SDO HMI 2014-04-14 19:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.36 | 262.00 | 24.64 | 136.53 | 12.22 | 263.15 | 1.22 | 352.93 | 0.3114 | -998.6 | -397.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.06 | 0.00 | 0.55 | 11.90 | 265.83 | 3.90 | 347.55 | 0.3099 | 838.0 | 678.2 | |
| 7.51 | 252.27 | 3.91 | 131.26 | 12.33 | 263.80 | 1.87 | 354.09 | 0.3117 | -1284.4 | -430.1 | |
| 12.46 | -2.00 | 6.48 | -2.00 | 12.08 | 263.74 | 1.81 | 354.21 | 0.3074 | -1547.9 | 999999 | |
| 4.15 | -2.00 | 2.16 | -2.00 | 11.89 | 263.56 | 1.62 | 354.74 | 0.3040 | -1687.6 | 999999 | |
| 23.24 | -2.00 | 12.09 | -2.00 | 12.11 | 263.34 | 1.41 | 355.49 | 0.3073 | -1457.6 | 999999 | |
| 0.00 | 1.15 | 0.00 | 0.63 | 20.28 | 262.32 | 0.39 | 359.16 | 0.4392 | -729.0 | -572.7 | |
| 0.00 | 0.97 | 0.00 | 0.53 | 18.01 | 258.58 | -3.35 | 7.88 | 0.4068 | -478.0 | -443.9 | |
| 0.00 | 0.62 | 0.00 | 0.34 | 18.02 | 258.17 | -3.76 | 8.84 | 0.4078 | -585.0 | -514.9 | |
| 0.00 | 1.33 | 0.00 | 0.70 | 12.61 | 255.01 | -6.92 | 20.61 | 0.3354 | 812.0 | 567.7 | |
| 0.00 | 1.41 | 0.00 | 0.76 | 16.07 | 254.15 | -7.78 | 19.41 | 0.3932 | 794.0 | 571.3 | |
| 0.00 | 1.24 | 0.00 | 0.65 | 10.00 | 249.65 | -12.28 | 38.05 | 0.3413 | 790.0 | 578.1 | |
| 0.00 | 0.80 | 0.00 | 0.44 | 14.34 | 242.64 | -19.29 | 43.57 | 0.4664 | 623.0 | 524.8 | |
| 0.00 | 1.15 | 0.00 | 0.67 | 13.88 | 236.54 | -25.39 | 52.00 | 0.5302 | 661.0 | 543.5 | |
| 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. | |