SDO HMI 2014-03-31 07:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.88 | 45.18 | 6.14 | 25.39 | -24.15 | 116.09 | 22.80 | 228.66 | 0.4727 | 49.8 | -17.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.72 | 15.79 | 4.37 | 8.94 | -23.56 | 117.67 | 24.38 | 231.46 | 0.4856 | 978.1 | 733.8 | |
| 1.05 | -1.00 | 0.60 | -1.00 | -23.70 | 117.40 | 24.12 | 230.96 | 0.4837 | 900.2 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -23.65 | 117.22 | 23.93 | 230.86 | 0.4810 | 969.0 | 615.2 | |
| 0.00 | 3.60 | 0.00 | 2.04 | -24.34 | 117.32 | 24.03 | 229.77 | 0.4879 | 585.0 | 581.1 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -23.87 | 117.12 | 23.83 | 230.36 | 0.4817 | 770.0 | 562.0 | |
| 0.00 | 1.05 | 0.00 | 0.60 | -24.51 | 117.03 | 23.74 | 229.17 | 0.4861 | 682.0 | 607.2 | |
| 0.00 | 1.67 | 0.00 | 0.94 | -23.95 | 116.84 | 23.56 | 229.95 | 0.4791 | 1037.0 | 810.7 | |
| 0.00 | 3.07 | 0.00 | 1.72 | -23.34 | 116.30 | 23.01 | 230.43 | 0.4676 | -622.0 | -384.9 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -24.36 | 115.21 | 21.92 | 227.40 | 0.4640 | -675.0 | -550.8 | |
| 0.00 | 3.95 | 0.00 | 2.21 | -24.80 | 115.26 | 21.97 | 226.69 | 0.4686 | -831.0 | -612.0 | |
| 0.00 | 1.40 | 0.00 | 0.78 | -24.65 | 114.98 | 21.69 | 226.62 | 0.4641 | -793.0 | -636.2 | |
| 2.11 | 4.21 | 1.17 | 2.35 | -24.63 | 114.66 | 21.37 | 226.26 | 0.4603 | -1076.2 | -873.7 | |
| 0.00 | 1.49 | 0.00 | 0.83 | -24.64 | 114.38 | 21.09 | 225.90 | 0.4573 | -872.0 | -718.8 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -24.61 | 113.67 | 20.38 | 225.06 | 0.4491 | -794.0 | -598.0 | |
| 0.00 | 1.67 | 0.00 | 0.92 | -25.17 | 113.06 | 19.77 | 223.31 | 0.4481 | -627.0 | -522.3 | |
| 0.00 | 1.84 | 0.00 | 1.02 | -25.15 | 112.67 | 19.38 | 222.81 | 0.4438 | -747.0 | -643.9 | |
| 0.00 | 1.49 | 0.00 | 0.82 | -25.19 | 111.41 | 18.13 | 220.97 | 0.4312 | -635.0 | -423.7 | |
| 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. | |