SDO HMI 2014-05-15 05:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.48 | 64.23 | 15.24 | 35.69 | 8.23 | 195.26 | -24.70 | 65.86 | 0.4547 | -166.6 | 23.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.64 | 8.34 | 196.99 | -22.97 | 64.13 | 0.4308 | -810.0 | -663.8 | |
| 0.00 | 3.05 | 0.00 | 1.67 | 7.54 | 196.97 | -22.99 | 65.87 | 0.4260 | -875.0 | -793.6 | |
| 11.94 | 30.00 | 6.55 | 16.46 | 8.03 | 196.88 | -23.08 | 64.89 | 0.4305 | -1062.7 | -637.2 | |
| 3.59 | -3.00 | 1.97 | -3.00 | 7.76 | 196.76 | -23.20 | 65.59 | 0.4304 | -887.1 | 999999 | |
| 0.81 | -3.00 | 0.44 | -3.00 | 8.04 | 196.61 | -23.35 | 65.13 | 0.4343 | -718.6 | 999999 | |
| 0.36 | 1.26 | 0.20 | 0.69 | 8.48 | 196.15 | -23.81 | 64.63 | 0.4437 | -928.8 | -711.9 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 9.63 | 194.55 | -25.41 | 63.78 | 0.4736 | 687.0 | 490.7 | |
| 0.54 | 1.89 | 0.30 | 1.06 | 8.92 | 194.09 | -25.87 | 65.52 | 0.4756 | 1020.2 | 860.3 | |
| 1.71 | 3.68 | 0.96 | 2.08 | 8.96 | 193.78 | -26.18 | 65.70 | 0.4801 | 966.5 | 738.5 | |
| 1.26 | 20.39 | 0.71 | 11.51 | 8.19 | 193.66 | -26.30 | 67.28 | 0.4773 | 1028.2 | 754.5 | |
| 4.76 | -10.00 | 2.69 | -10.00 | 8.29 | 193.31 | -26.65 | 67.35 | 0.4828 | 958.8 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.66 | 8.08 | 193.26 | -26.70 | 67.81 | 0.4824 | 674.0 | 551.4 | |
| 2.51 | -10.00 | 1.42 | -10.00 | 8.54 | 193.19 | -26.77 | 66.96 | 0.4859 | 779.4 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.42 | 10.42 | 190.02 | -29.94 | 65.84 | 0.5401 | 640.0 | 526.4 | |
| 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. | |