| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.74 | 279.04 | 23.33 | 145.96 | 12.35 | 263.06 | -4.37 | 13.14 | 0.3209 | -914.2 | -410.3 | |
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back to the solar disc SDO HMI 2014-04-14 09:00:34 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.24 | 0.00 | 0.65 | 12.87 | 265.70 | -1.73 | 5.29 | 0.3206 | 759.0 | 573.5 | |
| 17.33 | 262.34 | 9.03 | 136.79 | 12.09 | 263.77 | -3.67 | 11.59 | 0.3125 | -1592.2 | -445.2 | |
| 5.31 | -2.00 | 2.77 | -2.00 | 12.37 | 263.76 | -3.67 | 11.42 | 0.3171 | -1256.5 | 999999 | |
| 22.10 | -2.00 | 11.53 | -2.00 | 12.09 | 263.37 | -4.07 | 12.82 | 0.3139 | -1401.5 | 999999 | |
| 0.00 | 1.24 | 0.00 | 0.68 | 18.71 | 262.64 | -4.80 | 10.87 | 0.4217 | -845.0 | -625.4 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 17.34 | 262.04 | -5.39 | 12.94 | 0.4023 | -753.0 | -551.2 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 11.46 | 260.94 | -6.49 | 20.66 | 0.3154 | -727.0 | -559.8 | |
| 0.00 | 1.24 | 0.00 | 0.68 | 18.24 | 258.66 | -8.77 | 19.71 | 0.4311 | -635.0 | -563.6 | |
| 0.00 | 2.21 | 0.00 | 1.21 | 18.08 | 258.35 | -9.08 | 20.49 | 0.4304 | -692.0 | -630.3 | |
| 0.00 | 1.41 | 0.00 | 0.78 | 18.07 | 255.62 | -11.82 | 25.92 | 0.4472 | -908.0 | -743.9 | |
| 0.00 | 2.03 | 0.00 | 1.12 | 17.14 | 254.94 | -12.50 | 28.22 | 0.4391 | 844.0 | 625.3 | |
| 0.00 | 1.24 | 0.00 | 0.68 | 16.06 | 253.95 | -13.49 | 31.38 | 0.4322 | 834.0 | 654.4 | |
| 0.00 | 0.97 | 0.00 | 0.55 | 16.12 | 249.62 | -17.82 | 38.73 | 0.4718 | 745.0 | 591.4 | |
| 0.00 | 0.35 | 0.00 | 0.20 | 12.15 | 246.18 | -21.25 | 49.80 | 0.4658 | 607.0 | 688.8 | |
| 0.00 | 1.68 | 0.00 | 0.94 | 11.69 | 245.19 | -22.24 | 51.86 | 0.4732 | 758.0 | 609.1 | |
| 0.00 | 1.06 | 0.00 | 0.60 | 11.13 | 243.54 | -23.90 | 54.78 | 0.4885 | 818.0 | 670.8 | |
| 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. | |