SDO HMI 2014-04-01 01:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.41 | 293.28 | 83.73 | 349.45 | -11.38 | 17.30 | -66.09 | 99.53 | 0.9092 | -112.9 | -50.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 1.09 | -9.92 | 23.97 | -59.41 | 97.65 | 0.8577 | 679.0 | 616.9 | |
| 0.00 | 0.97 | 0.00 | 0.93 | -10.22 | 23.88 | -59.50 | 98.00 | 0.8584 | 664.0 | 580.1 | |
| 0.00 | 1.32 | 0.00 | 1.28 | -10.60 | 23.40 | -59.99 | 98.45 | 0.8626 | 543.0 | 534.8 | |
| 0.00 | 6.14 | 0.00 | 5.96 | -10.12 | 23.49 | -59.90 | 97.89 | 0.8619 | 442.0 | 474.7 | |
| 2.28 | 6.58 | 2.21 | 6.36 | -9.46 | 23.62 | -59.76 | 97.13 | 0.8609 | 656.8 | 544.6 | |
| 0.00 | 1.23 | 0.00 | 1.20 | -10.63 | 23.14 | -60.25 | 98.50 | 0.8648 | 614.0 | 546.1 | |
| 0.00 | 1.40 | 0.00 | 1.37 | -9.80 | 23.34 | -60.05 | 97.53 | 0.8632 | 425.0 | 373.1 | |
| 0.00 | 2.11 | 0.00 | 2.06 | -10.02 | 23.15 | -60.24 | 97.80 | 0.8648 | 489.0 | 391.3 | |
| 7.72 | 13.69 | 7.65 | 13.59 | -10.84 | 22.76 | -60.63 | 98.75 | 0.8680 | 647.8 | 258.0 | |
| 0.00 | 7.28 | 0.00 | 7.27 | -10.21 | 22.53 | -60.86 | 98.03 | 0.8701 | 474.0 | 370.2 | |
| 0.88 | 33.42 | 0.88 | 34.59 | -10.53 | 22.16 | -61.22 | 98.42 | 0.8731 | 450.3 | 176.8 | |
| 1.93 | -11.00 | 1.97 | -11.00 | -10.71 | 21.78 | -61.60 | 98.63 | 0.8762 | -343.8 | 999999 | |
| 2.19 | -11.00 | 2.24 | -11.00 | -10.56 | 21.77 | -61.62 | 98.46 | 0.8764 | 361.5 | 999999 | |
| 3.51 | -11.00 | 3.63 | -11.00 | -10.94 | 21.37 | -62.01 | 98.91 | 0.8796 | 526.8 | 999999 | |
| 0.00 | 1.32 | 0.00 | 1.36 | -10.37 | 21.45 | -61.94 | 98.26 | 0.8791 | 11.0 | -25.1 | |
| 0.70 | 3.25 | 0.73 | 3.39 | -10.39 | 21.04 | -62.34 | 98.29 | 0.8824 | 213.0 | -135.5 | |
| 6.84 | -11.00 | 7.21 | -11.00 | -11.03 | 20.74 | -62.65 | 99.03 | 0.8846 | 386.1 | 999999 | |
| 0.79 | 1.93 | 0.84 | 2.04 | -10.29 | 20.61 | -62.77 | 98.19 | 0.8858 | 307.4 | 235.2 | |
| 2.46 | 8.77 | 2.65 | 9.49 | -11.29 | 20.03 | -63.36 | 99.35 | 0.8902 | 476.2 | 274.9 | |
| 1.23 | 2.54 | 1.31 | 2.72 | -10.53 | 20.32 | -63.06 | 98.48 | 0.8881 | 87.6 | -27.3 | |
| 0.00 | 1.58 | 0.00 | 1.70 | -10.73 | 20.18 | -63.21 | 98.71 | 0.8892 | -539.0 | -409.7 | |
| 0.61 | 2.28 | 0.66 | 2.46 | -10.15 | 20.12 | -63.26 | 98.05 | 0.8898 | 250.3 | 123.6 | |
| 0.00 | 3.77 | 0.00 | 4.13 | -10.97 | 19.53 | -63.85 | 99.00 | 0.8941 | -151.0 | -100.3 | |
| 5.18 | 22.81 | 5.98 | 26.34 | -11.46 | 18.03 | -65.36 | 99.59 | 0.9052 | -156.3 | -172.8 | |
| 0.00 | 1.05 | 0.00 | 1.21 | -10.56 | 18.26 | -65.12 | 98.60 | 0.9038 | -296.0 | -275.4 | |
| 0.79 | 1.93 | 0.95 | 2.31 | -12.05 | 16.99 | -66.39 | 100.29 | 0.9125 | 296.9 | 171.9 | |
| 0.00 | 18.51 | 0.00 | 22.05 | -10.73 | 17.22 | -66.16 | 98.83 | 0.9112 | -509.0 | -312.7 | |
| 0.00 | 1.14 | 0.00 | 1.42 | -11.25 | 16.04 | -67.34 | 99.45 | 0.9192 | -536.0 | -507.5 | |
| 0.00 | 1.14 | 0.00 | 1.44 | -11.58 | 15.72 | -67.67 | 99.82 | 0.9213 | -821.0 | -647.8 | |
| 0.00 | 0.88 | 0.00 | 1.04 | -7.35 | 17.40 | -65.99 | 95.10 | 0.9113 | -357.0 | -335.6 | |
| 2.28 | 142.91 | 2.92 | 187.80 | -12.24 | 15.29 | -68.10 | 100.55 | 0.9240 | -1038.4 | -125.4 | |
| 1.84 | -31.00 | 2.34 | -31.00 | -11.71 | 15.49 | -67.90 | 99.97 | 0.9228 | -739.8 | 999999 | |
| 14.74 | -31.00 | 19.25 | -31.00 | -11.95 | 14.86 | -68.53 | 100.26 | 0.9268 | -622.8 | 999999 | |
| 7.54 | -31.00 | 10.02 | -31.00 | -12.30 | 14.41 | -68.98 | 100.65 | 0.9296 | -303.8 | 999999 | |
| 7.90 | -31.00 | 10.29 | -31.00 | -11.32 | 14.94 | -68.44 | 99.57 | 0.9265 | -530.0 | 999999 | |
| 0.00 | 2.19 | 0.00 | 2.85 | -10.54 | 15.08 | -68.31 | 98.72 | 0.9258 | -190.0 | -86.4 | |
| 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. | |