SDO HMI 2014-07-05 21:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.51 | 0.00 | 12.52 | 4.70 | 263.04 | 6.83 | 210.66 | 0.2099 | 633.4 | 408.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.09 | 0.00 | 1.17 | 4.76 | 283.85 | 27.64 | 273.83 | 0.4652 | -327.0 | -314.7 | |
| 0.00 | 3.36 | 0.00 | 1.79 | 4.27 | 278.10 | 21.89 | 273.07 | 0.3739 | -828.0 | -533.2 | |
| 0.00 | 2.36 | 0.00 | 1.22 | -3.98 | 270.21 | 14.00 | 242.40 | 0.2735 | 1020.0 | 790.8 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 9.47 | 267.00 | 10.79 | 300.17 | 0.2146 | 755.0 | 565.5 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 1.45 | 266.57 | 10.36 | 259.75 | 0.1835 | 707.0 | 522.1 | |
| 0.00 | 2.09 | 0.00 | 1.05 | 10.18 | 264.01 | 7.80 | 311.70 | 0.1798 | 1092.0 | 845.1 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 6.99 | 259.78 | 3.57 | 315.71 | 0.0889 | 684.0 | 555.8 | |
| 0.00 | 2.36 | 0.00 | 1.17 | 5.90 | 259.28 | 3.07 | 309.70 | 0.0696 | 1038.0 | 834.8 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 7.82 | 251.60 | -4.61 | 45.62 | 0.1119 | 853.0 | 691.7 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 4.31 | 250.77 | -5.44 | 79.95 | 0.0965 | 844.0 | 636.2 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 7.45 | 250.65 | -5.56 | 53.34 | 0.1203 | 867.0 | 644.3 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 6.17 | 250.45 | -5.76 | 63.77 | 0.1118 | 785.0 | 587.6 | |
| 0.00 | 2.81 | 0.00 | 1.41 | 3.48 | 248.71 | -7.49 | 88.92 | 0.1308 | 453.0 | 508.5 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 0.30 | 247.22 | -8.99 | 108.67 | 0.1657 | 924.0 | 674.8 | |
| 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. | |