| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.88 | 155.40 | 26.31 | 175.64 | -19.00 | 336.37 | -61.08 | 112.95 | 0.8959 | 385.9 | 171.7 | |
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back to the solar disc SDO HMI 2011-11-13 10:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.12 | 0.00 | 1.02 | -20.03 | 344.19 | -53.26 | 116.30 | 0.8419 | 510.0 | 423.8 | |
| 0.00 | 0.69 | 0.00 | 0.59 | -16.86 | 345.58 | -51.87 | 113.11 | 0.8206 | 442.0 | 310.0 | |
| 0.00 | 0.52 | 0.00 | 0.46 | -18.60 | 344.70 | -52.75 | 114.84 | 0.8335 | 251.0 | 302.7 | |
| 0.00 | 0.86 | 0.00 | 0.83 | -20.77 | 342.11 | -55.34 | 116.44 | 0.8610 | 532.0 | 476.0 | |
| 18.15 | 124.15 | 18.63 | 127.46 | -17.78 | 339.09 | -58.36 | 112.25 | 0.8779 | 656.0 | 211.1 | |
| 0.00 | 2.50 | 0.00 | 2.75 | -18.02 | 336.79 | -60.66 | 111.94 | 0.8955 | 251.0 | 244.0 | |
| 0.00 | 2.58 | 0.00 | 2.84 | -17.68 | 336.73 | -60.72 | 111.55 | 0.8954 | 483.0 | 342.0 | |
| 1.72 | 2.41 | 1.90 | 2.66 | -17.40 | 336.64 | -60.81 | 111.22 | 0.8956 | 445.3 | 474.0 | |
| 0.00 | 1.46 | 0.00 | 2.15 | -22.25 | 330.24 | -67.21 | 114.97 | 0.9427 | -279.0 | -282.8 | |
| 0.00 | 1.38 | 0.00 | 2.05 | -22.50 | 329.91 | -67.54 | 115.16 | 0.9448 | -353.0 | -236.6 | |
| 0.00 | 0.95 | 0.00 | 1.51 | -22.89 | 328.62 | -68.83 | 115.31 | 0.9517 | -328.0 | -313.1 | |
| 0.43 | 3.79 | 0.82 | 7.26 | -24.50 | 325.42 | -72.03 | 116.38 | 0.9673 | -30.4 | 19.9 | |
| 2.58 | -12.00 | 4.96 | -12.00 | -24.54 | 325.37 | -72.08 | 116.40 | 0.9675 | 117.1 | 999999 | |
| 0.00 | 3.36 | 0.00 | 5.51 | -21.96 | 327.81 | -69.64 | 114.20 | 0.9546 | -595.0 | -398.8 | |
| 0.00 | 9.29 | 0.00 | 17.98 | -23.86 | 325.15 | -72.30 | 115.67 | 0.9678 | 298.0 | 182.9 | |
| 0.00 | 0.34 | 0.00 | 0.57 | -22.01 | 327.47 | -69.98 | 114.19 | 0.9562 | -52.0 | -75.2 | |
| 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. | |