SDO HMI 2014-10-12 11:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.86 | 0.00 | 9.75 | 13.73 | 56.89 | 23.33 | 290.91 | 0.4118 | 296.6 | 298.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.96 | 0.00 | 0.57 | 12.47 | 66.43 | 32.87 | 283.59 | 0.5473 | -685.0 | -678.0 | |
| 0.00 | 0.96 | 0.00 | 0.57 | 13.55 | 66.48 | 32.92 | 285.54 | 0.5506 | -550.0 | -448.0 | |
| 0.00 | 0.96 | 0.00 | 0.57 | 13.11 | 66.27 | 32.71 | 284.81 | 0.5465 | -712.0 | -587.8 | |
| 0.00 | 1.40 | 0.00 | 0.78 | 12.84 | 59.94 | 26.38 | 286.55 | 0.4538 | 749.0 | 620.7 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 18.60 | 60.41 | 26.85 | 298.04 | 0.4870 | -676.0 | -578.1 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 15.70 | 59.06 | 25.50 | 293.17 | 0.4526 | -463.0 | -561.8 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 12.73 | 55.29 | 21.72 | 288.90 | 0.3832 | 782.0 | 622.2 | |
| 0.00 | 3.68 | 0.00 | 1.97 | 13.45 | 54.79 | 21.23 | 291.06 | 0.3790 | 872.0 | 684.1 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 13.19 | 54.47 | 20.91 | 290.65 | 0.3729 | 951.0 | 711.5 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 13.75 | 53.21 | 19.64 | 293.18 | 0.3568 | 881.0 | 725.6 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 13.28 | 52.90 | 19.34 | 292.19 | 0.3497 | 678.0 | 613.0 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 9.24 | 52.20 | 18.64 | 280.94 | 0.3227 | 605.0 | 543.3 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 15.04 | 49.94 | 16.37 | 300.48 | 0.3173 | 797.0 | 702.2 | |
| 0.00 | 1.40 | 0.00 | 0.73 | 14.98 | 49.67 | 16.11 | 300.70 | 0.3132 | 923.0 | 765.3 | |
| 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. | |