SDO HMI 2014-09-08 15:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.17 | 37.90 | 5.69 | 21.10 | 9.36 | 147.43 | 27.33 | 276.43 | 0.4575 | -114.0 | -75.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.57 | 6.51 | 2.03 | 3.70 | 9.19 | 149.70 | 29.59 | 275.90 | 0.4920 | -897.0 | -634.0 | |
| 0.00 | 3.39 | 0.00 | 1.92 | 9.55 | 149.31 | 29.20 | 276.66 | 0.4864 | -948.0 | -730.8 | |
| 0.00 | 1.25 | 0.00 | 0.71 | 9.74 | 149.22 | 29.12 | 277.05 | 0.4852 | -795.0 | -488.7 | |
| 0.53 | 1.96 | 0.30 | 1.11 | 9.32 | 149.14 | 29.04 | 276.19 | 0.4838 | -945.2 | -808.2 | |
| 1.96 | 5.53 | 1.09 | 3.08 | 8.89 | 147.72 | 27.61 | 275.36 | 0.4618 | -782.1 | -623.0 | |
| 0.45 | 1.34 | 0.25 | 0.74 | 10.17 | 147.04 | 26.93 | 278.25 | 0.4523 | 751.4 | 652.3 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 8.83 | 146.68 | 26.58 | 275.29 | 0.4458 | -842.0 | -651.9 | |
| 1.25 | 2.32 | 0.69 | 1.28 | 8.72 | 146.50 | 26.40 | 275.05 | 0.4430 | -792.0 | -712.1 | |
| 1.25 | 4.55 | 0.69 | 2.52 | 10.38 | 146.61 | 26.50 | 278.78 | 0.4460 | 985.4 | 763.7 | |
| 1.16 | 4.01 | 0.64 | 2.20 | 8.82 | 145.83 | 25.72 | 275.31 | 0.4325 | 799.9 | 410.2 | |
| 0.00 | 2.14 | 0.00 | 1.17 | 10.07 | 145.66 | 25.55 | 278.24 | 0.4309 | 745.0 | 510.6 | |
| 0.00 | 1.07 | 0.00 | 0.58 | 9.81 | 145.30 | 25.19 | 277.70 | 0.4250 | 894.0 | 724.9 | |
| 0.00 | 1.60 | 0.00 | 0.88 | 9.55 | 145.07 | 24.97 | 277.12 | 0.4213 | 874.0 | 557.6 | |
| 0.00 | 1.25 | 0.00 | 0.67 | 8.37 | 142.71 | 22.61 | 274.42 | 0.3831 | 715.0 | 646.1 | |
| 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. | |