SDO HMI 2011-05-31 03:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.76 | 202.45 | 32.75 | 181.48 | -19.90 | 20.41 | -54.33 | 113.52 | 0.8350 | 228.2 | 138.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.63 | 0.00 | 0.53 | -19.36 | 23.06 | -51.68 | 113.59 | 0.8098 | -522.0 | -371.0 | |
| 2.80 | 15.36 | 2.30 | 12.63 | -17.58 | 23.71 | -51.03 | 111.60 | 0.7993 | -695.7 | -521.5 | |
| 3.07 | -2.00 | 2.53 | -2.00 | -17.77 | 23.53 | -51.21 | 111.78 | 0.8015 | -604.9 | 999999 | |
| 0.00 | 1.54 | 0.00 | 1.29 | -19.23 | 22.91 | -51.83 | 113.39 | 0.8109 | -598.0 | -506.1 | |
| 0.00 | 1.45 | 0.00 | 1.23 | -19.65 | 22.51 | -52.23 | 113.78 | 0.8157 | -669.0 | -445.7 | |
| 0.00 | 0.63 | 0.00 | 0.54 | -19.29 | 22.57 | -52.17 | 113.37 | 0.8143 | -617.0 | -528.0 | |
| 0.54 | 2.17 | 0.46 | 1.85 | -19.13 | 22.22 | -52.52 | 113.08 | 0.8172 | -631.3 | -477.7 | |
| 0.00 | 3.25 | 0.00 | 2.74 | -17.76 | 22.60 | -52.13 | 111.53 | 0.8104 | -618.0 | -356.1 | |
| 3.52 | 24.21 | 3.04 | 21.03 | -18.45 | 21.62 | -53.12 | 112.11 | 0.8212 | -664.9 | -199.8 | |
| 1.26 | 2.62 | 1.11 | 2.30 | -18.54 | 20.82 | -53.92 | 112.02 | 0.8287 | 191.8 | 147.5 | |
| 25.57 | 149.06 | 23.31 | 135.87 | -20.43 | 19.82 | -54.92 | 113.99 | 0.8415 | 857.1 | 285.9 | |
| 0.00 | 0.36 | 0.00 | 0.34 | -19.47 | 17.90 | -56.84 | 112.44 | 0.8560 | -545.0 | -521.0 | |
| 0.00 | 0.63 | 0.00 | 0.61 | -19.73 | 17.70 | -57.04 | 112.69 | 0.8581 | -503.0 | -523.7 | |
| 0.00 | 0.54 | 0.00 | 0.52 | -19.60 | 17.65 | -57.09 | 112.53 | 0.8583 | -519.0 | -508.3 | |
| 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. | |