SDO HMI 2014-07-07 16:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.41 | 156.11 | 18.23 | 88.13 | 6.62 | 203.95 | -28.57 | 82.67 | 0.4808 | -712.8 | -393.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.61 | 5.43 | 205.54 | -26.97 | 85.00 | 0.4551 | 457.0 | 365.8 | |
| 0.00 | 0.82 | 0.00 | 0.46 | 6.71 | 205.16 | -27.35 | 82.28 | 0.4624 | -613.0 | -559.6 | |
| 8.44 | 11.26 | 4.72 | 6.29 | 7.16 | 205.03 | -27.48 | 81.33 | 0.4651 | -985.8 | -620.6 | |
| 0.00 | 0.64 | 0.00 | 0.36 | 4.47 | 204.86 | -27.66 | 87.15 | 0.4652 | -744.0 | -659.3 | |
| 23.15 | 130.12 | 13.05 | 73.32 | 6.49 | 204.10 | -28.42 | 82.92 | 0.4784 | -1263.1 | -431.7 | |
| 0.00 | 2.09 | 0.00 | 1.19 | 8.50 | 203.61 | -28.91 | 78.90 | 0.4892 | -641.0 | -414.7 | |
| 0.82 | 3.63 | 0.46 | 2.06 | 8.68 | 203.49 | -29.03 | 78.57 | 0.4914 | -778.3 | -611.5 | |
| 0.00 | 0.82 | 0.00 | 0.47 | 7.72 | 203.17 | -29.34 | 80.58 | 0.4942 | -624.0 | -465.8 | |
| 0.00 | 0.91 | 0.00 | 0.52 | 7.69 | 203.03 | -29.48 | 80.69 | 0.4962 | -584.0 | -497.9 | |
| 0.00 | 1.27 | 0.00 | 0.75 | 6.20 | 199.58 | -32.93 | 84.07 | 0.5455 | 801.0 | 656.8 | |
| 0.00 | 1.09 | 0.00 | 0.66 | 7.69 | 197.49 | -35.02 | 81.67 | 0.5769 | 749.0 | 669.8 | |
| 0.00 | 0.82 | 0.00 | 0.50 | 6.18 | 197.02 | -35.49 | 84.34 | 0.5823 | 642.0 | 492.3 | |
| 0.00 | 0.64 | 0.00 | 0.39 | 7.12 | 196.72 | -35.80 | 82.76 | 0.5873 | 637.0 | 525.3 | |
| 0.00 | 0.91 | 0.00 | 0.55 | 5.96 | 196.73 | -35.78 | 84.74 | 0.5862 | 645.0 | 537.1 | |
| 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. | |