SDO HMI 2014-10-10 03:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.13 | 0.00 | 9.13 | -20.57 | 73.02 | 8.69 | 198.43 | 0.4807 | 467.4 | 375.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.51 | -21.45 | 80.71 | 16.38 | 209.69 | 0.5321 | 688.0 | 520.7 | |
| 0.00 | 1.05 | 0.00 | 0.58 | -15.17 | 77.71 | 13.38 | 211.68 | 0.4272 | 671.0 | 588.8 | |
| 0.00 | 1.75 | 0.00 | 0.97 | -17.37 | 76.38 | 12.05 | 206.60 | 0.4470 | 624.0 | 583.7 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -16.95 | 75.36 | 11.04 | 205.05 | 0.4343 | 777.0 | 579.5 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -18.81 | 74.70 | 10.38 | 202.03 | 0.4566 | 769.0 | 697.2 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -18.01 | 74.50 | 10.17 | 202.32 | 0.4440 | 857.0 | 734.3 | |
| 0.00 | 1.14 | 0.00 | 0.63 | -18.77 | 74.51 | 10.18 | 201.68 | 0.4550 | 861.0 | 715.5 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -19.06 | 74.24 | 9.91 | 200.91 | 0.4577 | 712.0 | 516.0 | |
| 0.00 | 2.02 | 0.00 | 1.12 | -19.03 | 74.04 | 9.72 | 200.57 | 0.4561 | 805.0 | 702.0 | |
| 0.00 | 1.05 | 0.00 | 0.61 | -23.17 | 73.79 | 9.46 | 197.16 | 0.5144 | 761.0 | 635.7 | |
| 0.00 | 0.96 | 0.00 | 0.56 | -23.74 | 73.03 | 8.71 | 195.54 | 0.5194 | 692.0 | 569.9 | |
| 0.00 | 0.96 | 0.00 | 0.55 | -22.42 | 69.55 | 5.23 | 189.97 | 0.4883 | -569.0 | -467.2 | |
| 0.00 | 1.75 | 0.00 | 1.00 | -23.63 | 67.47 | 3.14 | 185.76 | 0.5023 | -678.0 | -584.2 | |
| 0.00 | 0.79 | 0.00 | 0.51 | -32.89 | 56.37 | -7.95 | 169.55 | 0.6430 | -426.0 | -384.3 | |
| 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. | |