SDO HMI 2014-05-10 19:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.04 | 285.79 | 31.05 | 170.74 | 14.78 | 249.29 | -29.09 | 57.32 | 0.5606 | -675.9 | -278.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.73 | 270.84 | 3.43 | 161.59 | 15.30 | 249.51 | -28.87 | 56.33 | 0.5617 | -820.4 | -340.4 | |
| 14.69 | -1.00 | 8.74 | -1.00 | 14.50 | 249.52 | -28.86 | 57.56 | 0.5558 | -1282.8 | 999999 | |
| 31.62 | -1.00 | 18.88 | -1.00 | 14.89 | 249.39 | -28.99 | 57.07 | 0.5602 | -1075.3 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.50 | 17.43 | 247.85 | -30.54 | 54.59 | 0.5970 | 602.0 | 440.1 | |
| 0.00 | 0.63 | 0.00 | 0.38 | 12.73 | 247.46 | -30.92 | 62.01 | 0.5697 | 600.0 | 615.9 | |
| 0.00 | 2.33 | 0.00 | 1.40 | 12.23 | 247.42 | -30.96 | 62.84 | 0.5672 | 679.0 | 606.2 | |
| 0.00 | 2.42 | 0.00 | 1.46 | 13.40 | 247.23 | -31.16 | 61.13 | 0.5769 | 651.0 | 591.1 | |
| 0.00 | 1.25 | 0.00 | 0.77 | 14.18 | 246.67 | -31.71 | 60.34 | 0.5887 | 820.0 | 752.9 | |
| 0.00 | 1.52 | 0.00 | 0.93 | 13.83 | 246.61 | -31.77 | 60.92 | 0.5872 | 653.0 | 606.0 | |
| 0.00 | 1.43 | 0.00 | 0.88 | 14.03 | 246.32 | -32.06 | 60.82 | 0.5920 | 589.0 | 536.5 | |
| 0.00 | 3.13 | 0.00 | 1.93 | 14.35 | 246.20 | -32.18 | 60.42 | 0.5955 | 737.0 | 642.4 | |
| 0.00 | 1.16 | 0.00 | 0.72 | 14.83 | 245.97 | -32.41 | 59.86 | 0.6013 | 669.0 | 533.8 | |
| 0.00 | 0.27 | 0.00 | 0.18 | 17.32 | 241.48 | -36.90 | 59.36 | 0.6685 | 581.0 | 587.0 | |
| 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. | |