SDO HMI 2014-03-16 03:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.21 | 113.64 | 38.08 | 287.73 | 5.64 | 11.16 | 77.89 | 277.24 | 0.9815 | 131.2 | 51.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.78 | 3.74 | 2.20 | 10.55 | 2.96 | 12.69 | 79.42 | 274.32 | 0.9853 | 296.2 | 233.9 | |
| 0.43 | 1.57 | 1.48 | 5.32 | 6.41 | 14.03 | 80.76 | 277.58 | 0.9902 | -130.2 | -133.3 | |
| 0.00 | 0.78 | 0.00 | 2.31 | 4.71 | 12.85 | 79.58 | 276.05 | 0.9865 | -513.0 | -416.3 | |
| 0.00 | 5.74 | 0.00 | 19.72 | 6.79 | 13.93 | 80.66 | 277.98 | 0.9901 | -38.0 | -59.6 | |
| 0.00 | 6.87 | 0.00 | 18.39 | 3.75 | 11.97 | 78.70 | 275.22 | 0.9834 | -337.0 | -303.4 | |
| 0.00 | 0.61 | 0.00 | 1.56 | 2.75 | 11.68 | 78.41 | 274.24 | 0.9820 | -256.0 | -221.9 | |
| 0.00 | 2.43 | 0.00 | 6.77 | 5.12 | 12.22 | 78.95 | 276.55 | 0.9848 | -318.0 | -320.1 | |
| 1.83 | 7.04 | 4.77 | 18.18 | 5.07 | 11.57 | 78.30 | 276.60 | 0.9828 | -234.4 | -309.5 | |
| 0.43 | -8.00 | 1.15 | -8.00 | 5.29 | 11.67 | 78.41 | 276.81 | 0.9832 | -62.8 | 999999 | |
| 0.00 | 3.65 | 0.00 | 10.14 | 6.63 | 11.93 | 78.66 | 278.12 | 0.9846 | -282.0 | -254.2 | |
| 0.00 | 2.52 | 0.00 | 6.99 | 6.97 | 11.98 | 78.71 | 278.45 | 0.9849 | -310.0 | -282.6 | |
| 5.65 | 65.21 | 14.07 | 157.88 | 5.90 | 10.93 | 77.66 | 277.53 | 0.9811 | 176.3 | 195.6 | |
| 5.13 | -12.00 | 12.31 | -12.00 | 6.31 | 10.29 | 77.02 | 278.04 | 0.9791 | 419.9 | 999999 | |
| 0.96 | 10.26 | 2.10 | 22.85 | 4.36 | 9.50 | 76.23 | 276.19 | 0.9751 | 318.1 | 58.6 | |
| 0.00 | 3.22 | 0.00 | 7.07 | 5.02 | 9.47 | 76.20 | 276.86 | 0.9754 | 513.0 | 421.3 | |
| 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. | |