SDO HMI 2014-03-01 14:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.79 | 239.49 | 35.14 | 141.40 | 15.93 | 101.42 | -23.48 | 44.88 | 0.5439 | -39.2 | -13.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.59 | 0.00 | 1.48 | 15.01 | 104.99 | -19.90 | 41.56 | 0.4977 | -653.0 | -666.4 | |
| 0.00 | 1.55 | 0.00 | 0.89 | 14.80 | 104.59 | -20.31 | 42.42 | 0.4995 | -808.0 | -646.0 | |
| 10.27 | 62.81 | 5.91 | 36.21 | 15.00 | 103.74 | -21.15 | 43.30 | 0.5103 | -949.2 | -484.7 | |
| 15.53 | -3.00 | 8.97 | -3.00 | 15.37 | 103.51 | -21.39 | 43.12 | 0.5166 | -732.6 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.51 | 17.07 | 103.01 | -21.88 | 41.51 | 0.5397 | -699.0 | -495.4 | |
| 0.00 | 1.04 | 0.00 | 0.60 | 14.80 | 102.74 | -22.16 | 44.91 | 0.5185 | -274.0 | -237.7 | |
| 1.12 | 77.56 | 0.65 | 45.52 | 15.83 | 102.56 | -22.34 | 43.72 | 0.5312 | 677.7 | -262.2 | |
| 11.82 | -7.00 | 6.92 | -7.00 | 16.19 | 102.48 | -22.41 | 43.34 | 0.5357 | -998.7 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.70 | 15.43 | 102.27 | -22.63 | 44.64 | 0.5299 | -523.0 | -448.0 | |
| 0.86 | -7.00 | 0.51 | -7.00 | 15.92 | 102.15 | -22.75 | 44.13 | 0.5363 | 767.6 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.61 | 16.41 | 101.45 | -23.45 | 44.34 | 0.5484 | -258.0 | -172.5 | |
| 0.00 | 0.60 | 0.00 | 0.35 | 12.22 | 101.70 | -23.19 | 50.02 | 0.5043 | 430.0 | 515.7 | |
| 0.00 | 1.12 | 0.00 | 0.66 | 14.81 | 101.34 | -23.56 | 46.65 | 0.5335 | -414.0 | -272.6 | |
| 0.00 | 1.04 | 0.00 | 0.60 | 12.70 | 101.53 | -23.37 | 49.50 | 0.5110 | 691.0 | 541.2 | |
| 3.62 | 14.41 | 2.14 | 8.53 | 16.07 | 101.12 | -23.78 | 45.18 | 0.5484 | 906.1 | 252.5 | |
| 0.00 | 1.29 | 0.00 | 0.75 | 13.11 | 101.45 | -23.44 | 48.97 | 0.5158 | 743.0 | 589.1 | |
| 0.00 | 0.86 | 0.00 | 0.50 | 14.75 | 101.18 | -23.72 | 46.93 | 0.5347 | -480.0 | -345.1 | |
| 0.00 | 1.12 | 0.00 | 0.66 | 14.86 | 100.93 | -23.97 | 47.07 | 0.5384 | -327.0 | -244.2 | |
| 0.00 | 0.86 | 0.00 | 0.51 | 15.63 | 100.39 | -24.50 | 46.64 | 0.5515 | 900.0 | 664.4 | |
| 0.35 | 6.21 | 0.20 | 3.67 | 14.96 | 100.21 | -24.69 | 47.77 | 0.5472 | 719.8 | 763.8 | |
| 0.00 | 0.86 | 0.00 | 0.51 | 15.75 | 99.94 | -24.96 | 47.00 | 0.5575 | 676.0 | 563.6 | |
| 0.00 | 1.29 | 0.00 | 0.77 | 15.62 | 99.92 | -24.98 | 47.19 | 0.5565 | 896.0 | 595.7 | |
| 0.00 | 0.78 | 0.00 | 0.46 | 15.14 | 99.91 | -24.98 | 47.86 | 0.5520 | 682.0 | 576.3 | |
| 0.00 | 2.42 | 0.00 | 1.45 | 16.41 | 99.68 | -25.22 | 46.41 | 0.5666 | 848.0 | 717.5 | |
| 0.00 | 1.04 | 0.00 | 0.62 | 15.71 | 99.50 | -25.40 | 47.54 | 0.5618 | 759.0 | 622.8 | |
| 0.00 | 0.78 | 0.00 | 0.47 | 15.88 | 99.37 | -25.52 | 47.46 | 0.5647 | 683.0 | 637.3 | |
| 9.23 | 29.07 | 5.56 | 17.55 | 16.03 | 98.94 | -25.96 | 47.73 | 0.5707 | 878.6 | 410.0 | |
| 1.55 | -27.00 | 0.94 | -27.00 | 16.46 | 98.84 | -26.05 | 47.26 | 0.5757 | -219.4 | 999999 | |
| 2.16 | -27.00 | 1.31 | -27.00 | 16.19 | 98.43 | -26.46 | 48.06 | 0.5776 | 775.1 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.76 | 19.30 | 97.79 | -27.11 | 44.78 | 0.6128 | 249.0 | 315.6 | |
| 3.28 | 19.84 | 2.03 | 12.27 | 17.34 | 97.10 | -27.79 | 47.93 | 0.6018 | 816.4 | 691.7 | |
| 0.00 | 1.81 | 0.00 | 1.12 | 16.68 | 96.79 | -28.11 | 49.11 | 0.5993 | 742.0 | 633.1 | |
| 0.00 | 1.29 | 0.00 | 0.81 | 17.70 | 96.16 | -28.74 | 48.42 | 0.6146 | 639.0 | 516.4 | |
| 0.00 | 1.29 | 0.00 | 0.82 | 18.34 | 95.29 | -29.61 | 48.44 | 0.6290 | 537.0 | 443.7 | |
| 0.00 | 1.64 | 0.00 | 1.04 | 17.65 | 94.95 | -29.95 | 49.63 | 0.6267 | 707.0 | 548.4 | |
| 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. | |