SDO HMI 2014-09-08 18:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.09 | 42.35 | 7.45 | 23.88 | 9.42 | 147.18 | 28.73 | 276.43 | 0.4790 | 2.5 | 9.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.65 | 5.53 | 2.12 | 3.20 | 9.23 | 149.89 | 31.44 | 275.87 | 0.5196 | -874.3 | -639.4 | |
| 3.12 | 5.44 | 1.80 | 3.14 | 9.56 | 149.52 | 31.08 | 276.52 | 0.5144 | -930.1 | -712.8 | |
| 0.00 | 2.32 | 0.00 | 1.33 | 9.29 | 149.39 | 30.94 | 276.01 | 0.5123 | -823.0 | -767.0 | |
| 0.00 | 3.39 | 0.00 | 1.92 | 9.01 | 147.73 | 29.29 | 275.51 | 0.4874 | -885.0 | -745.8 | |
| 0.71 | 1.87 | 0.40 | 1.06 | 10.10 | 147.17 | 28.73 | 277.83 | 0.4796 | 783.4 | 601.7 | |
| 0.00 | 0.98 | 0.00 | 0.55 | 8.92 | 146.68 | 28.23 | 275.38 | 0.4713 | -725.0 | -589.7 | |
| 1.78 | 3.12 | 1.00 | 1.75 | 8.74 | 146.56 | 28.11 | 275.01 | 0.4695 | -908.0 | -720.9 | |
| 1.25 | 2.85 | 0.70 | 1.60 | 10.47 | 146.65 | 28.20 | 278.67 | 0.4720 | 892.4 | 735.6 | |
| 1.78 | 3.03 | 0.99 | 1.69 | 8.88 | 145.78 | 27.33 | 275.34 | 0.4575 | 763.8 | 584.4 | |
| 0.00 | 2.14 | 0.00 | 1.19 | 9.61 | 145.70 | 27.26 | 276.95 | 0.4568 | 778.0 | 664.8 | |
| 0.00 | 3.48 | 0.00 | 1.93 | 9.98 | 145.70 | 27.25 | 277.75 | 0.4571 | 359.0 | 282.1 | |
| 0.80 | 2.23 | 0.44 | 1.23 | 9.89 | 145.14 | 26.70 | 277.63 | 0.4484 | 980.9 | 783.1 | |
| 0.00 | 2.58 | 0.00 | 1.43 | 9.56 | 145.08 | 26.63 | 276.90 | 0.4471 | 978.0 | 756.1 | |
| 0.00 | 2.05 | 0.00 | 1.13 | 9.11 | 144.90 | 26.46 | 275.92 | 0.4441 | 229.0 | 214.9 | |
| 0.00 | 1.34 | 0.00 | 0.73 | 8.59 | 143.40 | 24.96 | 274.81 | 0.4205 | 679.0 | 514.1 | |
| 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. | |