SDO HMI 2014-04-29 14:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.70 | 147.83 | 18.32 | 113.30 | -23.31 | 114.20 | 47.64 | 242.82 | 0.7650 | 373.2 | 212.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.16 | 0.00 | 0.85 | -17.96 | 113.04 | 46.49 | 249.49 | 0.7389 | -626.0 | -454.8 | |
| 0.00 | 1.78 | 0.00 | 1.30 | -18.53 | 112.82 | 46.27 | 248.67 | 0.7378 | -244.0 | -263.2 | |
| 23.70 | 130.54 | 18.32 | 100.93 | -23.34 | 114.72 | 48.16 | 242.98 | 0.7702 | 992.0 | 306.6 | |
| 0.00 | 1.07 | 0.00 | 0.80 | -21.78 | 113.23 | 46.68 | 244.53 | 0.7507 | -536.0 | -424.2 | |
| 0.00 | 2.49 | 0.00 | 1.86 | -21.94 | 113.21 | 46.65 | 244.31 | 0.7509 | -64.0 | -173.2 | |
| 0.00 | 0.71 | 0.00 | 0.52 | -21.17 | 112.05 | 45.49 | 244.95 | 0.7364 | -283.0 | -374.1 | |
| 0.00 | 0.80 | 0.00 | 0.58 | -22.78 | 110.57 | 44.02 | 242.32 | 0.7258 | -396.0 | -412.3 | |
| 0.00 | 1.34 | 0.00 | 0.96 | -22.72 | 110.41 | 43.86 | 242.34 | 0.7239 | -625.0 | -499.3 | |
| 0.00 | 3.30 | 0.00 | 2.34 | -22.46 | 109.86 | 43.30 | 242.48 | 0.7170 | -592.0 | -533.5 | |
| 0.00 | 0.36 | 0.00 | 0.25 | -25.92 | 108.08 | 41.53 | 237.15 | 0.7121 | -641.0 | -593.8 | |
| 0.00 | 0.71 | 0.00 | 0.51 | -27.48 | 108.56 | 42.00 | 235.35 | 0.7240 | -615.0 | -526.8 | |
| 0.00 | 1.34 | 0.00 | 0.93 | -27.58 | 106.26 | 39.70 | 234.07 | 0.7015 | -676.0 | -534.3 | |
| 0.00 | 1.16 | 0.00 | 0.79 | -27.68 | 104.72 | 38.16 | 233.11 | 0.6865 | -616.0 | -406.6 | |
| 0.00 | 1.07 | 0.00 | 0.68 | -30.61 | 97.59 | 31.03 | 224.46 | 0.6358 | -570.0 | -482.1 | |
| 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. | |