SDO HMI 2014-07-08 18:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.33 | 172.95 | 13.43 | 88.30 | 6.41 | 204.54 | -13.63 | 78.06 | 0.2408 | -859.9 | -430.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.73 | 0.00 | 0.37 | 5.20 | 206.72 | -11.45 | 81.92 | 0.2006 | -814.0 | -653.1 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 6.20 | 206.26 | -11.91 | 77.46 | 0.2111 | -804.0 | -677.2 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 11.06 | 205.83 | -12.34 | 58.19 | 0.2480 | -733.0 | -686.5 | |
| 0.82 | 3.63 | 0.42 | 1.85 | 7.08 | 205.61 | -12.55 | 74.20 | 0.2252 | -1148.7 | -900.5 | |
| 0.00 | 3.09 | 0.00 | 1.57 | 4.09 | 205.24 | -12.93 | 87.71 | 0.2244 | -664.0 | -658.3 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 11.57 | 204.78 | -13.39 | 58.46 | 0.2673 | -860.0 | -642.8 | |
| 25.51 | 150.79 | 13.01 | 76.90 | 6.27 | 204.69 | -13.48 | 78.48 | 0.2375 | -1408.5 | -443.7 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 9.20 | 204.47 | -13.70 | 67.20 | 0.2547 | -763.0 | -555.4 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 9.01 | 203.78 | -14.39 | 68.82 | 0.2644 | -877.0 | -651.0 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 5.51 | 202.53 | -15.64 | 82.67 | 0.2718 | -675.0 | -538.2 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 7.00 | 202.32 | -15.85 | 77.40 | 0.2789 | -847.0 | -759.0 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 6.20 | 202.03 | -16.14 | 80.40 | 0.2815 | 707.0 | 587.8 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 5.90 | 201.97 | -16.20 | 81.50 | 0.2817 | 993.0 | 778.5 | |
| 0.00 | 1.72 | 0.00 | 0.92 | 8.83 | 197.34 | -20.83 | 74.99 | 0.3653 | 861.0 | 659.4 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 6.17 | 197.21 | -20.96 | 82.33 | 0.3604 | 844.0 | 725.2 | |
| 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. | |