| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.88 | 108.79 | 17.28 | 67.33 | 18.04 | 223.74 | 33.37 | 299.31 | 0.6021 | -633.8 | -373.5 | |
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back to the solar disc SDO HMI 2011-11-29 03:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.59 | 16.83 | 225.88 | 35.50 | 296.20 | 0.6218 | 507.0 | 400.7 | |
| 1.45 | 22.32 | 0.91 | 13.93 | 18.05 | 224.67 | 34.29 | 298.73 | 0.6132 | -539.5 | -441.3 | |
| 5.22 | -2.00 | 3.25 | -2.00 | 17.80 | 224.46 | 34.09 | 298.48 | 0.6094 | -966.7 | 999999 | |
| 1.20 | -2.00 | 0.75 | -2.00 | 18.11 | 224.49 | 34.12 | 298.93 | 0.6114 | -693.4 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.70 | 19.01 | 224.58 | 34.21 | 300.22 | 0.6175 | -627.0 | -484.8 | |
| 0.00 | 2.31 | 0.00 | 1.43 | 17.80 | 224.12 | 33.75 | 298.69 | 0.6053 | -802.0 | -727.3 | |
| 0.00 | 1.37 | 0.00 | 0.85 | 17.53 | 223.99 | 33.62 | 298.35 | 0.6022 | -769.0 | -639.2 | |
| 0.00 | 1.54 | 0.00 | 0.96 | 18.21 | 224.10 | 33.73 | 299.32 | 0.6072 | -173.0 | -207.1 | |
| 0.00 | 1.37 | 0.00 | 0.83 | 14.80 | 223.32 | 32.95 | 294.43 | 0.5798 | 537.0 | 434.9 | |
| 20.01 | 74.23 | 12.37 | 45.88 | 18.18 | 223.57 | 33.20 | 299.62 | 0.6007 | -985.0 | -400.6 | |
| 0.00 | 1.03 | 0.00 | 0.62 | 15.11 | 222.97 | 32.60 | 295.14 | 0.5768 | 849.0 | 627.1 | |
| 0.00 | 0.77 | 0.00 | 0.47 | 16.18 | 223.09 | 32.72 | 296.79 | 0.5838 | -368.0 | -303.4 | |
| 0.00 | 0.86 | 0.00 | 0.52 | 19.17 | 221.38 | 31.01 | 302.64 | 0.5801 | -677.0 | -536.9 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 20.42 | 217.49 | 27.12 | 307.84 | 0.5431 | 570.0 | 472.7 | |
| 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. | |