SDO HMI 2014-03-31 06:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.36 | 40.79 | 8.62 | 22.83 | -24.11 | 116.23 | 22.39 | 228.30 | 0.4676 | 141.3 | -29.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.11 | 18.86 | 6.82 | 10.63 | -23.59 | 117.61 | 23.77 | 230.80 | 0.4787 | 954.6 | 662.0 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -24.27 | 117.34 | 23.51 | 229.35 | 0.4813 | 848.0 | 704.9 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -24.43 | 117.30 | 23.47 | 229.03 | 0.4822 | 674.0 | 544.7 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -24.50 | 117.10 | 23.27 | 228.69 | 0.4805 | 628.0 | 537.7 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -24.38 | 117.01 | 23.17 | 228.79 | 0.4784 | 706.0 | 571.2 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -23.97 | 116.82 | 22.99 | 229.29 | 0.4727 | 889.0 | 767.9 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -23.46 | 116.23 | 22.40 | 229.54 | 0.4613 | -683.0 | -506.1 | |
| 0.00 | 1.58 | 0.00 | 0.88 | -24.82 | 115.31 | 21.47 | 226.07 | 0.4633 | -882.0 | -722.6 | |
| 0.00 | 1.49 | 0.00 | 0.83 | -24.71 | 115.01 | 21.17 | 225.90 | 0.4588 | -768.0 | -645.1 | |
| 3.25 | 5.18 | 1.80 | 2.87 | -24.59 | 114.67 | 20.83 | 225.67 | 0.4539 | -996.2 | -694.8 | |
| 0.00 | 2.28 | 0.00 | 1.26 | -24.64 | 114.32 | 20.49 | 225.16 | 0.4505 | -824.0 | -626.6 | |
| 0.00 | 2.19 | 0.00 | 1.21 | -24.57 | 113.64 | 19.81 | 224.39 | 0.4424 | -844.0 | -594.0 | |
| 0.00 | 1.75 | 0.00 | 0.97 | -25.16 | 113.04 | 19.20 | 222.56 | 0.4420 | -670.0 | -516.5 | |
| 0.00 | 1.14 | 0.00 | 0.63 | -25.14 | 112.65 | 18.82 | 222.06 | 0.4377 | -878.0 | -763.2 | |
| 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. | |