SDO HMI 2014-07-22 03:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.02 | 163.58 | 23.10 | 102.44 | -20.98 | 68.93 | 27.76 | 225.38 | 0.6130 | 359.0 | 210.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.95 | 124.02 | 15.71 | 78.15 | -20.89 | 69.67 | 28.50 | 226.27 | 0.6192 | 1008.5 | 296.9 | |
| 2.36 | 15.33 | 1.47 | 9.54 | -20.84 | 68.37 | 27.20 | 225.05 | 0.6058 | 807.9 | 440.8 | |
| 2.36 | -2.00 | 1.47 | -2.00 | -21.07 | 68.38 | 27.21 | 224.76 | 0.6081 | 689.5 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.50 | -20.49 | 68.12 | 26.95 | 225.23 | 0.6002 | 759.0 | 717.1 | |
| 0.00 | 1.45 | 0.00 | 0.91 | -21.95 | 68.18 | 27.02 | 223.50 | 0.6143 | -659.0 | -574.5 | |
| 0.00 | 1.45 | 0.00 | 0.89 | -19.79 | 67.48 | 26.31 | 225.46 | 0.5874 | 373.0 | 441.8 | |
| 0.00 | 1.27 | 0.00 | 0.77 | -20.91 | 66.09 | 24.92 | 222.54 | 0.5844 | -679.0 | -517.9 | |
| 1.27 | 2.63 | 0.77 | 1.60 | -21.26 | 65.43 | 24.26 | 221.37 | 0.5817 | -785.5 | -646.7 | |
| 0.00 | 0.73 | 0.00 | 0.44 | -21.93 | 65.37 | 24.21 | 220.49 | 0.5880 | -532.0 | -449.5 | |
| 0.00 | 2.18 | 0.00 | 1.33 | -21.93 | 65.15 | 23.99 | 220.25 | 0.5859 | -540.0 | -441.4 | |
| 0.00 | 2.81 | 0.00 | 1.71 | -21.65 | 65.11 | 23.94 | 220.52 | 0.5826 | -854.0 | -688.1 | |
| 4.72 | 6.99 | 2.86 | 4.24 | -21.67 | 64.79 | 23.62 | 220.12 | 0.5799 | -928.9 | -769.0 | |
| 0.00 | 1.00 | 0.00 | 0.60 | -20.85 | 64.61 | 23.45 | 220.92 | 0.5699 | -807.0 | -687.4 | |
| 1.36 | 2.90 | 0.82 | 1.76 | -22.12 | 63.86 | 22.69 | 218.51 | 0.5762 | -829.6 | -650.9 | |
| 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. | |