SDO HMI 2011-05-31 06:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.39 | 107.95 | 15.67 | 66.16 | 15.79 | 40.70 | -32.40 | 61.14 | 0.5902 | -368.1 | -273.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.18 | 75.98 | 9.18 | 45.94 | 15.68 | 41.84 | -31.26 | 60.58 | 0.5757 | -1128.8 | -419.9 | |
| 3.43 | 5.33 | 2.10 | 3.26 | 15.18 | 40.62 | -32.47 | 62.20 | 0.5880 | -772.7 | -512.0 | |
| 0.00 | 3.70 | 0.00 | 2.27 | 15.41 | 40.54 | -32.55 | 61.90 | 0.5902 | -827.0 | -501.3 | |
| 0.00 | 1.26 | 0.00 | 0.78 | 15.76 | 40.22 | -32.88 | 61.58 | 0.5962 | -621.0 | -496.1 | |
| 0.00 | 0.99 | 0.00 | 0.61 | 15.89 | 39.97 | -33.13 | 61.54 | 0.6001 | -609.0 | -456.8 | |
| 0.00 | 1.81 | 0.00 | 1.12 | 16.43 | 39.71 | -33.38 | 60.89 | 0.6063 | -692.0 | -576.8 | |
| 1.26 | 3.61 | 0.79 | 2.26 | 15.36 | 38.47 | -34.63 | 63.28 | 0.6157 | 727.2 | 693.8 | |
| 1.45 | 2.98 | 0.92 | 1.89 | 16.92 | 38.11 | -34.98 | 61.17 | 0.6283 | 835.4 | 581.2 | |
| 0.00 | 1.81 | 0.00 | 1.17 | 16.49 | 36.16 | -36.93 | 62.93 | 0.6493 | 903.0 | 719.0 | |
| 0.00 | 2.17 | 0.00 | 1.41 | 16.72 | 36.07 | -37.02 | 62.66 | 0.6515 | 652.0 | 579.7 | |
| 0.00 | 1.08 | 0.00 | 0.70 | 15.70 | 36.25 | -36.84 | 64.03 | 0.6443 | 662.0 | 509.9 | |
| 0.00 | 1.45 | 0.00 | 0.94 | 15.92 | 36.05 | -37.04 | 63.81 | 0.6479 | 667.0 | 480.8 | |
| 1.54 | 5.78 | 1.01 | 3.81 | 16.66 | 35.40 | -37.69 | 63.10 | 0.6591 | 640.4 | 539.1 | |
| 2.53 | -13.00 | 1.67 | -13.00 | 16.88 | 35.27 | -37.82 | 62.85 | 0.6617 | 687.0 | 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. | |