SDO HMI 2014-03-10 19:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.91 | 72.08 | 13.33 | 37.07 | 6.57 | 10.72 | 7.15 | 332.79 | 0.2703 | 53.0 | 162.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.87 | 3.81 | 0.45 | 1.97 | 5.83 | 14.55 | 10.98 | 319.72 | 0.2944 | -1045.6 | -876.6 | |
| 0.00 | 1.04 | 0.00 | 0.54 | 6.06 | 14.04 | 10.47 | 321.58 | 0.2920 | -1037.0 | -783.2 | |
| 0.00 | 1.30 | 0.00 | 0.67 | 6.33 | 13.74 | 10.17 | 322.95 | 0.2926 | -927.0 | -845.0 | |
| 0.00 | 0.87 | 0.00 | 0.45 | 6.13 | 13.10 | 9.53 | 324.34 | 0.2836 | -853.0 | -747.2 | |
| 9.10 | 12.39 | 4.70 | 6.40 | 6.76 | 12.59 | 9.02 | 327.05 | 0.2876 | -1119.9 | -731.2 | |
| 0.00 | 2.86 | 0.00 | 1.48 | 6.97 | 12.35 | 8.78 | 328.14 | 0.2885 | -881.0 | -712.1 | |
| 0.00 | 1.91 | 0.00 | 0.98 | 6.97 | 12.14 | 8.57 | 328.76 | 0.2866 | -1054.0 | -803.9 | |
| 0.00 | 1.56 | 0.00 | 0.81 | 7.21 | 11.90 | 8.33 | 329.90 | 0.2880 | -882.0 | -580.7 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 5.29 | 10.51 | 6.94 | 330.85 | 0.2483 | 1100.0 | 922.5 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 5.38 | 10.27 | 6.70 | 331.87 | 0.2477 | 1030.0 | 801.9 | |
| 0.00 | 1.56 | 0.00 | 0.80 | 6.69 | 10.29 | 6.72 | 334.13 | 0.2677 | 834.0 | 680.7 | |
| 2.08 | 3.81 | 1.07 | 1.96 | 7.31 | 10.09 | 6.52 | 335.76 | 0.2756 | -908.2 | -592.7 | |
| 0.00 | 2.95 | 0.00 | 1.51 | 5.83 | 9.80 | 6.23 | 334.40 | 0.2509 | 1113.0 | 927.8 | |
| 10.48 | 28.93 | 5.38 | 14.85 | 6.59 | 9.42 | 5.85 | 336.98 | 0.2600 | 1183.7 | 653.7 | |
| 2.95 | -14.00 | 1.51 | -14.00 | 6.87 | 9.36 | 5.79 | 337.59 | 0.2640 | 1014.5 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 6.40 | 9.02 | 5.45 | 338.11 | 0.2546 | 833.0 | 653.2 | |
| 0.00 | 3.03 | 0.00 | 1.55 | 6.22 | 8.75 | 5.18 | 338.85 | 0.2499 | 942.0 | 748.9 | |
| 0.43 | 2.25 | 0.22 | 1.15 | 6.55 | 8.69 | 5.12 | 339.53 | 0.2549 | 885.8 | 783.0 | |
| 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. | |