| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.45 | 284.17 | 23.79 | 155.42 | -23.73 | 115.12 | 16.66 | 218.26 | 0.4262 | 460.9 | 343.4 | |
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back to the solar disc SDO HMI 2014-04-27 04:00:35 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.25 | 0.00 | 0.70 | -24.58 | 117.77 | 19.30 | 220.96 | 0.4605 | 633.0 | 540.1 | |
| 0.00 | 1.25 | 0.00 | 0.67 | -19.43 | 116.99 | 18.53 | 229.00 | 0.3987 | -720.0 | -551.5 | |
| 0.00 | 0.71 | 0.00 | 0.40 | -27.72 | 117.26 | 18.80 | 215.71 | 0.4908 | 567.0 | 483.8 | |
| 0.71 | 5.43 | 0.39 | 3.01 | -24.78 | 116.19 | 17.72 | 218.38 | 0.4470 | 777.8 | 539.0 | |
| 33.75 | 221.10 | 18.48 | 121.00 | -23.34 | 115.91 | 17.45 | 220.25 | 0.4279 | 1306.3 | 473.7 | |
| 0.00 | 1.16 | 0.00 | 0.64 | -24.50 | 115.87 | 17.40 | 218.34 | 0.4406 | 582.0 | 483.5 | |
| 0.00 | 5.43 | 0.00 | 2.99 | -24.18 | 115.72 | 17.25 | 218.60 | 0.4355 | 727.0 | 635.7 | |
| 4.36 | -5.00 | 2.38 | -5.00 | -23.48 | 115.38 | 16.92 | 219.20 | 0.4241 | 1023.7 | 999999 | |
| 1.34 | -5.00 | 0.73 | -5.00 | -23.86 | 115.43 | 16.97 | 218.66 | 0.4291 | 736.1 | 999999 | |
| 0.00 | 1.42 | 0.00 | 0.78 | -24.47 | 115.41 | 16.95 | 217.67 | 0.4360 | 721.0 | 633.1 | |
| 0.00 | 0.89 | 0.00 | 0.49 | -25.80 | 115.50 | 17.03 | 215.83 | 0.4524 | -504.0 | -421.0 | |
| 0.00 | 3.12 | 0.00 | 1.73 | -25.54 | 115.35 | 16.89 | 215.98 | 0.4480 | -327.0 | -620.7 | |
| 0.00 | 1.07 | 0.00 | 0.59 | -25.35 | 115.26 | 16.79 | 216.11 | 0.4448 | -659.0 | -520.8 | |
| 2.58 | 4.19 | 1.42 | 2.30 | -24.61 | 115.12 | 16.66 | 217.00 | 0.4348 | 880.7 | 695.7 | |
| 0.71 | 4.90 | 0.39 | 2.68 | -24.59 | 114.56 | 16.10 | 216.15 | 0.4293 | 874.1 | 661.7 | |
| 0.00 | 0.98 | 0.00 | 0.53 | -23.76 | 114.42 | 15.96 | 217.20 | 0.4180 | 733.0 | 595.3 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -24.47 | 114.10 | 15.64 | 215.56 | 0.4235 | 617.0 | 472.8 | |
| 0.00 | 3.56 | 0.00 | 1.96 | -25.70 | 114.08 | 15.62 | 213.75 | 0.4386 | -783.0 | -698.0 | |
| 0.00 | 0.71 | 0.00 | 0.39 | -26.44 | 114.15 | 15.69 | 212.83 | 0.4484 | 734.0 | 675.9 | |
| 0.00 | 2.23 | 0.00 | 1.22 | -25.38 | 113.90 | 15.44 | 213.91 | 0.4330 | -948.0 | -799.0 | |
| 0.00 | 1.25 | 0.00 | 0.69 | -26.67 | 113.97 | 15.51 | 212.24 | 0.4498 | 841.0 | 701.6 | |
| 0.00 | 2.32 | 0.00 | 1.22 | -20.03 | 112.04 | 13.58 | 219.38 | 0.3492 | -779.0 | -631.9 | |
| 0.00 | 0.89 | 0.00 | 0.47 | -20.89 | 111.69 | 13.23 | 217.07 | 0.3562 | -832.0 | -701.0 | |
| 0.00 | 1.25 | 0.00 | 0.68 | -26.54 | 112.18 | 13.71 | 209.41 | 0.4337 | 527.0 | 538.5 | |
| 0.00 | 0.71 | 0.00 | 0.39 | -26.94 | 112.05 | 13.59 | 208.70 | 0.4380 | 633.0 | 527.4 | |
| 0.00 | 1.34 | 0.00 | 0.72 | -24.18 | 110.45 | 11.99 | 209.33 | 0.3884 | -681.0 | -574.6 | |
| 0.00 | 1.25 | 0.00 | 0.68 | -26.32 | 109.70 | 11.24 | 205.16 | 0.4127 | -834.0 | -621.9 | |
| 0.00 | 2.40 | 0.00 | 1.28 | -23.76 | 108.09 | 9.63 | 204.91 | 0.3652 | -716.0 | -611.9 | |
| 0.00 | 1.25 | 0.00 | 0.69 | -29.26 | 108.43 | 9.96 | 199.82 | 0.4471 | -615.0 | -358.9 | |
| 0.00 | 2.94 | 0.00 | 1.56 | -23.42 | 107.44 | 8.97 | 203.84 | 0.3557 | -737.0 | -571.4 | |
| 0.00 | 1.51 | 0.00 | 0.83 | -28.12 | 107.17 | 8.71 | 198.45 | 0.4238 | -709.0 | -515.5 | |
| 0.00 | 1.16 | 0.00 | 0.64 | -30.50 | 105.08 | 6.62 | 192.78 | 0.4507 | -708.0 | -525.8 | |
| 0.00 | 2.76 | 0.00 | 1.48 | -26.90 | 103.63 | 5.17 | 191.94 | 0.3903 | -691.0 | -578.9 | |
| 0.00 | 1.25 | 0.00 | 0.67 | -26.58 | 103.08 | 4.62 | 190.87 | 0.3835 | -726.0 | -575.1 | |
| 0.00 | 1.51 | 0.00 | 0.80 | -25.58 | 101.46 | 3.00 | 187.50 | 0.3633 | -756.0 | -526.4 | |
| 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. | |