SDO HMI 2014-08-09 10:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.61 | 25.19 | 1.95 | 13.81 | -18.78 | 160.74 | 1.47 | 183.28 | 0.4271 | 851.5 | 662.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.75 | -18.99 | 164.02 | 4.75 | 190.39 | 0.4362 | 719.0 | 562.7 | |
| 0.00 | 2.62 | 0.00 | 1.44 | -19.05 | 163.12 | 3.85 | 188.44 | 0.4348 | 770.0 | 616.5 | |
| 0.00 | 1.99 | 0.00 | 1.10 | -19.75 | 160.87 | 1.61 | 183.43 | 0.4420 | 927.0 | 837.0 | |
| 0.00 | 2.08 | 0.00 | 1.14 | -19.41 | 160.67 | 1.41 | 183.06 | 0.4365 | 924.0 | 713.6 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -20.22 | 160.52 | 1.25 | 182.63 | 0.4491 | 742.0 | 601.2 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -19.57 | 160.45 | 1.18 | 182.55 | 0.4390 | 981.0 | 726.5 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -16.24 | 160.43 | 1.17 | 182.91 | 0.3858 | 708.0 | 499.2 | |
| 3.61 | 8.13 | 1.95 | 4.39 | -17.16 | 160.31 | 1.04 | 182.50 | 0.4006 | 1050.8 | 731.0 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -19.64 | 160.19 | 0.93 | 181.99 | 0.4399 | 858.0 | 624.8 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -20.01 | 159.61 | 0.35 | 180.73 | 0.4455 | 881.0 | 666.1 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -21.41 | 159.61 | 0.35 | 180.69 | 0.4673 | 796.0 | 586.1 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -20.42 | 159.42 | 0.15 | 180.32 | 0.4519 | 760.0 | 641.9 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -20.11 | 159.32 | 0.05 | 180.11 | 0.4471 | 763.0 | 544.3 | |
| 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. | |