SDO HMI 2014-09-12 20:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.34 | 0.00 | 19.25 | -20.30 | 105.91 | 41.39 | 234.99 | 0.7583 | 301.9 | 290.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 4.89 | 0.00 | 3.98 | -19.98 | 110.16 | 45.64 | 237.88 | 0.7956 | 614.0 | 434.6 | |
| 0.00 | 1.33 | 0.00 | 1.04 | -20.68 | 107.26 | 42.74 | 235.46 | 0.7730 | 579.0 | 510.3 | |
| 0.00 | 2.13 | 0.00 | 1.65 | -20.39 | 107.03 | 42.51 | 235.66 | 0.7693 | 605.0 | 507.1 | |
| 0.00 | 1.69 | 0.00 | 1.32 | -21.34 | 107.05 | 42.53 | 234.60 | 0.7748 | 589.0 | 485.1 | |
| 0.00 | 1.33 | 0.00 | 1.01 | -19.76 | 106.00 | 41.48 | 235.76 | 0.7563 | 664.0 | 493.3 | |
| 0.00 | 0.80 | 0.00 | 0.60 | -19.58 | 105.81 | 41.29 | 235.86 | 0.7535 | 538.0 | 481.6 | |
| 0.00 | 1.07 | 0.00 | 0.79 | -19.12 | 105.54 | 41.02 | 236.22 | 0.7483 | 652.0 | 570.0 | |
| 0.00 | 3.82 | 0.00 | 2.89 | -20.56 | 105.53 | 41.01 | 234.55 | 0.7564 | 684.0 | 533.9 | |
| 0.00 | 1.25 | 0.00 | 0.94 | -20.60 | 105.24 | 40.72 | 234.32 | 0.7540 | 552.0 | 506.4 | |
| 0.00 | 0.98 | 0.00 | 0.73 | -20.28 | 104.63 | 40.11 | 234.30 | 0.7464 | 660.0 | 545.0 | |
| 0.00 | 1.33 | 0.00 | 0.95 | -18.98 | 102.72 | 38.20 | 234.56 | 0.7201 | -512.0 | -463.3 | |
| 0.00 | 1.96 | 0.00 | 1.37 | -18.77 | 101.81 | 37.29 | 234.18 | 0.7098 | -665.0 | -571.1 | |
| 0.00 | 1.60 | 0.00 | 1.15 | -20.83 | 101.89 | 37.37 | 231.81 | 0.7241 | -62.0 | -93.2 | |
| 0.00 | 1.16 | 0.00 | 0.83 | -23.95 | 99.27 | 34.75 | 226.33 | 0.7225 | -671.0 | -576.1 | |
| 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. | |