SDO HMI 2011-12-08 09:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.01 | 179.29 | 26.16 | 114.11 | 18.33 | 103.31 | 34.81 | 300.17 | 0.6290 | -261.9 | -216.3 | |
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back to the solar disc SDO HMI 2011-12-08 09:58:56 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 | 0.62 | 16.24 | 107.02 | 38.52 | 295.08 | 0.6626 | -540.0 | -431.4 | |
| 0.00 | 0.77 | 0.00 | 0.50 | 17.90 | 105.07 | 36.58 | 298.48 | 0.6474 | -160.0 | -145.1 | |
| 14.32 | 26.94 | 9.21 | 17.34 | 17.19 | 104.79 | 36.29 | 297.61 | 0.6405 | 922.5 | 498.5 | |
| 0.00 | 1.19 | 0.00 | 0.76 | 16.88 | 103.61 | 35.12 | 297.83 | 0.6248 | 594.0 | 436.9 | |
| 0.00 | 1.79 | 0.00 | 1.13 | 16.66 | 103.34 | 34.85 | 297.67 | 0.6203 | 426.0 | 385.9 | |
| 21.57 | 122.51 | 13.76 | 78.22 | 18.74 | 103.39 | 34.89 | 300.69 | 0.6323 | -1145.9 | -325.0 | |
| 0.00 | 1.79 | 0.00 | 1.13 | 17.19 | 103.04 | 34.54 | 298.63 | 0.6195 | -730.0 | -602.2 | |
| 3.50 | 9.12 | 2.18 | 5.68 | 17.81 | 101.79 | 33.29 | 300.36 | 0.6079 | -895.3 | -586.8 | |
| 0.00 | 1.36 | 0.00 | 0.85 | 18.18 | 101.75 | 33.26 | 300.93 | 0.6097 | -699.0 | -599.1 | |
| 1.62 | 4.26 | 1.01 | 2.65 | 18.27 | 101.33 | 32.83 | 301.36 | 0.6052 | -896.6 | -323.5 | |
| 0.00 | 1.96 | 0.00 | 1.22 | 19.18 | 101.12 | 32.62 | 302.85 | 0.6084 | -916.0 | -633.8 | |
| 0.00 | 1.11 | 0.00 | 0.67 | 16.17 | 99.78 | 31.29 | 299.19 | 0.5736 | 750.0 | 581.5 | |
| 0.00 | 2.05 | 0.00 | 1.24 | 17.99 | 99.08 | 30.58 | 302.57 | 0.5764 | 94.0 | 201.9 | |
| 0.00 | 2.05 | 0.00 | 1.22 | 16.29 | 98.62 | 30.13 | 300.23 | 0.5598 | 849.0 | 718.5 | |
| 0.00 | 1.45 | 0.00 | 0.88 | 18.93 | 98.46 | 29.97 | 304.49 | 0.5755 | 729.0 | 558.1 | |
| 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. | |