SDO HMI 2014-09-19 18:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.09 | 30.20 | 4.39 | 18.49 | -21.01 | 310.46 | -22.76 | 142.07 | 0.5887 | -301.7 | -229.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.57 | -19.31 | 313.72 | -19.49 | 144.32 | 0.5419 | 624.0 | 516.7 | |
| 0.00 | 3.10 | 0.00 | 1.82 | -18.92 | 313.47 | -19.75 | 143.52 | 0.5396 | 951.0 | 757.7 | |
| 0.00 | 0.97 | 0.00 | 0.57 | -18.91 | 313.06 | -20.15 | 142.95 | 0.5429 | 451.0 | 404.8 | |
| 0.00 | 1.24 | 0.00 | 0.74 | -20.00 | 312.71 | -20.50 | 143.73 | 0.5584 | 766.0 | 553.2 | |
| 0.00 | 1.15 | 0.00 | 0.68 | -18.63 | 312.49 | -20.73 | 141.85 | 0.5450 | 675.0 | 582.7 | |
| 0.80 | 2.57 | 0.49 | 1.59 | -21.75 | 310.26 | -22.96 | 142.59 | 0.5986 | -932.0 | -845.5 | |
| 1.77 | 3.54 | 1.09 | 2.18 | -21.08 | 310.02 | -23.19 | 141.57 | 0.5935 | -753.2 | -540.1 | |
| 0.00 | 0.89 | 0.00 | 0.55 | -21.91 | 309.70 | -23.52 | 142.12 | 0.6051 | -821.0 | -667.9 | |
| 0.00 | 1.15 | 0.00 | 0.71 | -21.29 | 309.81 | -23.41 | 141.56 | 0.5976 | -770.0 | -519.1 | |
| 0.00 | 1.51 | 0.00 | 0.94 | -22.30 | 309.49 | -23.73 | 142.29 | 0.6110 | -566.0 | -434.9 | |
| 0.53 | 2.57 | 0.33 | 1.60 | -22.03 | 309.43 | -23.78 | 141.93 | 0.6086 | -717.2 | -584.1 | |
| 2.48 | 8.15 | 1.54 | 5.06 | -21.65 | 309.46 | -23.75 | 141.56 | 0.6044 | -931.9 | -657.1 | |
| 0.00 | 2.39 | 0.00 | 1.48 | -21.21 | 309.40 | -23.82 | 140.99 | 0.6003 | -640.0 | -574.0 | |
| 1.51 | -12.00 | 0.94 | -12.00 | -21.63 | 309.18 | -24.03 | 141.21 | 0.6066 | -760.9 | 999999 | |
| 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. | |