| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.40 | 0.00 | 14.33 | -15.08 | 127.77 | 21.29 | 242.53 | 0.3995 | 480.1 | 433.4 | |
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back to the solar disc SDO HMI 2014-03-30 07:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.32 | 0.00 | 0.78 | -6.82 | 140.51 | 34.03 | 267.64 | 0.5583 | 677.0 | 609.8 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -7.63 | 134.26 | 27.78 | 266.21 | 0.4649 | 734.0 | 516.6 | |
| 0.00 | 0.96 | 0.00 | 0.54 | -6.70 | 133.76 | 27.28 | 268.26 | 0.4573 | 573.0 | 494.4 | |
| 0.00 | 1.05 | 0.00 | 0.59 | -15.64 | 133.35 | 26.87 | 248.83 | 0.4686 | 622.0 | 478.4 | |
| 0.00 | 3.51 | 0.00 | 1.95 | -14.04 | 132.72 | 26.24 | 251.89 | 0.4532 | 975.0 | 687.3 | |
| 0.00 | 1.32 | 0.00 | 0.74 | -19.20 | 133.13 | 26.65 | 241.59 | 0.4836 | 761.0 | 680.3 | |
| 0.00 | 5.09 | 0.00 | 2.81 | -15.41 | 131.86 | 25.38 | 248.44 | 0.4462 | 744.0 | 642.2 | |
| 0.00 | 1.32 | 0.00 | 0.72 | -15.52 | 131.39 | 24.91 | 247.90 | 0.4399 | 912.0 | 746.5 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -15.58 | 130.82 | 24.34 | 247.39 | 0.4319 | 968.0 | 787.5 | |
| 0.00 | 1.49 | 0.00 | 0.79 | -12.99 | 126.87 | 20.39 | 250.88 | 0.3609 | 773.0 | 588.0 | |
| 0.00 | 1.84 | 0.00 | 0.98 | -20.95 | 122.37 | 15.89 | 225.49 | 0.3602 | 841.0 | 601.8 | |
| 0.00 | 1.40 | 0.00 | 0.71 | -11.49 | 118.69 | 12.21 | 247.19 | 0.2259 | 721.0 | 494.1 | |
| 0.00 | 0.96 | 0.00 | 0.49 | -15.17 | 116.06 | 9.59 | 227.01 | 0.2207 | -904.0 | -741.5 | |
| 0.00 | 1.14 | 0.00 | 0.58 | -18.69 | 114.48 | 8.01 | 212.15 | 0.2490 | -867.0 | -752.2 | |
| 0.00 | 1.23 | 0.00 | 0.62 | -15.73 | 113.07 | 6.59 | 214.87 | 0.1943 | 917.0 | 552.6 | |
| 0.00 | 1.84 | 0.00 | 0.96 | -23.86 | 112.65 | 6.18 | 198.35 | 0.3139 | -766.0 | -656.0 | |
| 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. | |