SDO HMI 2014-03-31 23:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 77.61 | 253.55 | 96.27 | 318.39 | -11.46 | 17.08 | -67.41 | 99.67 | 0.9184 | -194.1 | -56.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.70 | 0.00 | 0.70 | -11.09 | 23.60 | -60.89 | 99.04 | 0.8702 | 392.0 | 362.9 | |
| 0.00 | 1.75 | 0.00 | 1.76 | -9.98 | 23.47 | -61.02 | 97.77 | 0.8715 | 513.0 | 491.4 | |
| 3.86 | 7.98 | 3.87 | 7.99 | -9.50 | 23.56 | -60.93 | 97.22 | 0.8709 | 659.2 | 474.3 | |
| 0.00 | 0.88 | 0.00 | 0.88 | -10.12 | 23.36 | -61.13 | 97.94 | 0.8724 | 435.0 | 517.9 | |
| 0.00 | 0.61 | 0.00 | 0.62 | -10.57 | 23.01 | -61.47 | 98.47 | 0.8752 | 414.0 | 457.7 | |
| 0.00 | 1.05 | 0.00 | 1.07 | -10.09 | 23.05 | -61.44 | 97.91 | 0.8750 | 403.0 | 430.8 | |
| 7.81 | 11.93 | 8.04 | 12.29 | -10.84 | 22.60 | -61.89 | 98.78 | 0.8786 | 571.4 | 341.6 | |
| 0.61 | 6.84 | 0.63 | 7.09 | -10.23 | 22.61 | -61.87 | 98.09 | 0.8786 | 391.4 | 374.3 | |
| 0.00 | 0.70 | 0.00 | 0.73 | -10.44 | 22.34 | -62.15 | 98.34 | 0.8807 | 459.0 | 432.8 | |
| 0.00 | 2.02 | 0.00 | 2.12 | -10.56 | 21.97 | -62.52 | 98.49 | 0.8837 | 341.0 | 213.3 | |
| 1.23 | 7.02 | 1.30 | 7.43 | -10.56 | 21.70 | -62.79 | 98.50 | 0.8859 | 357.5 | -135.2 | |
| 0.00 | 0.44 | 0.00 | 0.46 | -10.39 | 21.77 | -62.72 | 98.30 | 0.8854 | 133.0 | 185.8 | |
| 3.24 | 25.17 | 3.49 | 27.56 | -10.97 | 21.21 | -63.28 | 98.98 | 0.8897 | 523.8 | -17.8 | |
| 8.77 | -13.00 | 9.59 | -13.00 | -11.05 | 20.76 | -63.73 | 99.08 | 0.8931 | 384.9 | 999999 | |
| 0.53 | 2.19 | 0.57 | 2.38 | -10.42 | 20.94 | -63.55 | 98.37 | 0.8919 | -66.8 | -31.5 | |
| 0.61 | 1.67 | 0.68 | 1.84 | -10.26 | 20.51 | -63.98 | 98.21 | 0.8953 | 169.3 | 176.2 | |
| 1.40 | 4.74 | 1.58 | 5.33 | -11.41 | 19.90 | -64.59 | 99.52 | 0.8996 | 468.0 | 369.7 | |
| 0.79 | -17.00 | 0.89 | -17.00 | -11.30 | 19.95 | -64.54 | 99.39 | 0.8992 | 232.8 | 999999 | |
| 0.88 | 2.46 | 0.98 | 2.75 | -10.09 | 20.08 | -64.41 | 98.04 | 0.8986 | 255.5 | 118.2 | |
| 0.00 | 1.14 | 0.00 | 1.32 | -11.12 | 19.08 | -65.41 | 99.22 | 0.9057 | -342.0 | -311.1 | |
| 3.16 | 22.45 | 3.80 | 27.11 | -11.40 | 18.04 | -66.45 | 99.58 | 0.9130 | -329.9 | -275.9 | |
| 1.67 | -21.00 | 2.04 | -21.00 | -11.42 | 17.57 | -66.92 | 99.61 | 0.9163 | 531.2 | 999999 | |
| 0.00 | 0.53 | 0.00 | 0.64 | -10.67 | 17.75 | -66.73 | 98.79 | 0.9152 | -237.0 | -251.5 | |
| 0.70 | 2.02 | 0.88 | 2.53 | -12.09 | 16.99 | -67.50 | 100.37 | 0.9201 | 110.4 | 218.4 | |
| 0.00 | 6.14 | 0.00 | 7.61 | -10.87 | 17.27 | -67.22 | 99.02 | 0.9185 | -620.0 | -404.5 | |
| 0.00 | 3.95 | 0.00 | 4.89 | -10.41 | 17.32 | -67.17 | 98.53 | 0.9183 | -290.0 | -299.9 | |
| 0.00 | 0.96 | 0.00 | 1.23 | -12.24 | 16.41 | -68.08 | 100.55 | 0.9238 | -216.0 | -187.1 | |
| 0.00 | 1.14 | 0.00 | 1.48 | -11.26 | 16.10 | -68.39 | 99.51 | 0.9262 | -445.0 | -458.4 | |
| 0.00 | 0.61 | 0.00 | 0.76 | -7.51 | 17.47 | -67.02 | 95.36 | 0.9184 | -397.0 | -318.4 | |
| 0.00 | 1.58 | 0.00 | 2.08 | -11.47 | 15.73 | -68.75 | 99.75 | 0.9284 | -485.0 | -434.3 | |
| 1.14 | 133.57 | 1.52 | 183.95 | -11.65 | 15.46 | -69.03 | 99.96 | 0.9301 | -658.5 | -71.2 | |
| 31.48 | -31.00 | 43.13 | -31.00 | -12.11 | 14.85 | -69.64 | 100.47 | 0.9337 | -665.6 | 999999 | |
| 0.00 | 0.61 | 0.00 | 0.82 | -10.74 | 15.51 | -68.98 | 98.97 | 0.9301 | -471.0 | -458.0 | |
| 9.73 | -31.00 | 13.28 | -31.00 | -11.29 | 14.96 | -69.53 | 99.59 | 0.9333 | -513.4 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.97 | -10.54 | 14.74 | -69.75 | 98.80 | 0.9349 | 188.0 | 102.1 | |
| 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. | |