SDO HMI 2011-05-07 00:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 95.51 | 386.61 | 52.22 | 211.87 | 16.65 | 48.67 | 14.82 | 324.87 | 0.4264 | -258.0 | -117.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.15 | 0.00 | 1.23 | 18.67 | 54.03 | 20.18 | 318.95 | 0.4996 | 911.0 | 761.1 | |
| 0.00 | 1.16 | 0.00 | 0.65 | 16.81 | 52.03 | 18.19 | 319.16 | 0.4588 | 580.0 | 411.4 | |
| 4.20 | 243.00 | 2.32 | 134.10 | 16.31 | 51.29 | 17.44 | 319.58 | 0.4455 | -943.9 | -375.7 | |
| 32.91 | -3.00 | 18.13 | -3.00 | 16.26 | 50.69 | 16.84 | 320.48 | 0.4390 | -1153.3 | 999999 | |
| 14.40 | -3.00 | 7.95 | -3.00 | 16.68 | 50.70 | 16.85 | 321.10 | 0.4440 | -823.9 | 999999 | |
| 8.32 | -3.00 | 4.56 | -3.00 | 16.22 | 50.03 | 16.18 | 321.52 | 0.4319 | -982.8 | 999999 | |
| 0.00 | 1.88 | 0.00 | 1.04 | 17.19 | 50.02 | 16.17 | 322.96 | 0.4435 | -504.0 | -439.0 | |
| 0.00 | 1.43 | 0.00 | 0.79 | 16.70 | 49.74 | 15.90 | 322.72 | 0.4349 | -585.0 | -378.9 | |
| 0.00 | 2.68 | 0.00 | 1.47 | 16.21 | 49.54 | 15.69 | 322.36 | 0.4270 | -912.0 | -700.4 | |
| 3.04 | 3.40 | 1.65 | 1.85 | 15.50 | 49.19 | 15.34 | 321.89 | 0.4148 | -949.8 | -895.0 | |
| 1.07 | 4.38 | 0.59 | 2.40 | 16.49 | 49.07 | 15.22 | 323.59 | 0.4260 | -741.7 | -537.5 | |
| 0.00 | 1.70 | 0.00 | 0.92 | 15.01 | 48.76 | 14.91 | 321.91 | 0.4047 | -839.0 | -689.3 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 17.72 | 48.78 | 14.93 | 325.82 | 0.4388 | 666.0 | 488.2 | |
| 0.00 | 0.80 | 0.00 | 0.46 | 22.24 | 48.69 | 14.84 | 331.35 | 0.4964 | 687.0 | 563.2 | |
| 0.36 | 1.52 | 0.20 | 0.84 | 19.08 | 48.14 | 14.29 | 328.70 | 0.4509 | -666.5 | -515.0 | |
| 0.00 | 1.25 | 0.00 | 0.69 | 19.14 | 47.98 | 14.13 | 329.05 | 0.4504 | -564.0 | -451.1 | |
| 3.49 | 4.65 | 1.93 | 2.57 | 18.94 | 47.86 | 14.02 | 329.02 | 0.4469 | -868.4 | -644.6 | |
| 0.00 | 2.59 | 0.00 | 1.44 | 19.33 | 47.83 | 13.98 | 329.55 | 0.4518 | -803.0 | -618.2 | |
| 0.00 | 1.88 | 0.00 | 1.04 | 19.03 | 47.64 | 13.79 | 329.53 | 0.4464 | -813.0 | -700.0 | |
| 0.00 | 0.63 | 0.00 | 0.35 | 19.56 | 47.59 | 13.74 | 330.25 | 0.4529 | -638.0 | -550.6 | |
| 0.00 | 0.36 | 0.00 | 0.20 | 18.93 | 47.34 | 13.49 | 329.96 | 0.4426 | -511.0 | -566.8 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 16.20 | 46.97 | 13.12 | 327.12 | 0.4032 | -762.0 | -600.5 | |
| 0.00 | 1.43 | 0.00 | 0.77 | 15.85 | 45.11 | 11.26 | 330.49 | 0.3830 | 859.0 | 665.9 | |
| 0.00 | 2.50 | 0.00 | 1.36 | 17.89 | 45.01 | 11.16 | 333.23 | 0.4107 | 752.0 | 560.9 | |
| 0.00 | 1.43 | 0.00 | 0.77 | 17.20 | 44.87 | 11.02 | 332.72 | 0.4001 | 430.0 | 386.9 | |
| 1.34 | 87.92 | 0.72 | 47.25 | 16.26 | 44.33 | 10.48 | 332.72 | 0.3828 | 888.3 | 542.1 | |
| 21.73 | -26.00 | 11.68 | -26.00 | 16.87 | 44.14 | 10.29 | 333.88 | 0.3901 | 1044.5 | 999999 | |
| 0.00 | 6.71 | 0.00 | 3.63 | 17.94 | 44.20 | 10.36 | 334.97 | 0.4059 | 687.0 | 609.8 | |
| 3.49 | -26.00 | 1.87 | -26.00 | 16.39 | 43.92 | 10.08 | 333.79 | 0.3816 | 1185.5 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.68 | 18.40 | 44.04 | 10.19 | 335.81 | 0.4113 | 691.0 | 490.4 | |
| 1.16 | -26.00 | 0.62 | -26.00 | 16.77 | 43.81 | 9.97 | 334.49 | 0.3864 | 802.3 | 999999 | |
| 0.00 | 0.54 | 0.00 | 0.29 | 17.16 | 43.51 | 9.67 | 335.59 | 0.3899 | 766.0 | 580.5 | |
| 0.00 | 2.50 | 0.00 | 1.35 | 17.41 | 42.95 | 9.10 | 337.12 | 0.3900 | 950.0 | 728.4 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 18.32 | 42.67 | 8.83 | 338.64 | 0.4017 | 698.0 | 503.8 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 19.06 | 42.23 | 8.38 | 340.30 | 0.4103 | 740.0 | 597.0 | |
| 0.00 | 2.86 | 0.00 | 1.55 | 19.29 | 41.69 | 7.84 | 341.66 | 0.4109 | 652.0 | 581.9 | |
| 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. | |