SDO HMI 2014-09-09 03:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.44 | 42.28 | 8.71 | 25.13 | 9.51 | 147.29 | 33.81 | 276.30 | 0.5539 | 23.7 | 60.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.99 | 13.47 | 3.08 | 8.29 | 9.38 | 150.28 | 36.80 | 275.97 | 0.5965 | -699.2 | -549.8 | |
| 2.94 | -1.00 | 1.81 | -1.00 | 9.63 | 150.16 | 36.68 | 276.40 | 0.5948 | -803.9 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.64 | 9.17 | 147.84 | 34.36 | 275.64 | 0.5621 | -639.0 | -462.9 | |
| 0.00 | 1.34 | 0.00 | 0.79 | 8.95 | 147.08 | 33.60 | 275.25 | 0.5511 | -605.0 | -477.8 | |
| 1.16 | 4.19 | 0.69 | 2.49 | 10.06 | 147.17 | 33.69 | 277.28 | 0.5527 | -826.5 | -620.7 | |
| 0.89 | 2.05 | 0.53 | 1.21 | 8.88 | 146.67 | 33.19 | 275.15 | 0.5451 | -764.7 | -679.1 | |
| 0.00 | 1.07 | 0.00 | 0.63 | 9.37 | 145.85 | 32.36 | 276.06 | 0.5332 | 679.0 | 545.2 | |
| 0.00 | 0.71 | 0.00 | 0.42 | 9.70 | 145.88 | 32.40 | 276.68 | 0.5339 | 396.0 | 372.5 | |
| 0.00 | 0.89 | 0.00 | 0.52 | 9.95 | 145.69 | 32.21 | 277.18 | 0.5312 | 420.0 | 339.7 | |
| 3.66 | 8.03 | 2.13 | 4.67 | 9.51 | 145.46 | 31.98 | 276.36 | 0.5277 | 892.5 | 628.1 | |
| 0.00 | 1.16 | 0.00 | 0.67 | 10.00 | 145.37 | 31.89 | 277.30 | 0.5266 | 553.0 | 453.2 | |
| 0.80 | 4.64 | 0.47 | 2.69 | 9.81 | 145.17 | 31.69 | 276.94 | 0.5235 | 895.2 | 640.6 | |
| 0.00 | 3.21 | 0.00 | 1.86 | 9.25 | 144.86 | 31.38 | 275.88 | 0.5187 | 802.0 | 560.2 | |
| 0.00 | 0.45 | 0.00 | 0.25 | 7.91 | 142.65 | 29.17 | 273.22 | 0.4854 | 181.0 | 281.8 | |
| 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. | |