| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.47 | 219.69 | 81.26 | 419.11 | -18.65 | 149.92 | 74.37 | 250.98 | 0.9639 | 49.3 | 7.5 | |
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back to the solar disc SDO HMI 2014-05-26 03:00:39 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.32 | 84.78 | 40.05 | 212.37 | -18.37 | 153.72 | 78.17 | 251.53 | 0.9803 | 231.5 | 4.5 | |
| 0.00 | 2.16 | 0.00 | 4.69 | -17.35 | 152.08 | 76.54 | 252.50 | 0.9743 | 348.0 | 333.1 | |
| 0.00 | 2.53 | 0.00 | 5.26 | -17.56 | 151.53 | 75.98 | 252.26 | 0.9723 | 489.0 | 399.0 | |
| 0.00 | 0.27 | 0.00 | 0.51 | -16.98 | 149.96 | 74.41 | 252.76 | 0.9657 | 308.0 | 335.3 | |
| 3.25 | 9.38 | 5.88 | 17.09 | -17.38 | 149.33 | 73.78 | 252.32 | 0.9630 | -178.2 | 263.6 | |
| 0.00 | 1.98 | 0.00 | 3.99 | -19.04 | 150.84 | 75.30 | 250.69 | 0.9699 | 270.0 | 281.0 | |
| 0.00 | 3.52 | 0.00 | 5.53 | -17.21 | 146.69 | 71.15 | 252.31 | 0.9502 | -25.0 | 15.5 | |
| 0.00 | 0.81 | 0.00 | 1.27 | -17.50 | 146.66 | 71.12 | 252.00 | 0.9502 | 36.0 | 139.6 | |
| 3.25 | 39.95 | 4.88 | 59.54 | -17.55 | 145.83 | 70.28 | 251.88 | 0.9458 | -296.4 | -214.0 | |
| 8.93 | -9.00 | 13.19 | -9.00 | -17.94 | 145.41 | 69.87 | 251.44 | 0.9437 | -389.6 | 999999 | |
| 0.81 | 5.32 | 1.26 | 8.21 | -19.85 | 146.29 | 70.74 | 249.50 | 0.9493 | -199.0 | -158.5 | |
| 1.26 | -11.00 | 1.94 | -11.00 | -19.99 | 145.94 | 70.39 | 249.33 | 0.9476 | -298.9 | 999999 | |
| 5.05 | 30.03 | 7.27 | 43.35 | -19.21 | 144.62 | 69.07 | 250.02 | 0.9400 | 607.9 | 404.2 | |
| 0.00 | 2.44 | 0.00 | 3.65 | -20.25 | 145.53 | 69.99 | 249.01 | 0.9456 | -409.0 | -378.3 | |
| 1.71 | 34.72 | 2.50 | 50.91 | -20.04 | 144.94 | 69.40 | 249.17 | 0.9423 | -509.2 | -243.1 | |
| 2.89 | -15.00 | 4.29 | -15.00 | -21.01 | 145.17 | 69.62 | 248.17 | 0.9441 | -202.8 | 999999 | |
| 0.00 | 1.80 | 0.00 | 2.74 | -21.52 | 145.53 | 69.98 | 247.67 | 0.9463 | 300.0 | 289.8 | |
| 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. | |