SDO HMI 2014-08-15 06:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.67 | 40.76 | 9.88 | 24.15 | -17.54 | 105.22 | 23.09 | 222.99 | 0.5504 | 558.2 | 410.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.53 | 0.00 | 0.91 | -17.46 | 106.20 | 24.07 | 224.29 | 0.5593 | 595.0 | 474.6 | |
| 1.71 | 4.24 | 1.02 | 2.53 | -17.55 | 105.97 | 23.84 | 223.90 | 0.5579 | 749.7 | 512.3 | |
| 5.68 | 10.01 | 3.37 | 5.94 | -17.18 | 105.89 | 23.75 | 224.28 | 0.5533 | 1003.5 | 696.9 | |
| 0.00 | 2.53 | 0.00 | 1.50 | -17.50 | 105.72 | 23.59 | 223.66 | 0.5549 | 775.0 | 708.1 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -17.43 | 105.54 | 23.40 | 223.54 | 0.5523 | 845.0 | 793.6 | |
| 0.00 | 0.99 | 0.00 | 0.59 | -17.56 | 105.49 | 23.35 | 223.31 | 0.5531 | 573.0 | 499.0 | |
| 1.35 | 2.98 | 0.81 | 1.78 | -18.46 | 105.51 | 23.37 | 222.18 | 0.5626 | 749.7 | 557.8 | |
| 0.00 | 0.99 | 0.00 | 0.60 | -20.18 | 105.63 | 23.50 | 220.23 | 0.5816 | 701.0 | 505.6 | |
| 6.40 | 10.19 | 3.79 | 6.04 | -17.73 | 105.02 | 22.89 | 222.51 | 0.5504 | 910.0 | 696.5 | |
| 0.00 | 1.35 | 0.00 | 0.79 | -16.46 | 104.00 | 21.87 | 222.90 | 0.5269 | -554.0 | -360.3 | |
| 1.53 | 3.52 | 0.89 | 2.04 | -16.59 | 103.27 | 21.14 | 221.76 | 0.5210 | -920.8 | -679.0 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -16.99 | 102.53 | 20.40 | 220.24 | 0.5181 | -835.0 | -653.9 | |
| 0.00 | 0.63 | 0.00 | 0.38 | -20.49 | 102.84 | 20.71 | 216.40 | 0.5602 | 497.0 | 415.4 | |
| 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. | |