SDO HMI 2014-07-08 19:00:40 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 | 14.73 | -22.64 | 200.39 | -17.22 | 148.41 | 0.5224 | 272.4 | 195.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.61 | -20.95 | 206.36 | -11.26 | 156.31 | 0.4556 | 931.0 | 710.0 | |
| 0.00 | 0.82 | 0.00 | 0.46 | -21.71 | 204.99 | -12.63 | 154.57 | 0.4750 | 663.0 | 573.2 | |
| 0.00 | 4.09 | 0.00 | 2.32 | -22.04 | 203.16 | -14.45 | 151.83 | 0.4920 | 740.0 | 585.1 | |
| 0.00 | 1.63 | 0.00 | 0.93 | -21.70 | 203.20 | -14.41 | 151.54 | 0.4873 | 847.0 | 640.4 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -22.28 | 202.97 | -14.65 | 151.77 | 0.4965 | 576.0 | 437.9 | |
| 0.00 | 1.82 | 0.00 | 1.01 | -19.80 | 202.95 | -14.66 | 149.00 | 0.4643 | 821.0 | 633.8 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -20.63 | 202.87 | -14.74 | 149.82 | 0.4758 | 704.0 | 515.2 | |
| 0.00 | 3.81 | 0.00 | 2.31 | -27.04 | 200.16 | -17.45 | 152.27 | 0.5762 | -644.0 | -599.8 | |
| 0.00 | 1.18 | 0.00 | 0.71 | -26.45 | 199.69 | -17.93 | 151.09 | 0.5723 | -728.0 | -599.4 | |
| 0.00 | 3.63 | 0.00 | 2.12 | -22.69 | 199.20 | -18.42 | 146.54 | 0.5307 | 786.0 | 741.8 | |
| 0.00 | 1.09 | 0.00 | 0.64 | -22.86 | 199.17 | -18.44 | 146.70 | 0.5329 | 732.0 | 644.0 | |
| 0.00 | 0.91 | 0.00 | 0.54 | -21.58 | 195.65 | -21.97 | 140.53 | 0.5492 | -396.0 | -410.2 | |
| 0.00 | 2.27 | 0.00 | 1.34 | -20.92 | 195.22 | -22.39 | 139.17 | 0.5462 | -606.0 | -474.1 | |
| 0.00 | 1.00 | 0.00 | 0.61 | -18.84 | 189.96 | -27.66 | 130.56 | 0.5804 | -613.0 | -449.7 | |
| 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. | |