SDO HMI 2014-04-28 12:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.78 | 201.67 | 23.78 | 126.51 | -23.46 | 114.78 | 33.91 | 236.49 | 0.6158 | 558.1 | 327.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.60 | 0.00 | 0.99 | -21.30 | 114.67 | 33.80 | 239.73 | 0.6023 | -777.0 | -558.3 | |
| 0.00 | 0.89 | 0.00 | 0.55 | -21.46 | 114.67 | 33.80 | 239.49 | 0.6031 | -645.0 | -525.2 | |
| 34.30 | 181.81 | 21.59 | 114.39 | -23.39 | 115.13 | 34.26 | 236.87 | 0.6192 | 1131.3 | 402.6 | |
| 0.00 | 1.60 | 0.00 | 1.01 | -24.29 | 115.08 | 34.21 | 235.52 | 0.6239 | 451.0 | 282.2 | |
| 1.34 | -3.00 | 0.84 | -3.00 | -23.85 | 114.82 | 33.96 | 236.00 | 0.6185 | 703.2 | 999999 | |
| 2.14 | 4.72 | 1.35 | 2.98 | -24.40 | 114.83 | 33.96 | 235.20 | 0.6218 | 748.9 | 582.1 | |
| 0.00 | 1.07 | 0.00 | 0.65 | -20.68 | 112.66 | 31.80 | 239.46 | 0.5745 | -754.0 | -601.2 | |
| 0.00 | 1.34 | 0.00 | 0.81 | -21.37 | 112.06 | 31.20 | 237.97 | 0.5712 | -527.0 | -503.8 | |
| 0.00 | 0.98 | 0.00 | 0.59 | -22.31 | 110.66 | 29.79 | 235.45 | 0.5603 | -716.0 | -590.5 | |
| 0.00 | 1.51 | 0.00 | 0.90 | -23.59 | 109.65 | 28.78 | 232.62 | 0.5574 | -791.0 | -651.8 | |
| 0.00 | 2.05 | 0.00 | 1.23 | -25.10 | 109.83 | 28.97 | 230.47 | 0.5707 | -736.0 | -554.7 | |
| 0.00 | 0.89 | 0.00 | 0.53 | -25.01 | 107.88 | 27.02 | 228.90 | 0.5484 | -664.0 | -539.8 | |
| 0.00 | 1.07 | 0.00 | 0.64 | -27.59 | 106.63 | 25.77 | 223.91 | 0.5577 | -830.0 | -671.0 | |
| 0.00 | 2.14 | 0.00 | 1.24 | -27.12 | 103.54 | 22.67 | 221.25 | 0.5224 | -625.0 | -570.0 | |
| 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. | |