SDO HMI 2014-05-20 14:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.79 | 197.84 | 20.54 | 140.57 | -24.88 | 190.04 | 41.15 | 236.41 | 0.7188 | 521.4 | 261.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.73 | -25.72 | 191.95 | 43.06 | 236.30 | 0.7416 | 563.0 | 417.2 | |
| 28.79 | 180.83 | 20.54 | 128.99 | -24.70 | 190.42 | 41.53 | 236.86 | 0.7216 | 1082.2 | 329.2 | |
| 0.00 | 0.72 | 0.00 | 0.52 | -26.59 | 190.41 | 41.52 | 234.46 | 0.7308 | 510.0 | 412.2 | |
| 0.00 | 0.90 | 0.00 | 0.64 | -26.04 | 189.77 | 40.88 | 234.82 | 0.7217 | 310.0 | 383.3 | |
| 0.00 | 0.90 | 0.00 | 0.61 | -25.31 | 186.05 | 37.16 | 233.67 | 0.6801 | -608.0 | -441.4 | |
| 0.00 | 0.81 | 0.00 | 0.55 | -25.65 | 186.04 | 37.15 | 233.23 | 0.6820 | -603.0 | -544.6 | |
| 0.00 | 3.60 | 0.00 | 2.42 | -25.82 | 185.77 | 36.88 | 232.84 | 0.6802 | -830.0 | -668.2 | |
| 0.00 | 1.44 | 0.00 | 0.97 | -26.08 | 185.82 | 36.93 | 232.52 | 0.6823 | -651.0 | -508.9 | |
| 0.00 | 1.71 | 0.00 | 1.15 | -26.49 | 185.46 | 36.58 | 231.77 | 0.6812 | -642.0 | -498.5 | |
| 0.00 | 0.90 | 0.00 | 0.61 | -28.12 | 184.68 | 35.79 | 229.18 | 0.6839 | -507.0 | -380.2 | |
| 0.00 | 0.90 | 0.00 | 0.61 | -28.33 | 184.38 | 35.49 | 228.72 | 0.6823 | -563.0 | -495.4 | |
| 0.00 | 1.53 | 0.00 | 1.03 | -28.50 | 184.28 | 35.39 | 228.43 | 0.6825 | -695.0 | -512.5 | |
| 0.00 | 1.53 | 0.00 | 1.04 | -28.78 | 184.21 | 35.32 | 228.05 | 0.6838 | -568.0 | -459.7 | |
| 0.00 | 1.08 | 0.00 | 0.70 | -29.40 | 179.58 | 30.70 | 223.79 | 0.6449 | -457.0 | -393.2 | |
| 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. | |