SDO HMI 2014-12-01 06:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.91 | 236.18 | 54.56 | 284.33 | 3.28 | 162.68 | 65.64 | 273.23 | 0.9121 | -308.4 | -140.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.62 | 203.61 | 18.39 | 251.79 | 2.49 | 163.83 | 66.79 | 272.34 | 0.9207 | -526.4 | -176.9 | |
| 23.34 | -1.00 | 28.51 | -1.00 | 3.36 | 163.11 | 66.07 | 273.29 | 0.9157 | -545.1 | 999999 | |
| 0.00 | 1.37 | 0.00 | 1.63 | 4.38 | 162.47 | 65.43 | 274.42 | 0.9113 | -276.0 | -250.1 | |
| 0.00 | 0.26 | 0.00 | 0.29 | 4.13 | 161.37 | 64.33 | 274.16 | 0.9032 | -296.0 | -337.0 | |
| 0.00 | 2.82 | 0.00 | 3.07 | 3.88 | 159.98 | 62.94 | 273.91 | 0.8925 | -646.0 | -546.1 | |
| 0.00 | 1.97 | 0.00 | 2.13 | 4.42 | 159.80 | 62.76 | 274.52 | 0.8911 | 144.0 | 83.2 | |
| 0.00 | 1.45 | 0.00 | 1.55 | 3.32 | 159.32 | 62.29 | 273.30 | 0.8872 | 42.0 | 98.5 | |
| 0.77 | 2.39 | 0.82 | 2.56 | 4.51 | 159.42 | 62.38 | 274.64 | 0.8881 | 433.8 | 314.2 | |
| 0.00 | 0.26 | 0.00 | 0.27 | 3.84 | 158.62 | 61.59 | 273.89 | 0.8816 | 351.0 | 269.0 | |
| 0.34 | 1.28 | 0.34 | 1.29 | 3.50 | 157.47 | 60.43 | 273.53 | 0.8718 | 428.0 | 364.2 | |
| 1.28 | 2.91 | 1.24 | 2.81 | 5.80 | 156.08 | 59.04 | 276.24 | 0.8603 | 487.6 | 312.2 | |
| 4.79 | 15.98 | 4.54 | 15.18 | 6.35 | 155.43 | 58.39 | 276.92 | 0.8547 | 720.0 | 364.4 | |
| 0.26 | -12.00 | 0.24 | -12.00 | 6.62 | 155.42 | 58.38 | 277.23 | 0.8548 | 558.3 | 999999 | |
| 0.51 | 1.88 | 0.48 | 1.76 | 4.13 | 154.98 | 57.94 | 274.32 | 0.8498 | 544.7 | 412.6 | |
| 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. | |