| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.72 | 41.63 | 20.99 | 63.81 | 21.25 | 299.74 | -69.44 | 67.25 | 0.9460 | -198.8 | -0.2 | |
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back to the solar disc SDO HMI 2011-12-12 21:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.02 | 0.00 | 1.57 | 25.48 | 300.33 | -68.85 | 62.77 | 0.9484 | -134.0 | -138.2 | |
| 4.51 | 5.45 | 5.76 | 6.95 | 20.00 | 303.75 | -65.43 | 67.96 | 0.9237 | -495.4 | -532.8 | |
| 1.28 | 2.30 | 1.69 | 3.05 | 20.11 | 302.88 | -66.30 | 67.99 | 0.9290 | -174.6 | -299.6 | |
| 0.00 | 1.87 | 0.00 | 2.41 | 18.85 | 303.43 | -65.75 | 69.25 | 0.9244 | -528.0 | -374.6 | |
| 0.00 | 1.87 | 0.00 | 2.95 | 22.82 | 299.34 | -69.84 | 65.68 | 0.9509 | 62.0 | 41.2 | |
| 4.51 | 8.17 | 6.32 | 11.49 | 20.28 | 301.60 | -67.58 | 68.01 | 0.9367 | -410.4 | -66.4 | |
| 2.72 | 3.58 | 3.81 | 5.00 | 19.90 | 301.52 | -67.66 | 68.42 | 0.9368 | -286.3 | -226.6 | |
| 0.00 | 2.04 | 0.00 | 2.67 | 18.26 | 302.87 | -66.31 | 69.97 | 0.9273 | -412.0 | -282.5 | |
| 0.00 | 0.60 | 0.00 | 1.04 | 23.36 | 297.49 | -71.69 | 65.38 | 0.9600 | 388.0 | 375.7 | |
| 0.00 | 0.85 | 0.00 | 1.19 | 19.56 | 301.41 | -67.77 | 68.80 | 0.9371 | -235.0 | -202.5 | |
| 0.00 | 1.11 | 0.00 | 1.52 | 18.99 | 301.89 | -67.29 | 69.34 | 0.9338 | -265.0 | -234.9 | |
| 0.00 | 1.62 | 0.00 | 2.51 | 21.32 | 299.43 | -69.75 | 67.24 | 0.9492 | -185.0 | -87.8 | |
| 1.70 | 7.66 | 3.41 | 15.44 | 23.52 | 295.04 | -74.14 | 65.53 | 0.9702 | 319.5 | 218.5 | |
| 0.00 | 1.53 | 0.00 | 2.46 | 20.47 | 298.64 | -70.54 | 68.23 | 0.9526 | -43.0 | 22.1 | |
| 0.00 | 0.94 | 0.00 | 1.60 | 21.31 | 297.50 | -71.68 | 67.50 | 0.9586 | 247.0 | 187.4 | |
| 0.00 | 1.02 | 0.00 | 1.96 | 22.61 | 295.70 | -73.48 | 66.38 | 0.9672 | 490.0 | 427.8 | |
| 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. | |