SDO HMI 2014-05-26 13:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.90 | 138.05 | 73.22 | 422.81 | -18.87 | 150.55 | 80.49 | 251.04 | 0.9850 | -100.9 | -33.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.53 | 0.00 | 5.78 | -17.59 | 152.59 | 82.53 | 252.43 | 0.9920 | 248.0 | 204.9 | |
| 0.00 | 0.27 | 0.00 | 0.93 | -17.41 | 151.93 | 81.87 | 252.60 | 0.9905 | 422.0 | 419.3 | |
| 11.27 | 50.86 | 50.91 | 241.32 | -18.56 | 153.91 | 83.85 | 251.48 | 0.9945 | -97.8 | -102.2 | |
| 0.72 | 6.49 | 1.91 | 17.19 | -17.28 | 149.11 | 79.05 | 252.66 | 0.9829 | 474.8 | 279.4 | |
| 0.36 | 1.26 | 1.25 | 4.36 | -18.70 | 151.67 | 81.61 | 251.29 | 0.9900 | 335.8 | 292.0 | |
| 0.00 | 1.26 | 0.00 | 2.75 | -17.18 | 146.64 | 76.58 | 252.67 | 0.9745 | 87.0 | 44.0 | |
| 0.00 | 0.45 | 0.00 | 1.27 | -19.23 | 149.74 | 79.68 | 250.70 | 0.9850 | 150.0 | 145.6 | |
| 0.00 | 1.62 | 0.00 | 3.53 | -17.40 | 146.66 | 76.59 | 252.44 | 0.9746 | 252.0 | 220.8 | |
| 1.71 | 12.99 | 3.52 | 26.49 | -17.39 | 145.82 | 75.76 | 252.41 | 0.9714 | -209.0 | -206.4 | |
| 3.52 | -9.00 | 7.08 | -9.00 | -17.65 | 145.50 | 75.43 | 252.12 | 0.9702 | -137.2 | 999999 | |
| 0.54 | 1.35 | 1.06 | 2.66 | -18.04 | 145.09 | 75.03 | 251.70 | 0.9686 | -277.5 | -247.7 | |
| 0.81 | 59.97 | 1.64 | 116.53 | -20.03 | 145.41 | 75.35 | 249.67 | 0.9704 | -275.6 | 32.6 | |
| 0.63 | -12.00 | 1.28 | -12.00 | -20.19 | 145.50 | 75.44 | 249.51 | 0.9709 | -292.4 | 999999 | |
| 2.34 | -12.00 | 4.57 | -12.00 | -20.30 | 144.89 | 74.83 | 249.36 | 0.9684 | -562.5 | 999999 | |
| 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. | |