| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.84 | 450.63 | 40.98 | 264.09 | -21.05 | 17.07 | 18.15 | 212.94 | 0.5366 | 935.5 | 369.8 | |
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back to the solar disc SDO HMI 2014-10-15 02:00:31 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.57 | 0.00 | 0.92 | -18.56 | 20.19 | 21.28 | 220.19 | 0.5353 | 642.0 | 498.5 | |
| 0.00 | 0.96 | 0.00 | 0.57 | -20.56 | 19.79 | 20.87 | 217.22 | 0.5537 | -726.0 | -602.6 | |
| 0.00 | 1.22 | 0.00 | 0.71 | -18.93 | 18.76 | 19.84 | 217.79 | 0.5260 | 845.0 | 713.2 | |
| 0.87 | 423.88 | 0.52 | 248.74 | -21.56 | 17.88 | 18.97 | 213.55 | 0.5491 | 650.6 | 395.2 | |
| 34.62 | -4.00 | 20.37 | -4.00 | -21.21 | 17.53 | 18.61 | 213.44 | 0.5421 | 1167.6 | 999999 | |
| 0.00 | 1.31 | 0.00 | 0.75 | -18.58 | 17.21 | 18.30 | 216.02 | 0.5081 | -352.0 | -327.1 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -18.57 | 16.94 | 18.03 | 215.63 | 0.5056 | -699.0 | -572.1 | |
| 33.04 | -4.00 | 19.34 | -4.00 | -20.95 | 16.92 | 18.01 | 212.86 | 0.5341 | 1383.0 | 999999 | |
| 0.00 | 1.49 | 0.00 | 0.86 | -21.72 | 14.76 | 15.85 | 208.88 | 0.5273 | 863.0 | 746.3 | |
| 0.00 | 1.22 | 0.00 | 0.71 | -21.31 | 14.62 | 15.70 | 209.07 | 0.5211 | 924.0 | 771.9 | |
| 0.00 | 1.14 | 0.00 | 0.66 | -21.88 | 14.38 | 15.46 | 208.14 | 0.5266 | 641.0 | 517.0 | |
| 0.00 | 1.49 | 0.00 | 0.87 | -22.79 | 14.04 | 15.13 | 206.79 | 0.5360 | -827.0 | -714.1 | |
| 1.31 | 6.29 | 0.75 | 3.62 | -21.05 | 13.59 | 14.68 | 207.72 | 0.5103 | 837.0 | 485.6 | |
| 0.00 | 1.14 | 0.00 | 0.66 | -21.81 | 13.20 | 14.29 | 206.38 | 0.5177 | -646.0 | -550.2 | |
| 0.00 | 1.66 | 0.00 | 0.95 | -21.20 | 13.14 | 14.23 | 206.86 | 0.5093 | -658.0 | -542.8 | |
| 0.00 | 5.07 | 0.00 | 2.83 | -18.60 | 11.19 | 12.28 | 206.05 | 0.4608 | -375.0 | -352.4 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -21.58 | 7.66 | 8.75 | 197.08 | 0.4835 | -630.0 | -557.6 | |
| 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. | |