SDO HMI 2014-04-18 14:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.44 | 213.82 | 35.65 | 122.80 | -12.22 | 182.05 | -29.82 | 105.12 | 0.5058 | 400.1 | 51.1 | |
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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 | 0.58 | -13.91 | 188.52 | -23.35 | 112.15 | 0.4171 | 737.0 | 600.0 | |
| 0.00 | 1.33 | 0.00 | 0.73 | -13.69 | 187.56 | -24.31 | 110.99 | 0.4302 | 666.0 | 524.3 | |
| 7.71 | 17.36 | 4.27 | 9.62 | -8.84 | 185.24 | -26.63 | 99.10 | 0.4504 | 959.9 | 729.5 | |
| 0.00 | 2.13 | 0.00 | 1.18 | -8.05 | 184.55 | -27.32 | 97.25 | 0.4600 | 543.0 | 463.6 | |
| 0.00 | 1.06 | 0.00 | 0.60 | -11.14 | 183.96 | -27.91 | 103.69 | 0.4747 | 593.0 | 488.9 | |
| 0.00 | 2.83 | 0.00 | 1.59 | -8.37 | 184.08 | -27.79 | 97.85 | 0.4676 | -548.0 | -400.5 | |
| 0.00 | 0.71 | 0.00 | 0.40 | -10.86 | 183.71 | -28.16 | 103.02 | 0.4777 | 663.0 | 487.2 | |
| 3.19 | 40.30 | 1.81 | 22.83 | -12.33 | 183.37 | -28.50 | 105.91 | 0.4867 | 831.0 | 489.6 | |
| 20.11 | -8.00 | 11.38 | -8.00 | -12.06 | 183.37 | -28.50 | 105.36 | 0.4859 | 1019.6 | 999999 | |
| 3.72 | 6.02 | 2.10 | 3.40 | -8.75 | 183.18 | -28.69 | 98.50 | 0.4817 | -971.5 | -676.2 | |
| 0.00 | 1.68 | 0.00 | 0.96 | -12.17 | 182.51 | -29.36 | 105.26 | 0.4988 | 729.0 | 652.1 | |
| 18.51 | 84.59 | 10.70 | 48.96 | -13.34 | 181.50 | -30.37 | 107.15 | 0.5169 | 1198.0 | 283.6 | |
| 0.53 | 3.99 | 0.31 | 2.29 | -11.46 | 181.60 | -30.27 | 103.57 | 0.5102 | 492.2 | 35.5 | |
| 0.00 | 1.33 | 0.00 | 0.76 | -10.13 | 181.72 | -30.16 | 101.00 | 0.5058 | -886.0 | -771.5 | |
| 0.00 | 1.77 | 0.00 | 1.03 | -12.22 | 181.04 | -30.83 | 104.86 | 0.5203 | -986.0 | -799.8 | |
| 0.00 | 1.24 | 0.00 | 0.72 | -11.49 | 181.02 | -30.85 | 103.46 | 0.5187 | -821.0 | -701.9 | |
| 2.83 | 11.96 | 1.65 | 6.96 | -12.33 | 180.67 | -31.20 | 104.93 | 0.5259 | -1073.5 | -691.0 | |
| 0.00 | 3.90 | 0.00 | 2.26 | -11.54 | 180.73 | -31.14 | 103.47 | 0.5230 | -787.0 | -747.5 | |
| 0.00 | 3.54 | 0.00 | 2.07 | -12.71 | 180.29 | -31.58 | 105.51 | 0.5323 | -892.0 | -711.1 | |
| 0.00 | 0.53 | 0.00 | 0.31 | -12.52 | 180.31 | -31.56 | 105.18 | 0.5315 | -879.0 | -761.3 | |
| 1.06 | 5.58 | 0.62 | 3.26 | -12.01 | 180.28 | -31.59 | 104.20 | 0.5307 | -913.3 | -750.5 | |
| 0.35 | 1.77 | 0.21 | 1.04 | -12.42 | 180.15 | -31.72 | 104.95 | 0.5336 | -941.2 | -723.9 | |
| 4.43 | 15.77 | 2.60 | 9.26 | -12.69 | 179.93 | -31.94 | 105.36 | 0.5374 | -964.7 | -731.2 | |
| 0.00 | 1.06 | 0.00 | 0.62 | -11.95 | 179.74 | -32.13 | 103.94 | 0.5382 | -601.0 | -413.5 | |
| 0.00 | 0.80 | 0.00 | 0.46 | -8.51 | 179.99 | -31.88 | 97.55 | 0.5290 | 584.0 | 486.9 | |
| 0.00 | 1.51 | 0.00 | 0.91 | -16.81 | 177.76 | -34.11 | 111.76 | 0.5802 | 708.0 | 548.2 | |
| 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. | |