| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.82 | 36.00 | 1.40 | 17.84 | 7.83 | 207.59 | -1.33 | 107.49 | 0.0357 | -22.0 | 165.9 | |
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back to the solar disc SDO HMI 2014-09-29 04:00:33 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 0.39 | 7.37 | 210.66 | 1.74 | 287.94 | 0.0318 | -1106.0 | -894.2 | |
| 0.00 | 3.09 | 0.00 | 1.53 | 7.61 | 210.12 | 1.20 | 303.99 | 0.0251 | -643.0 | -731.8 | |
| 0.00 | 2.65 | 0.00 | 1.31 | 7.44 | 209.63 | 0.71 | 311.31 | 0.0165 | -1106.0 | -941.5 | |
| 0.00 | 1.15 | 0.00 | 0.57 | 6.30 | 208.66 | -0.26 | 153.74 | 0.0102 | -832.0 | -620.2 | |
| 0.00 | 1.06 | 0.00 | 0.52 | 7.62 | 208.48 | -0.44 | 28.46 | 0.0160 | -930.0 | -737.2 | |
| 0.00 | 3.35 | 0.00 | 1.66 | 7.11 | 208.09 | -0.83 | 70.52 | 0.0154 | -1287.0 | -921.6 | |
| 0.00 | 0.79 | 0.00 | 0.39 | 7.02 | 207.79 | -1.13 | 79.81 | 0.0201 | -866.0 | -696.0 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 8.73 | 207.17 | -1.75 | 42.01 | 0.0452 | 839.0 | 589.6 | |
| 1.32 | 8.91 | 0.66 | 4.42 | 7.95 | 206.96 | -1.95 | 59.63 | 0.0393 | 1019.6 | 708.4 | |
| 0.00 | 1.24 | 0.00 | 0.61 | 6.41 | 206.85 | -2.07 | 100.92 | 0.0367 | 856.0 | 659.5 | |
| 0.00 | 3.53 | 0.00 | 1.75 | 8.25 | 206.54 | -2.38 | 58.65 | 0.0484 | 1205.0 | 1025.7 | |
| 0.00 | 0.97 | 0.00 | 0.48 | 7.95 | 206.54 | -2.38 | 64.28 | 0.0459 | 970.0 | 846.2 | |
| 1.50 | 5.74 | 0.74 | 2.85 | 8.73 | 206.51 | -2.41 | 51.23 | 0.0536 | 1151.1 | 825.9 | |
| 0.00 | 1.41 | 0.00 | 0.70 | 7.67 | 206.45 | -2.47 | 70.54 | 0.0455 | 1081.0 | 835.6 | |
| 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. | |