SDO HMI 2014-07-22 11:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.49 | 130.20 | 19.99 | 85.51 | -21.02 | 68.96 | 32.17 | 229.35 | 0.6572 | 454.6 | 203.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.79 | 101.62 | 11.11 | 67.21 | -20.97 | 69.87 | 33.08 | 230.21 | 0.6657 | 1023.4 | 275.0 | |
| 4.63 | -1.00 | 3.04 | -1.00 | -20.80 | 69.24 | 32.46 | 229.90 | 0.6582 | 940.6 | 999999 | |
| 3.36 | -1.00 | 2.20 | -1.00 | -20.83 | 69.05 | 32.27 | 229.72 | 0.6565 | 923.9 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.70 | -20.34 | 68.14 | 31.35 | 229.55 | 0.6434 | 725.0 | 568.5 | |
| 2.36 | 8.44 | 1.53 | 5.49 | -21.19 | 68.18 | 31.40 | 228.53 | 0.6505 | 773.5 | 606.4 | |
| 0.00 | 2.81 | 0.00 | 1.80 | -19.88 | 67.65 | 30.87 | 229.71 | 0.6349 | 638.0 | 555.4 | |
| 0.00 | 3.36 | 0.00 | 2.17 | -22.62 | 66.19 | 29.41 | 225.00 | 0.6432 | -449.0 | -333.4 | |
| 0.00 | 1.18 | 0.00 | 0.75 | -21.72 | 65.79 | 29.01 | 225.72 | 0.6316 | -576.0 | -483.5 | |
| 0.00 | 2.54 | 0.00 | 1.62 | -21.81 | 65.55 | 28.77 | 225.38 | 0.6300 | -703.0 | -524.6 | |
| 0.00 | 1.36 | 0.00 | 0.86 | -21.22 | 65.35 | 28.57 | 225.91 | 0.6229 | -808.0 | -656.1 | |
| 0.00 | 1.00 | 0.00 | 0.63 | -21.54 | 64.93 | 28.15 | 225.11 | 0.6217 | -829.0 | -633.1 | |
| 2.81 | 5.08 | 1.77 | 3.20 | -21.60 | 64.72 | 27.94 | 224.83 | 0.6202 | -893.4 | -731.3 | |
| 0.54 | 1.72 | 0.34 | 1.08 | -22.06 | 63.64 | 26.85 | 223.17 | 0.6141 | -848.3 | -709.8 | |
| 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. | |