SDO HMI 2014-09-12 18:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.51 | 23.76 | 1.14 | 17.82 | -20.67 | 106.10 | 40.47 | 233.99 | 0.7523 | 149.6 | 295.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 4.54 | 0.00 | 3.61 | -19.98 | 110.13 | 44.50 | 237.27 | 0.7853 | 565.0 | 457.6 | |
| 0.62 | 1.60 | 0.48 | 1.22 | -20.69 | 107.28 | 41.65 | 234.80 | 0.7631 | 549.6 | 467.4 | |
| 0.00 | 2.85 | 0.00 | 2.16 | -20.37 | 107.04 | 41.42 | 235.03 | 0.7591 | 701.0 | 594.3 | |
| 0.00 | 1.33 | 0.00 | 1.02 | -21.15 | 107.09 | 41.46 | 234.17 | 0.7640 | 327.0 | 283.7 | |
| 0.00 | 1.25 | 0.00 | 0.95 | -21.35 | 107.03 | 41.40 | 233.91 | 0.7645 | 652.0 | 517.6 | |
| 0.00 | 2.49 | 0.00 | 1.85 | -19.74 | 106.03 | 40.41 | 235.12 | 0.7460 | 635.0 | 538.7 | |
| 0.89 | 3.65 | 0.66 | 2.70 | -20.51 | 105.55 | 39.93 | 233.93 | 0.7460 | 665.1 | 569.8 | |
| 0.00 | 0.53 | 0.00 | 0.40 | -20.67 | 105.48 | 39.85 | 233.69 | 0.7463 | 435.0 | 397.5 | |
| 0.00 | 0.80 | 0.00 | 0.61 | -22.56 | 105.68 | 40.06 | 231.69 | 0.7597 | 304.0 | 321.6 | |
| 0.00 | 1.25 | 0.00 | 0.87 | -19.19 | 102.67 | 37.04 | 233.50 | 0.7100 | -579.0 | -418.0 | |
| 0.00 | 0.27 | 0.00 | 0.19 | -19.04 | 102.47 | 36.84 | 233.54 | 0.7071 | -382.0 | -444.3 | |
| 0.00 | 0.71 | 0.00 | 0.49 | -18.75 | 101.72 | 36.09 | 233.34 | 0.6976 | -574.0 | -437.4 | |
| 0.00 | 1.07 | 0.00 | 0.75 | -23.69 | 99.22 | 33.59 | 225.69 | 0.7104 | -543.0 | -517.2 | |
| 0.00 | 1.42 | 0.00 | 1.00 | -23.90 | 99.24 | 33.61 | 225.47 | 0.7122 | -678.0 | -606.6 | |
| 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. | |