SDO HMI 2010-11-16 07:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 152.47 | 709.46 | 94.14 | 438.59 | 13.70 | 172.38 | 35.27 | 289.84 | 0.5976 | -90.7 | -3.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.95 | 0.00 | 0.61 | 11.44 | 176.18 | 39.07 | 284.72 | 0.6410 | -1.0 | -42.8 | |
| 0.34 | 347.39 | 0.22 | 223.81 | 12.02 | 176.00 | 38.89 | 285.66 | 0.6401 | -808.2 | -273.6 | |
| 1.12 | -2.00 | 0.72 | -2.00 | 12.03 | 175.85 | 38.74 | 285.71 | 0.6381 | -960.3 | 999999 | |
| 69.19 | -2.00 | 44.57 | -2.00 | 12.84 | 175.95 | 38.84 | 286.93 | 0.6415 | -1149.8 | 999999 | |
| 5.24 | -2.00 | 3.33 | -2.00 | 12.71 | 175.07 | 37.97 | 287.00 | 0.6298 | -1107.0 | 999999 | |
| 0.00 | 1.38 | 0.00 | 0.87 | 12.11 | 174.93 | 37.82 | 286.11 | 0.6264 | -805.0 | -706.1 | |
| 2.66 | 6.27 | 1.68 | 3.96 | 12.69 | 174.61 | 37.50 | 287.13 | 0.6237 | -917.5 | -640.1 | |
| 0.00 | 1.55 | 0.00 | 0.97 | 10.85 | 173.97 | 36.86 | 284.37 | 0.6105 | -737.0 | -584.6 | |
| 0.00 | 0.77 | 0.00 | 0.49 | 13.10 | 174.29 | 37.19 | 287.86 | 0.6208 | -723.0 | -642.8 | |
| 0.00 | 1.98 | 0.00 | 1.24 | 12.59 | 174.17 | 37.06 | 287.10 | 0.6177 | -917.0 | -759.1 | |
| 0.00 | 7.39 | 0.00 | 4.62 | 12.23 | 173.84 | 36.73 | 286.64 | 0.6124 | -740.0 | -736.1 | |
| 0.00 | 4.04 | 0.00 | 2.53 | 12.74 | 173.89 | 36.78 | 287.44 | 0.6145 | -666.0 | -731.7 | |
| 0.00 | 1.80 | 0.00 | 1.13 | 13.17 | 173.92 | 36.82 | 288.10 | 0.6162 | -949.0 | -709.5 | |
| 0.00 | 3.09 | 0.00 | 1.93 | 12.42 | 173.65 | 36.54 | 287.01 | 0.6103 | -844.0 | -689.4 | |
| 0.00 | 1.72 | 0.00 | 1.07 | 12.73 | 173.21 | 36.10 | 287.66 | 0.6054 | -609.0 | -501.5 | |
| 0.00 | 1.12 | 0.00 | 0.69 | 12.16 | 173.11 | 36.01 | 286.77 | 0.6025 | -672.0 | -610.2 | |
| 0.69 | 2.75 | 0.42 | 1.70 | 13.36 | 172.48 | 35.38 | 288.94 | 0.5978 | 457.2 | 78.6 | |
| 0.00 | 0.60 | 0.00 | 0.37 | 13.49 | 171.83 | 34.73 | 289.43 | 0.5896 | 621.0 | 472.0 | |
| 0.00 | 1.12 | 0.00 | 0.67 | 13.83 | 170.49 | 33.38 | 290.58 | 0.5729 | 666.0 | 434.6 | |
| 0.00 | 0.34 | 0.00 | 0.21 | 15.69 | 170.37 | 33.26 | 293.73 | 0.5790 | 455.0 | 466.2 | |
| 1.89 | 5.07 | 1.13 | 3.04 | 13.57 | 169.90 | 32.79 | 290.41 | 0.5639 | -725.7 | -249.2 | |
| 0.00 | 0.60 | 0.00 | 0.36 | 15.69 | 170.19 | 33.08 | 293.84 | 0.5767 | 579.0 | 511.3 | |
| 0.00 | 1.63 | 0.00 | 0.98 | 14.09 | 169.76 | 32.66 | 291.36 | 0.5642 | 643.0 | 492.3 | |
| 0.00 | 1.03 | 0.00 | 0.62 | 13.76 | 169.64 | 32.53 | 290.86 | 0.5611 | 601.0 | 394.0 | |
| 0.00 | 1.72 | 0.00 | 1.04 | 15.85 | 169.92 | 32.81 | 294.24 | 0.5739 | 790.0 | 614.6 | |
| 0.00 | 0.34 | 0.00 | 0.21 | 14.25 | 169.61 | 32.50 | 291.70 | 0.5627 | 439.0 | 500.8 | |
| 0.00 | 1.98 | 0.00 | 1.19 | 16.01 | 169.84 | 32.73 | 294.54 | 0.5736 | 617.0 | 454.1 | |
| 9.11 | 303.30 | 5.43 | 178.64 | 14.29 | 169.29 | 32.18 | 291.93 | 0.5586 | 926.0 | 406.2 | |
| 1.46 | 3.52 | 0.87 | 2.10 | 14.62 | 169.30 | 32.20 | 292.49 | 0.5602 | 685.1 | 375.7 | |
| 0.00 | 1.20 | 0.00 | 0.72 | 16.20 | 169.58 | 32.47 | 295.00 | 0.5711 | 576.0 | 425.9 | |
| 0.00 | 2.66 | 0.00 | 1.57 | 13.34 | 168.39 | 31.28 | 290.73 | 0.5423 | -579.0 | -502.0 | |
| 0.00 | 0.86 | 0.00 | 0.50 | 13.44 | 168.12 | 31.01 | 291.04 | 0.5390 | 592.0 | 480.4 | |
| 60.08 | -28.00 | 35.37 | -28.00 | 15.02 | 167.86 | 30.75 | 293.98 | 0.5426 | 1171.1 | 999999 | |
| 0.69 | -28.00 | 0.40 | -28.00 | 14.55 | 167.11 | 30.00 | 293.60 | 0.5302 | 810.2 | 999999 | |
| 0.00 | 1.29 | 0.00 | 0.75 | 14.34 | 166.79 | 29.69 | 293.41 | 0.5250 | 824.0 | 693.3 | |
| 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. | |