SDO HMI 2014-02-25 10:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.86 | 146.36 | 32.30 | 112.20 | 8.38 | 132.55 | -47.23 | 72.53 | 0.7632 | 408.4 | 118.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.78 | 0.00 | 0.53 | 13.53 | 141.38 | -38.39 | 61.57 | 0.6890 | -535.0 | -424.7 | |
| 0.00 | 2.24 | 0.00 | 1.45 | 7.28 | 142.24 | -37.54 | 69.69 | 0.6468 | -806.0 | -689.4 | |
| 0.00 | 1.12 | 0.00 | 0.73 | 7.26 | 141.36 | -38.41 | 70.18 | 0.6575 | -590.0 | -462.0 | |
| 0.00 | 0.86 | 0.00 | 0.57 | 8.02 | 140.67 | -39.11 | 69.45 | 0.6694 | -702.0 | -565.6 | |
| 0.00 | 1.46 | 0.00 | 0.97 | 7.76 | 140.50 | -39.27 | 69.91 | 0.6702 | -616.0 | -556.2 | |
| 0.00 | 1.29 | 0.00 | 0.87 | 8.01 | 140.12 | -39.65 | 69.75 | 0.6759 | -742.0 | -646.1 | |
| 0.00 | 1.64 | 0.00 | 1.11 | 8.87 | 139.39 | -40.39 | 68.94 | 0.6884 | -692.0 | -565.8 | |
| 2.58 | 4.31 | 1.88 | 3.13 | 7.33 | 134.92 | -44.85 | 72.99 | 0.7339 | -554.7 | -372.9 | |
| 0.00 | 1.46 | 0.00 | 1.10 | 6.81 | 132.87 | -46.90 | 74.42 | 0.7550 | -550.0 | -429.6 | |
| 8.01 | 36.87 | 6.16 | 28.33 | 8.82 | 132.36 | -47.42 | 72.07 | 0.7671 | 949.1 | 401.0 | |
| 0.00 | 6.03 | 0.00 | 4.57 | 6.99 | 132.59 | -47.19 | 74.29 | 0.7587 | 261.0 | 282.2 | |
| 0.00 | 2.33 | 0.00 | 1.79 | 7.78 | 132.08 | -47.70 | 73.49 | 0.7667 | 533.0 | 509.0 | |
| 30.49 | 85.97 | 23.65 | 67.05 | 8.36 | 131.76 | -48.02 | 72.88 | 0.7719 | 703.8 | 69.3 | |
| 0.78 | -13.00 | 0.61 | -13.00 | 9.14 | 131.63 | -48.15 | 71.96 | 0.7758 | 432.7 | 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. | |