| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.74 | 56.46 | 20.62 | 73.67 | 21.13 | 300.21 | -65.68 | 66.77 | 0.9251 | -215.9 | -44.4 | |
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back to the solar disc SDO HMI 2011-12-13 03:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 1.26 | 25.42 | 300.24 | -65.64 | 62.23 | 0.9315 | -263.0 | -275.8 | |
| 4.34 | 9.54 | 4.93 | 10.81 | 19.98 | 303.83 | -62.06 | 67.35 | 0.9015 | -578.4 | -561.7 | |
| 0.00 | 1.28 | 0.00 | 1.47 | 19.83 | 303.39 | -62.50 | 67.60 | 0.9043 | -208.0 | -175.3 | |
| 1.36 | 2.21 | 1.60 | 2.60 | 20.06 | 302.81 | -63.07 | 67.46 | 0.9086 | -318.2 | -248.1 | |
| 0.00 | 1.02 | 0.00 | 1.16 | 18.98 | 303.56 | -62.33 | 68.50 | 0.9020 | -518.0 | -433.2 | |
| 0.00 | 0.94 | 0.00 | 1.11 | 19.90 | 302.64 | -63.24 | 67.67 | 0.9095 | -336.0 | -280.9 | |
| 4.68 | 15.67 | 5.73 | 19.30 | 20.19 | 301.70 | -64.18 | 67.52 | 0.9160 | -432.3 | 69.8 | |
| 0.00 | 1.11 | 0.00 | 1.29 | 18.80 | 302.71 | -63.17 | 68.85 | 0.9076 | -404.0 | -363.9 | |
| 1.87 | 4.17 | 2.54 | 5.68 | 22.67 | 299.49 | -66.39 | 65.27 | 0.9325 | -264.6 | 74.6 | |
| 0.00 | 1.70 | 0.00 | 2.27 | 22.16 | 299.74 | -66.14 | 65.77 | 0.9305 | -382.0 | -271.2 | |
| 0.00 | 3.15 | 0.00 | 3.86 | 19.85 | 301.60 | -64.28 | 67.91 | 0.9163 | -567.0 | -393.1 | |
| 0.00 | 0.85 | 0.00 | 1.04 | 19.60 | 301.50 | -64.38 | 68.20 | 0.9167 | -394.0 | -299.1 | |
| 0.00 | 1.45 | 0.00 | 1.95 | 21.52 | 299.45 | -66.44 | 66.50 | 0.9315 | 65.0 | 82.8 | |
| 0.00 | 1.79 | 0.00 | 2.48 | 21.69 | 298.72 | -67.16 | 66.44 | 0.9358 | 527.0 | 434.1 | |
| 0.00 | 1.53 | 0.00 | 2.09 | 20.45 | 298.88 | -67.01 | 67.73 | 0.9337 | -57.0 | -16.2 | |
| 1.45 | 2.04 | 2.33 | 3.29 | 22.69 | 295.62 | -70.27 | 65.87 | 0.9530 | 440.9 | 461.4 | |
| 2.04 | 7.07 | 3.49 | 12.01 | 23.31 | 294.55 | -71.34 | 65.37 | 0.9585 | 341.3 | 316.7 | |
| 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. | |