| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.69 | 177.10 | 29.98 | 185.67 | 19.16 | 193.49 | -60.60 | 69.13 | 0.8817 | -425.4 | -136.0 | |
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back to the solar disc SDO HMI 2011-11-24 07:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.77 | 0.00 | 0.71 | 17.20 | 197.51 | -56.57 | 70.68 | 0.8469 | -437.0 | -377.6 | |
| 0.94 | 154.13 | 0.95 | 156.27 | 19.34 | 194.78 | -59.31 | 68.71 | 0.8728 | -613.9 | -188.2 | |
| 1.71 | -2.00 | 1.75 | -2.00 | 19.33 | 194.35 | -59.74 | 68.79 | 0.8762 | -230.2 | 999999 | |
| 21.08 | -2.00 | 21.33 | -2.00 | 18.78 | 194.56 | -59.53 | 69.39 | 0.8739 | -802.8 | 999999 | |
| 1.11 | 1.29 | 1.19 | 1.37 | 18.61 | 192.81 | -61.28 | 69.86 | 0.8872 | -267.8 | -280.7 | |
| 0.00 | 0.94 | 0.00 | 1.01 | 18.79 | 192.69 | -61.40 | 69.67 | 0.8883 | -223.0 | -256.1 | |
| 1.20 | 1.71 | 1.36 | 1.94 | 19.78 | 191.08 | -63.01 | 68.81 | 0.9012 | 377.1 | 289.0 | |
| 0.00 | 0.69 | 0.00 | 0.84 | 21.72 | 189.19 | -64.89 | 66.96 | 0.9159 | -210.0 | -216.8 | |
| 1.54 | 4.37 | 1.95 | 5.53 | 21.15 | 188.14 | -65.95 | 67.72 | 0.9221 | 460.9 | 420.5 | |
| 1.11 | 1.29 | 1.45 | 1.67 | 21.71 | 187.48 | -66.61 | 67.21 | 0.9266 | 430.3 | 412.0 | |
| 0.00 | 0.60 | 0.00 | 0.71 | 18.18 | 189.70 | -64.39 | 70.75 | 0.9093 | -129.0 | -152.4 | |
| 0.00 | 2.14 | 0.00 | 2.96 | 22.18 | 186.10 | -67.99 | 66.87 | 0.9351 | 396.0 | 313.9 | |
| 0.00 | 6.17 | 0.00 | 8.71 | 21.94 | 185.56 | -68.53 | 67.19 | 0.9380 | 365.0 | 201.1 | |
| 0.00 | 1.03 | 0.00 | 1.46 | 21.56 | 185.42 | -68.67 | 67.61 | 0.9385 | 170.0 | 161.7 | |
| 0.00 | 0.77 | 0.00 | 1.10 | 21.33 | 185.21 | -68.88 | 67.88 | 0.9395 | 127.0 | 164.9 | |
| 0.00 | 1.20 | 0.00 | 1.39 | 15.13 | 189.75 | -64.34 | 74.09 | 0.9066 | -250.0 | -207.2 | |
| 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. | |