| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.80 | 29.63 | 10.93 | 54.92 | 21.13 | 299.93 | -73.12 | 67.84 | 0.9630 | -238.1 | -21.3 | |
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back to the solar disc SDO HMI 2011-12-12 14:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.55 | 4.94 | 3.85 | 7.44 | 20.00 | 303.74 | -69.31 | 68.57 | 0.9458 | -524.1 | -378.6 | |
| 0.00 | 0.85 | 0.00 | 1.34 | 20.26 | 302.83 | -70.21 | 68.42 | 0.9507 | -159.0 | -162.3 | |
| 0.00 | 1.79 | 0.00 | 2.74 | 19.81 | 303.29 | -69.76 | 68.82 | 0.9481 | -253.0 | -173.2 | |
| 0.00 | 0.60 | 0.00 | 0.91 | 19.56 | 303.44 | -69.61 | 69.07 | 0.9471 | -258.0 | -269.3 | |
| 0.00 | 1.11 | 0.00 | 1.75 | 20.10 | 302.81 | -70.24 | 68.58 | 0.9507 | -238.0 | -185.2 | |
| 0.68 | 1.28 | 1.04 | 1.95 | 18.81 | 303.24 | -69.80 | 69.88 | 0.9476 | -338.9 | -365.3 | |
| 3.23 | 5.53 | 5.46 | 9.36 | 20.43 | 301.47 | -71.57 | 68.41 | 0.9575 | -258.6 | -149.3 | |
| 0.34 | -7.00 | 0.58 | -7.00 | 20.24 | 301.38 | -71.66 | 68.62 | 0.9578 | -335.0 | 999999 | |
| 0.00 | 2.13 | 0.00 | 3.72 | 20.59 | 300.87 | -72.18 | 68.31 | 0.9603 | 316.0 | 310.8 | |
| 0.00 | 2.72 | 0.00 | 4.64 | 19.90 | 301.26 | -71.78 | 68.99 | 0.9581 | -188.0 | -113.8 | |
| 0.00 | 1.79 | 0.00 | 3.01 | 19.61 | 301.37 | -71.67 | 69.27 | 0.9574 | -266.0 | -154.4 | |
| 0.00 | 6.21 | 0.00 | 16.17 | 23.47 | 295.36 | -77.69 | 65.94 | 0.9823 | 388.0 | 140.9 | |
| 0.00 | 0.68 | 0.00 | 1.89 | 22.35 | 294.29 | -78.76 | 67.16 | 0.9851 | -110.0 | 35.5 | |
| 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. | |