SDO HMI 2014-03-03 20:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.86 | 192.68 | 47.17 | 127.57 | 7.71 | 134.02 | 38.77 | 290.42 | 0.6642 | 193.7 | 13.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.62 | 3.82 | 140.15 | 44.91 | 282.42 | 0.7236 | -387.0 | -363.5 | |
| 19.16 | 25.55 | 13.35 | 17.81 | 7.63 | 137.50 | 42.26 | 288.59 | 0.7056 | -806.9 | -393.7 | |
| 0.00 | 0.95 | 0.00 | 0.66 | 8.15 | 137.08 | 41.84 | 289.48 | 0.7027 | -546.0 | -540.2 | |
| 0.00 | 5.35 | 0.00 | 3.70 | 7.83 | 136.92 | 41.68 | 289.12 | 0.6995 | -898.0 | -752.1 | |
| 0.43 | 1.47 | 0.30 | 1.02 | 8.29 | 136.94 | 41.69 | 289.74 | 0.7016 | -604.2 | -494.8 | |
| 0.43 | 2.24 | 0.29 | 1.52 | 8.33 | 135.59 | 40.34 | 290.44 | 0.6859 | 559.0 | 406.3 | |
| 0.00 | 1.12 | 0.00 | 0.76 | 8.20 | 135.53 | 40.29 | 290.29 | 0.6847 | 591.0 | 430.1 | |
| 3.88 | 147.10 | 2.55 | 96.24 | 6.68 | 133.85 | 38.60 | 289.00 | 0.6577 | -923.8 | 56.6 | |
| 23.83 | -8.00 | 15.64 | -8.00 | 7.46 | 133.62 | 38.37 | 290.23 | 0.6583 | 752.9 | 999999 | |
| 1.29 | 2.85 | 0.86 | 1.89 | 8.86 | 133.78 | 38.54 | 292.12 | 0.6668 | 650.6 | 559.6 | |
| 0.00 | 0.52 | 0.00 | 0.34 | 8.66 | 133.26 | 38.01 | 292.13 | 0.6596 | 437.0 | 344.8 | |
| 3.80 | -8.00 | 2.48 | -8.00 | 8.00 | 133.07 | 37.82 | 291.29 | 0.6540 | 553.5 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.79 | 8.52 | 133.05 | 37.80 | 292.05 | 0.6564 | 598.0 | 493.6 | |
| 15.97 | -8.00 | 10.36 | -8.00 | 8.14 | 132.55 | 37.31 | 291.79 | 0.6484 | 866.4 | 999999 | |
| 2.07 | -8.00 | 1.34 | -8.00 | 8.34 | 132.27 | 37.02 | 292.22 | 0.6459 | 763.2 | 999999 | |
| 0.00 | 1.99 | 0.00 | 1.28 | 7.64 | 132.04 | 36.80 | 291.35 | 0.6397 | 274.0 | 424.1 | |
| 0.00 | 1.47 | 0.00 | 0.94 | 7.68 | 131.71 | 36.47 | 291.59 | 0.6358 | 491.0 | 530.9 | |
| 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. | |