SDO HMI 2014-04-14 11:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.55 | 88.67 | 15.45 | 48.07 | -9.56 | 242.60 | -23.73 | 100.87 | 0.4060 | 371.0 | 242.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.86 | 0.00 | 0.97 | -11.20 | 248.75 | -17.59 | 108.83 | 0.3146 | 933.0 | 712.0 | |
| 0.00 | 1.24 | 0.00 | 0.66 | -9.83 | 245.79 | -20.55 | 102.87 | 0.3562 | 669.0 | 424.7 | |
| 0.00 | 1.86 | 0.00 | 0.99 | -9.29 | 244.85 | -21.49 | 100.97 | 0.3699 | 984.0 | 679.6 | |
| 0.00 | 1.50 | 0.00 | 0.81 | -9.92 | 244.01 | -22.32 | 102.30 | 0.3846 | 742.0 | 605.3 | |
| 0.00 | 1.15 | 0.00 | 0.62 | -10.08 | 243.41 | -22.93 | 102.46 | 0.3945 | 678.0 | 516.2 | |
| 0.00 | 2.12 | 0.00 | 1.15 | -9.49 | 242.99 | -23.35 | 100.83 | 0.3997 | -501.0 | -627.5 | |
| 16.00 | 24.05 | 8.64 | 12.99 | -8.37 | 242.86 | -23.47 | 98.00 | 0.3996 | 983.3 | 715.5 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -9.21 | 242.81 | -23.53 | 100.08 | 0.4020 | -769.0 | -642.6 | |
| 1.06 | 43.67 | 0.57 | 23.72 | -10.05 | 242.71 | -23.63 | 102.12 | 0.4053 | -892.9 | 10.4 | |
| 10.61 | -9.00 | 5.76 | -9.00 | -9.82 | 242.36 | -23.98 | 101.44 | 0.4103 | -963.8 | 999999 | |
| 0.00 | 2.56 | 0.00 | 1.39 | -8.56 | 242.45 | -23.88 | 98.38 | 0.4064 | 659.0 | 463.3 | |
| 0.88 | -9.00 | 0.48 | -9.00 | -9.99 | 242.01 | -24.32 | 101.73 | 0.4161 | 982.0 | 999999 | |
| 0.00 | 3.18 | 0.00 | 1.75 | -10.65 | 241.05 | -25.29 | 102.91 | 0.4326 | 850.0 | 625.1 | |
| 0.00 | 1.15 | 0.00 | 0.63 | -11.48 | 240.70 | -25.64 | 104.66 | 0.4402 | 690.0 | 583.6 | |
| 0.00 | 1.68 | 0.00 | 0.93 | -12.69 | 240.02 | -26.32 | 107.03 | 0.4542 | 735.0 | 577.4 | |
| 0.00 | 0.97 | 0.00 | 0.54 | -12.62 | 239.72 | -26.62 | 106.73 | 0.4585 | 665.0 | 568.5 | |
| 0.00 | 0.80 | 0.00 | 0.44 | -9.48 | 239.28 | -27.06 | 99.78 | 0.4572 | 703.0 | 563.7 | |
| 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. | |