| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 105.90 | 499.08 | 82.46 | 387.49 | -13.88 | 120.93 | -47.27 | 112.03 | 0.7710 | 374.9 | 170.8 | |
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back to the solar disc SDO HMI 2011-11-03 12:58:59 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.30 | 1.99 | 0.93 | 1.43 | -18.70 | 127.10 | -41.10 | 120.81 | 0.7274 | 643.8 | 606.8 | |
| 10.11 | 290.18 | 7.45 | 215.70 | -14.83 | 123.98 | -44.22 | 114.38 | 0.7425 | 1072.8 | 277.3 | |
| 0.61 | -2.00 | 0.45 | -2.00 | -15.73 | 123.61 | -44.59 | 115.34 | 0.7501 | 567.0 | 999999 | |
| 33.02 | -2.00 | 24.60 | -2.00 | -15.23 | 123.49 | -44.72 | 114.66 | 0.7494 | 746.6 | 999999 | |
| 11.67 | -2.00 | 8.68 | -2.00 | -14.52 | 123.33 | -44.88 | 113.70 | 0.7483 | 703.8 | 999999 | |
| 1.04 | -2.00 | 0.78 | -2.00 | -15.20 | 122.97 | -45.23 | 114.39 | 0.7546 | 104.2 | 999999 | |
| 0.00 | 1.64 | 0.00 | 1.25 | -14.59 | 122.03 | -46.17 | 113.24 | 0.7621 | 516.0 | 464.6 | |
| 0.00 | 0.43 | 0.00 | 0.33 | -14.85 | 121.82 | -46.38 | 113.48 | 0.7652 | 272.0 | 279.0 | |
| 0.00 | 2.42 | 0.00 | 1.85 | -14.08 | 121.63 | -46.57 | 112.44 | 0.7644 | 657.0 | 390.0 | |
| 2.59 | 3.28 | 1.99 | 2.53 | -13.82 | 121.25 | -46.95 | 111.97 | 0.7675 | 485.2 | 481.8 | |
| 0.00 | 4.93 | 0.00 | 3.92 | -13.39 | 119.44 | -48.76 | 110.77 | 0.7847 | -583.0 | -622.6 | |
| 5.79 | 7.17 | 4.72 | 5.85 | -14.68 | 118.64 | -49.56 | 112.06 | 0.7966 | -757.2 | -613.8 | |
| 0.00 | 0.61 | 0.00 | 0.50 | -15.04 | 118.39 | -49.82 | 112.40 | 0.8002 | -623.0 | -514.3 | |
| 1.30 | 1.47 | 1.09 | 1.23 | -14.82 | 117.44 | -50.76 | 111.79 | 0.8086 | -700.1 | -648.0 | |
| 2.51 | 14.87 | 2.12 | 12.60 | -15.15 | 117.14 | -51.07 | 112.08 | 0.8125 | -788.7 | -592.0 | |
| 10.29 | 127.93 | 8.28 | 103.73 | -11.02 | 118.21 | -49.99 | 107.46 | 0.7904 | 907.0 | 211.4 | |
| 0.00 | 3.54 | 0.00 | 2.98 | -14.58 | 117.17 | -51.03 | 111.42 | 0.8105 | -746.0 | -633.7 | |
| 0.00 | 0.95 | 0.00 | 0.80 | -14.30 | 117.12 | -51.09 | 111.07 | 0.8102 | -487.0 | -398.3 | |
| 4.15 | -15.00 | 3.53 | -15.00 | -15.17 | 116.78 | -51.42 | 111.98 | 0.8159 | -373.6 | 999999 | |
| 2.77 | 3.98 | 2.32 | 3.33 | -13.74 | 117.09 | -51.11 | 110.40 | 0.8089 | -506.7 | -552.9 | |
| 0.69 | 17.37 | 0.60 | 15.00 | -15.59 | 116.48 | -51.72 | 112.38 | 0.8199 | 169.1 | -304.0 | |
| 0.00 | 0.78 | 0.00 | 0.66 | -14.42 | 116.73 | -51.47 | 111.08 | 0.8142 | -497.0 | -397.9 | |
| 13.74 | -16.00 | 11.20 | -16.00 | -10.99 | 117.65 | -50.55 | 107.25 | 0.7960 | 537.5 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.89 | -14.59 | 116.43 | -51.77 | 111.19 | 0.8176 | -476.0 | -359.4 | |
| 1.64 | 2.33 | 1.41 | 2.01 | -14.46 | 116.12 | -52.08 | 110.93 | 0.8200 | -318.7 | -123.0 | |
| 0.00 | 1.47 | 0.00 | 1.27 | -14.68 | 116.05 | -52.15 | 111.16 | 0.8214 | -394.0 | -277.9 | |
| 0.52 | -25.00 | 0.45 | -25.00 | -14.53 | 116.00 | -52.20 | 110.97 | 0.8214 | 56.7 | 999999 | |
| 0.00 | 1.21 | 0.00 | 1.12 | -18.36 | 114.22 | -53.98 | 114.79 | 0.8477 | -479.0 | -475.9 | |
| 0.00 | 1.38 | 0.00 | 1.28 | -18.13 | 114.22 | -53.99 | 114.54 | 0.8471 | -547.0 | -498.5 | |
| 0.00 | 0.86 | 0.00 | 0.74 | -12.81 | 116.14 | -52.06 | 108.98 | 0.8155 | -403.0 | -357.8 | |
| 0.52 | 4.49 | 0.44 | 3.86 | -10.13 | 115.20 | -53.00 | 105.52 | 0.8182 | 699.7 | 574.8 | |
| 1.64 | -31.00 | 1.42 | -31.00 | -10.29 | 115.01 | -53.19 | 105.66 | 0.8204 | 473.9 | 999999 | |
| 0.00 | 1.64 | 0.00 | 1.45 | -9.06 | 113.65 | -54.55 | 103.87 | 0.8308 | 403.0 | 316.3 | |
| 0.00 | 1.12 | 0.00 | 1.18 | -15.78 | 108.87 | -59.33 | 110.34 | 0.8847 | -323.0 | -273.9 | |
| 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. | |