| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.99 | 192.32 | 32.80 | 187.80 | 19.29 | 193.23 | -58.13 | 68.52 | 0.8620 | -341.2 | -106.4 | |
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back to the solar disc SDO HMI 2011-11-24 12:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.20 | 160.29 | 1.12 | 150.46 | 19.27 | 194.86 | -56.50 | 68.25 | 0.8496 | -681.1 | -208.5 | |
| 2.91 | -1.00 | 2.75 | -1.00 | 19.38 | 194.45 | -56.91 | 68.20 | 0.8532 | -349.2 | 999999 | |
| 23.98 | -1.00 | 22.46 | -1.00 | 18.76 | 194.61 | -56.75 | 68.89 | 0.8509 | -797.7 | 999999 | |
| 2.23 | 3.25 | 2.18 | 3.19 | 18.69 | 192.88 | -58.47 | 69.29 | 0.8653 | -286.8 | -301.0 | |
| 0.00 | 2.06 | 0.00 | 2.04 | 19.06 | 192.49 | -58.86 | 68.94 | 0.8689 | -226.0 | -165.3 | |
| 1.28 | 1.88 | 1.33 | 1.95 | 19.77 | 191.19 | -60.17 | 68.36 | 0.8802 | 515.1 | 444.1 | |
| 0.00 | 1.54 | 0.00 | 1.80 | 22.00 | 187.83 | -63.53 | 66.45 | 0.9072 | 229.0 | 212.6 | |
| 0.00 | 4.37 | 0.00 | 5.04 | 21.30 | 188.02 | -63.33 | 67.18 | 0.9051 | 660.0 | 506.4 | |
| 0.00 | 2.06 | 0.00 | 2.44 | 21.82 | 187.31 | -64.04 | 66.72 | 0.9105 | 672.0 | 571.4 | |
| 0.00 | 1.37 | 0.00 | 1.64 | 22.01 | 187.16 | -64.20 | 66.54 | 0.9117 | 469.0 | 435.0 | |
| 0.00 | 0.94 | 0.00 | 1.04 | 19.00 | 188.92 | -62.43 | 69.58 | 0.8963 | 312.0 | 328.4 | |
| 1.28 | 3.08 | 1.55 | 3.70 | 21.56 | 186.79 | -64.56 | 67.08 | 0.9136 | 546.5 | 533.8 | |
| 0.00 | 0.26 | 0.00 | 0.32 | 22.14 | 185.91 | -65.45 | 66.58 | 0.9199 | 333.0 | 292.0 | |
| 1.11 | 7.71 | 1.41 | 9.79 | 21.93 | 185.46 | -65.89 | 66.86 | 0.9225 | 327.4 | 201.2 | |
| 0.00 | 0.94 | 0.00 | 1.13 | 20.29 | 186.78 | -64.58 | 68.46 | 0.9125 | 501.0 | 386.2 | |
| 0.00 | 1.11 | 0.00 | 1.41 | 21.62 | 185.51 | -65.84 | 67.20 | 0.9219 | 449.0 | 414.9 | |
| 0.00 | 1.46 | 0.00 | 1.85 | 21.42 | 185.29 | -66.06 | 67.44 | 0.9231 | 269.0 | 230.7 | |
| 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. | |