SDO HMI 2011-05-06 08:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 86.22 | 427.72 | 45.74 | 227.27 | 16.48 | 48.54 | 5.87 | 344.18 | 0.3616 | -266.2 | -175.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.15 | 291.90 | 1.14 | 155.25 | 15.93 | 50.56 | 7.88 | 338.49 | 0.3611 | -1149.9 | -422.9 | |
| 2.86 | -1.00 | 1.52 | -1.00 | 15.83 | 50.30 | 7.62 | 339.02 | 0.3581 | -1287.7 | 999999 | |
| 29.78 | -1.00 | 15.83 | -1.00 | 16.25 | 50.25 | 7.58 | 339.57 | 0.3642 | -1211.5 | 999999 | |
| 8.14 | -1.00 | 4.34 | -1.00 | 16.73 | 50.24 | 7.56 | 340.07 | 0.3715 | -947.6 | 999999 | |
| 1.25 | -1.00 | 0.66 | -1.00 | 15.61 | 50.07 | 7.39 | 339.37 | 0.3533 | -1267.3 | 999999 | |
| 2.33 | -1.00 | 1.23 | -1.00 | 15.89 | 49.86 | 7.18 | 340.20 | 0.3565 | -1084.4 | 999999 | |
| 7.06 | -1.00 | 3.75 | -1.00 | 16.18 | 49.65 | 6.97 | 341.01 | 0.3598 | -1101.0 | 999999 | |
| 3.58 | -1.00 | 1.90 | -1.00 | 16.66 | 49.63 | 6.96 | 341.49 | 0.3672 | -651.5 | 999999 | |
| 0.00 | 1.79 | 0.00 | 0.94 | 15.15 | 49.36 | 6.68 | 340.76 | 0.3424 | -793.0 | -593.3 | |
| 1.52 | 4.74 | 0.80 | 2.50 | 15.54 | 49.31 | 6.63 | 341.27 | 0.3481 | -920.8 | -774.8 | |
| 4.65 | 5.54 | 2.45 | 2.93 | 15.66 | 48.55 | 5.88 | 343.37 | 0.3462 | -1061.9 | -902.2 | |
| 0.00 | 1.52 | 0.00 | 0.81 | 17.17 | 48.31 | 5.64 | 345.19 | 0.3689 | -519.0 | -353.6 | |
| 0.00 | 1.70 | 0.00 | 0.92 | 19.13 | 48.35 | 5.67 | 346.43 | 0.3996 | -865.0 | -711.2 | |
| 0.00 | 1.34 | 0.00 | 0.71 | 15.94 | 47.96 | 5.29 | 345.19 | 0.3481 | -528.0 | -491.7 | |
| 0.00 | 7.60 | 0.00 | 4.11 | 19.35 | 47.97 | 5.29 | 347.44 | 0.4018 | -837.0 | -841.9 | |
| 0.00 | 1.07 | 0.00 | 0.57 | 15.84 | 47.30 | 4.62 | 346.91 | 0.3438 | -791.0 | -583.6 | |
| 0.00 | 1.43 | 0.00 | 0.76 | 16.51 | 46.40 | 3.72 | 349.77 | 0.3516 | -845.0 | -666.9 | |
| 0.00 | 2.33 | 0.00 | 1.24 | 18.00 | 46.17 | 3.50 | 351.07 | 0.3750 | 804.0 | 508.4 | |
| 0.00 | 1.07 | 0.00 | 0.57 | 17.32 | 45.90 | 3.23 | 351.45 | 0.3633 | 564.0 | 386.2 | |
| 0.00 | 1.07 | 0.00 | 0.56 | 15.74 | 45.15 | 2.48 | 352.85 | 0.3359 | 912.0 | 788.1 | |
| 0.00 | 1.07 | 0.00 | 0.57 | 17.74 | 44.80 | 2.12 | 354.47 | 0.3679 | 816.0 | 727.2 | |
| 15.83 | 76.55 | 8.39 | 40.52 | 17.02 | 44.63 | 1.96 | 354.71 | 0.3560 | 1128.2 | 649.4 | |
| 0.00 | 4.56 | 0.00 | 2.42 | 17.32 | 44.35 | 1.68 | 355.54 | 0.3604 | 872.0 | 754.8 | |
| 2.33 | -22.00 | 1.23 | -22.00 | 16.35 | 44.31 | 1.63 | 355.42 | 0.3445 | 1034.4 | 999999 | |
| 0.00 | 3.85 | 0.00 | 2.04 | 17.57 | 44.26 | 1.58 | 355.84 | 0.3645 | 643.0 | 520.1 | |
| 4.74 | -22.00 | 2.50 | -22.00 | 16.57 | 44.15 | 1.48 | 355.91 | 0.3480 | 1194.2 | 999999 | |
| 0.00 | 5.28 | 0.00 | 2.79 | 17.06 | 44.03 | 1.36 | 356.34 | 0.3558 | 866.0 | 784.9 | |
| 0.00 | 1.07 | 0.00 | 0.56 | 16.02 | 43.99 | 1.32 | 356.24 | 0.3388 | 797.0 | 555.6 | |
| 0.00 | 1.61 | 0.00 | 0.86 | 17.77 | 43.88 | 1.20 | 356.87 | 0.3673 | 607.0 | 483.7 | |
| 0.00 | 0.72 | 0.00 | 0.38 | 16.83 | 43.87 | 1.20 | 356.73 | 0.3519 | 892.0 | 690.2 | |
| 0.00 | 2.95 | 0.00 | 1.56 | 16.44 | 43.87 | 1.19 | 356.67 | 0.3456 | 1177.0 | 991.8 | |
| 0.00 | 1.43 | 0.00 | 0.76 | 16.54 | 43.71 | 1.04 | 357.12 | 0.3470 | 869.0 | 747.1 | |
| 0.00 | 1.43 | 0.00 | 0.76 | 16.89 | 43.62 | 0.94 | 357.43 | 0.3528 | 780.0 | 688.5 | |
| 0.00 | 0.80 | 0.00 | 0.43 | 17.90 | 43.56 | 0.89 | 357.71 | 0.3691 | 550.0 | 427.6 | |
| 0.00 | 1.16 | 0.00 | 0.62 | 17.06 | 43.40 | 0.72 | 358.04 | 0.3553 | 762.0 | 611.2 | |
| 0.00 | 0.80 | 0.00 | 0.42 | 14.78 | 38.89 | -3.79 | 11.43 | 0.3239 | -844.0 | -682.3 | |
| 0.00 | 1.34 | 0.00 | 0.71 | 15.74 | 38.43 | -4.25 | 12.13 | 0.3409 | -746.0 | -523.9 | |
| 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. | |