SDO HMI 2014-03-06 14:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.33 | 138.37 | 32.60 | 132.02 | -10.01 | 359.60 | -59.43 | 97.35 | 0.8568 | 532.4 | 243.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.64 | 0.00 | 1.49 | -9.38 | 1.60 | -57.43 | 96.50 | 0.8390 | -339.0 | -261.9 | |
| 18.85 | 113.47 | 17.79 | 106.74 | -10.32 | 0.00 | -59.03 | 97.70 | 0.8533 | 729.2 | 296.6 | |
| 11.59 | -2.00 | 10.88 | -2.00 | -9.56 | 0.23 | -58.80 | 96.79 | 0.8516 | 716.0 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.82 | -8.06 | 359.97 | -59.06 | 95.05 | 0.8546 | -268.0 | -310.1 | |
| 0.00 | 0.86 | 0.00 | 0.83 | -9.75 | 359.40 | -59.63 | 97.05 | 0.8589 | 382.0 | 279.8 | |
| 0.00 | 0.95 | 0.00 | 0.92 | -9.89 | 359.05 | -59.97 | 97.23 | 0.8618 | 384.0 | 311.9 | |
| 0.78 | 1.82 | 0.78 | 1.83 | -10.96 | 357.83 | -61.20 | 98.53 | 0.8719 | 399.4 | 284.2 | |
| 0.00 | 1.04 | 0.00 | 1.05 | -10.11 | 357.74 | -61.29 | 97.55 | 0.8730 | 299.0 | 327.5 | |
| 0.00 | 0.61 | 0.00 | 0.62 | -10.26 | 357.50 | -61.53 | 97.74 | 0.8750 | 263.0 | 195.9 | |
| 3.11 | 9.77 | 3.15 | 9.89 | -9.07 | 357.62 | -61.41 | 96.37 | 0.8744 | 430.7 | 269.2 | |
| 0.00 | 3.20 | 0.00 | 3.35 | -10.21 | 356.54 | -62.49 | 97.74 | 0.8828 | -462.0 | -429.4 | |
| 0.00 | 1.47 | 0.00 | 1.53 | -9.40 | 356.81 | -62.22 | 96.80 | 0.8810 | 135.0 | 101.1 | |
| 0.00 | 1.56 | 0.00 | 1.66 | -11.17 | 355.85 | -63.18 | 98.85 | 0.8880 | 293.0 | 220.3 | |
| 0.00 | 1.12 | 0.00 | 1.29 | -14.42 | 353.66 | -65.37 | 102.56 | 0.9038 | -436.0 | -388.3 | |
| 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. | |