| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.64 | 55.62 | 9.25 | 30.63 | 8.28 | 133.87 | -20.57 | 52.84 | 0.4355 | 421.4 | 160.3 | |
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back to the solar disc SDO HMI 2014-02-27 08:09:27 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.38 | 0.00 | 0.72 | 6.62 | 141.49 | -12.96 | 43.41 | 0.3256 | -890.0 | -803.1 | |
| 0.00 | 2.24 | 0.00 | 1.18 | 6.62 | 141.24 | -13.21 | 43.94 | 0.3285 | -805.0 | -645.5 | |
| 0.00 | 1.64 | 0.00 | 0.86 | 6.26 | 141.06 | -13.38 | 45.10 | 0.3262 | -865.0 | -752.9 | |
| 0.00 | 1.29 | 0.00 | 0.68 | 6.06 | 139.65 | -14.79 | 48.43 | 0.3408 | -856.0 | -729.7 | |
| 0.00 | 6.30 | 0.00 | 3.33 | 6.89 | 139.60 | -14.85 | 46.77 | 0.3507 | -324.0 | -668.0 | |
| 0.00 | 0.78 | 0.00 | 0.42 | 7.98 | 134.50 | -19.95 | 53.03 | 0.4247 | 585.0 | 484.4 | |
| 0.00 | 1.21 | 0.00 | 0.66 | 7.27 | 133.28 | -21.16 | 56.02 | 0.4337 | 723.0 | 609.9 | |
| 11.12 | 14.66 | 6.17 | 8.13 | 8.77 | 132.88 | -21.56 | 53.76 | 0.4523 | 1009.1 | 654.9 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 9.40 | 132.00 | -22.45 | 53.76 | 0.4691 | 529.0 | 449.8 | |
| 0.86 | 6.90 | 0.48 | 3.86 | 8.79 | 131.74 | -22.70 | 55.13 | 0.4668 | 922.7 | 634.0 | |
| 4.66 | 7.93 | 2.60 | 4.44 | 8.49 | 131.63 | -22.81 | 55.80 | 0.4656 | 984.3 | 645.9 | |
| 0.00 | 1.64 | 0.00 | 0.92 | 9.42 | 131.50 | -22.94 | 54.31 | 0.4754 | 482.0 | 374.4 | |
| 0.00 | 1.55 | 0.00 | 0.88 | 9.74 | 131.38 | -23.06 | 53.92 | 0.4797 | 603.0 | 485.1 | |
| 0.00 | 1.12 | 0.00 | 0.63 | 8.90 | 131.41 | -23.04 | 55.33 | 0.4720 | 384.0 | 353.8 | |
| 0.00 | 0.60 | 0.00 | 0.34 | 11.28 | 131.10 | -23.35 | 51.72 | 0.4972 | -566.0 | -538.3 | |
| 0.00 | 3.97 | 0.00 | 2.22 | 8.30 | 131.09 | -23.36 | 56.77 | 0.4709 | 610.0 | 711.2 | |
| 0.00 | 1.38 | 0.00 | 0.78 | 9.07 | 130.08 | -24.36 | 56.57 | 0.4901 | 458.0 | 333.7 | |
| 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. | |