0.00 | 1.13 | 0.00 | 0.59 | 6.36 | 13.83 | 11.91 | 318.57 | 0.3114 | -865.0 | -757.2 | |
| 0.00 | 3.90 | 0.00 | 2.03 | 6.14 | 13.45 | 11.54 | 319.00 | 0.3046 | -826.0 | -692.1 | |
| 11.52 | 18.89 | 5.99 | 9.82 | 6.55 | 12.91 | 11.00 | 321.24 | 0.3042 | -1066.0 | -696.4 | |
| 0.00 | 1.04 | 0.00 | 0.54 | 6.82 | 12.34 | 10.43 | 323.27 | 0.3018 | -758.0 | -575.3 | |
| 1.39 | 3.55 | 0.72 | 1.85 | 7.12 | 12.01 | 10.10 | 324.73 | 0.3027 | -877.5 | -690.1 | |
| 0.00 | 2.17 | 0.00 | 1.12 | 6.54 | 10.60 | 8.69 | 327.62 | 0.2815 | 870.0 | 599.8 | |
| 0.00 | 1.30 | 0.00 | 0.67 | 5.31 | 10.49 | 8.58 | 325.48 | 0.2632 | 865.0 | 654.9 | |
| 1.99 | 3.64 | 1.03 | 1.88 | 7.26 | 10.10 | 8.19 | 330.45 | 0.2877 | -828.0 | -626.8 | |
| 0.00 | 3.55 | 0.00 | 1.82 | 5.79 | 9.77 | 7.86 | 328.75 | 0.2635 | 926.0 | 707.9 | |
| 2.51 | 25.30 | 1.29 | 13.02 | 6.76 | 9.61 | 7.69 | 331.10 | 0.2764 | 949.2 | 736.2 | |
| 13.26 | -14.00 | 6.82 | -14.00 | 6.58 | 9.27 | 7.36 | 331.85 | 0.2709 | 1099.8 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.45 | 6.45 | 8.94 | 7.02 | 332.72 | 0.2664 | 863.0 | 726.0 | |
| 0.00 | 3.29 | 0.00 | 1.69 | 6.29 | 8.75 | 6.84 | 333.07 | 0.2626 | 978.0 | 727.3 | |
| 0.00 | 2.34 | 0.00 | 1.20 | 6.60 | 8.70 | 6.78 | 333.78 | 0.2668 | 910.0 | 734.2 | |
| 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. | |