SDO HMI 2014-02-26 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 |
| 93.46 | 397.56 | 83.67 | 351.00 | -13.03 | 108.16 | -56.25 | 100.95 | 0.8248 | 257.6 | -52.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.21 | 0.00 | 0.69 | -12.63 | 133.72 | -30.70 | 102.70 | 0.5127 | 587.0 | 468.6 | |
| 0.00 | 1.29 | 0.00 | 0.79 | -12.96 | 128.48 | -35.93 | 102.25 | 0.5874 | 781.0 | 656.4 | |
| 0.00 | 0.69 | 0.00 | 0.43 | -17.03 | 127.16 | -37.25 | 108.68 | 0.6132 | 688.0 | 454.1 | |
| 0.00 | 1.29 | 0.00 | 0.80 | -11.42 | 127.52 | -36.89 | 99.52 | 0.5989 | 596.0 | 612.9 | |
| 0.00 | 2.15 | 0.00 | 1.33 | -11.40 | 127.26 | -37.15 | 99.46 | 0.6025 | 859.0 | 772.5 | |
| 0.00 | 1.12 | 0.00 | 0.69 | -8.90 | 127.37 | -37.04 | 95.30 | 0.5999 | 702.0 | 620.1 | |
| 0.00 | 1.29 | 0.00 | 0.80 | -11.42 | 127.03 | -37.39 | 99.46 | 0.6056 | 597.0 | 631.0 | |
| 2.50 | 9.30 | 1.55 | 5.78 | -11.03 | 127.05 | -37.36 | 98.82 | 0.6051 | 886.6 | 743.7 | |
| 0.00 | 0.86 | 0.00 | 0.54 | -11.62 | 126.96 | -37.46 | 99.80 | 0.6068 | 785.0 | 652.2 | |
| 0.00 | 1.29 | 0.00 | 0.80 | -12.06 | 126.85 | -37.57 | 100.51 | 0.6087 | 664.0 | 493.5 | |
| 0.00 | 1.29 | 0.00 | 0.81 | -12.49 | 126.54 | -37.87 | 101.17 | 0.6132 | 639.0 | 544.4 | |
| 0.60 | 2.15 | 0.38 | 1.34 | -11.06 | 126.74 | -37.68 | 98.86 | 0.6094 | 673.9 | 544.9 | |
| 0.00 | 1.38 | 0.00 | 0.85 | -6.98 | 127.24 | -37.17 | 92.10 | 0.6024 | 473.0 | 446.2 | |
| 0.00 | 1.21 | 0.00 | 0.75 | -7.53 | 126.96 | -37.45 | 93.02 | 0.6060 | 675.0 | 500.8 | |
| 0.00 | 0.34 | 0.00 | 0.22 | -15.38 | 125.42 | -39.00 | 105.63 | 0.6323 | 548.0 | 492.5 | |
| 0.00 | 1.03 | 0.00 | 0.67 | -16.08 | 124.69 | -39.72 | 106.57 | 0.6429 | 647.0 | 565.3 | |
| 0.00 | 1.12 | 0.00 | 0.72 | -14.80 | 124.99 | -39.42 | 104.64 | 0.6369 | 537.0 | 428.9 | |
| 0.00 | 2.84 | 0.00 | 1.85 | -14.58 | 124.04 | -40.38 | 104.12 | 0.6488 | 586.0 | 496.5 | |
| 0.00 | 0.43 | 0.00 | 0.29 | -11.33 | 122.14 | -42.28 | 98.99 | 0.6701 | 413.0 | 451.0 | |
| 0.00 | 0.78 | 0.00 | 0.52 | -10.43 | 121.43 | -42.98 | 97.63 | 0.6788 | 608.0 | 502.4 | |
| 0.00 | 0.60 | 0.00 | 0.41 | -10.80 | 121.20 | -43.21 | 98.17 | 0.6818 | 507.0 | 505.9 | |
| 0.00 | 0.95 | 0.00 | 0.78 | -17.60 | 111.19 | -53.22 | 106.68 | 0.7992 | -515.0 | -421.5 | |
| 0.00 | 0.52 | 0.00 | 0.43 | -19.14 | 110.28 | -54.13 | 108.51 | 0.8096 | -506.0 | -470.7 | |
| 0.00 | 0.52 | 0.00 | 0.41 | -13.39 | 112.08 | -52.33 | 101.43 | 0.7879 | -412.0 | -344.5 | |
| 0.00 | 1.12 | 0.00 | 0.90 | -12.79 | 112.11 | -52.30 | 100.66 | 0.7874 | -570.0 | -397.7 | |
| 0.00 | 1.38 | 0.00 | 1.14 | -11.63 | 110.42 | -54.00 | 99.18 | 0.8049 | 387.0 | 402.8 | |
| 0.00 | 0.95 | 0.00 | 0.79 | -11.29 | 110.09 | -54.32 | 98.77 | 0.8082 | 669.0 | 515.1 | |
| 0.00 | 0.78 | 0.00 | 0.67 | -13.42 | 108.45 | -55.96 | 101.39 | 0.8244 | -321.0 | -304.3 | |
| 0.00 | 1.29 | 0.00 | 1.12 | -12.55 | 108.48 | -55.93 | 100.33 | 0.8241 | -340.0 | -302.1 | |
| 1.64 | 355.70 | 1.45 | 323.04 | -13.44 | 107.78 | -56.63 | 101.41 | 0.8308 | -865.7 | -100.9 | |
| 25.41 | -30.00 | 22.76 | -30.00 | -13.70 | 107.29 | -57.12 | 101.71 | 0.8355 | -730.0 | 999999 | |
| 0.00 | 0.69 | 0.00 | 0.64 | -15.31 | 106.16 | -58.25 | 103.62 | 0.8460 | -430.0 | -434.1 | |
| 1.03 | -30.00 | 0.94 | -30.00 | -13.83 | 106.55 | -57.86 | 101.86 | 0.8423 | 250.7 | 999999 | |
| 3.79 | -30.00 | 3.48 | -30.00 | -14.20 | 106.34 | -58.07 | 102.31 | 0.8442 | -495.5 | 999999 | |
| 58.49 | -30.00 | 53.11 | -30.00 | -12.76 | 106.78 | -57.63 | 100.59 | 0.8402 | 682.0 | 999999 | |
| 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. | |