SDO HMI 2014-07-20 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 |
| 66.76 | 211.89 | 37.19 | 118.15 | -21.25 | 68.25 | 7.77 | 196.00 | 0.4594 | 126.7 | 152.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.78 | 147.67 | 8.82 | 82.43 | -21.22 | 69.57 | 9.09 | 198.59 | 0.4642 | 1047.0 | 358.5 | |
| 2.63 | -1.00 | 1.47 | -1.00 | -21.09 | 69.47 | 8.99 | 198.48 | 0.4616 | 1218.7 | 999999 | |
| 15.60 | -1.00 | 8.68 | -1.00 | -20.88 | 69.26 | 8.78 | 198.23 | 0.4576 | 1228.9 | 999999 | |
| 0.91 | -1.00 | 0.51 | -1.00 | -21.18 | 69.04 | 8.56 | 197.60 | 0.4610 | 692.1 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -20.37 | 68.67 | 8.19 | 197.45 | 0.4472 | 582.0 | 459.4 | |
| 2.54 | 3.99 | 1.40 | 2.20 | -19.99 | 68.06 | 7.58 | 196.48 | 0.4387 | 958.6 | 758.9 | |
| 0.00 | 2.72 | 0.00 | 1.50 | -20.37 | 66.54 | 6.06 | 193.10 | 0.4385 | -892.0 | -644.9 | |
| 0.00 | 3.36 | 0.00 | 1.86 | -21.38 | 66.05 | 5.57 | 191.58 | 0.4523 | -479.0 | -392.6 | |
| 2.72 | 5.99 | 1.52 | 3.34 | -22.06 | 65.62 | 5.14 | 190.41 | 0.4613 | -867.2 | -726.0 | |
| 0.00 | 4.44 | 0.00 | 2.49 | -22.40 | 65.56 | 5.08 | 190.16 | 0.4664 | -715.0 | -640.9 | |
| 13.70 | 20.95 | 7.60 | 11.64 | -21.58 | 65.34 | 4.86 | 190.05 | 0.4532 | -1152.1 | -734.9 | |
| 5.08 | 21.50 | 2.84 | 11.99 | -22.30 | 65.03 | 4.55 | 189.15 | 0.4634 | -804.8 | -739.8 | |
| 7.80 | -12.00 | 4.35 | -12.00 | -22.05 | 64.83 | 4.35 | 188.83 | 0.4592 | -990.2 | 999999 | |
| 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. | |