SDO HMI 2014-12-01 09:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.22 | 198.62 | 53.39 | 255.78 | 3.30 | 162.68 | 67.28 | 273.24 | 0.9233 | -274.0 | -120.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.59 | 166.15 | 18.36 | 220.77 | 2.52 | 163.93 | 68.53 | 272.37 | 0.9321 | -463.1 | -127.6 | |
| 21.11 | -1.00 | 27.56 | -1.00 | 3.36 | 163.08 | 67.68 | 273.28 | 0.9266 | -510.9 | 999999 | |
| 0.00 | 1.37 | 0.00 | 1.73 | 4.35 | 162.31 | 66.91 | 274.37 | 0.9216 | -430.0 | -333.6 | |
| 0.00 | 3.93 | 0.00 | 4.90 | 3.88 | 162.00 | 66.60 | 273.86 | 0.9194 | -707.0 | -609.4 | |
| 0.00 | 0.51 | 0.00 | 0.63 | 3.05 | 161.81 | 66.40 | 272.96 | 0.9180 | -562.0 | -573.2 | |
| 0.00 | 4.27 | 0.00 | 4.92 | 3.88 | 159.90 | 64.50 | 273.89 | 0.9044 | -616.0 | -546.3 | |
| 0.00 | 1.11 | 0.00 | 1.27 | 4.36 | 159.77 | 64.36 | 274.42 | 0.9035 | 10.0 | -7.8 | |
| 0.00 | 0.94 | 0.00 | 1.07 | 4.54 | 159.52 | 64.12 | 274.63 | 0.9017 | 328.0 | 287.9 | |
| 0.00 | 1.28 | 0.00 | 1.45 | 4.42 | 159.43 | 64.03 | 274.50 | 0.9010 | 259.0 | 235.6 | |
| 0.00 | 1.71 | 0.00 | 1.80 | 3.38 | 157.38 | 61.97 | 273.37 | 0.8847 | 498.0 | 403.0 | |
| 0.00 | 1.28 | 0.00 | 1.30 | 5.77 | 156.11 | 60.71 | 276.14 | 0.8747 | 419.0 | 359.9 | |
| 0.00 | 2.05 | 0.00 | 2.06 | 6.22 | 155.83 | 60.43 | 276.67 | 0.8725 | 328.0 | 248.4 | |
| 7.52 | 11.88 | 7.47 | 11.79 | 6.41 | 155.38 | 59.98 | 276.90 | 0.8688 | 621.9 | 395.6 | |
| 0.00 | 1.11 | 0.00 | 1.09 | 4.21 | 154.97 | 59.56 | 274.38 | 0.8644 | 484.0 | 357.4 | |
| 0.00 | 1.03 | 0.00 | 1.00 | 6.32 | 154.89 | 59.49 | 276.84 | 0.8645 | 9.0 | 17.6 | |
| 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. | |