SDO HMI 2011-01-05 05:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.99 | 414.89 | 45.02 | 255.70 | 31.37 | 188.24 | -11.15 | 16.14 | 0.5961 | -947.0 | -321.0 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.10 | 0.00 | 0.66 | 30.06 | 194.15 | -5.24 | 8.15 | 0.5601 | -743.0 | -585.7 | |
| 0.00 | 2.21 | 0.00 | 1.48 | 37.92 | 189.59 | -9.80 | 11.49 | 0.6765 | 637.0 | 581.4 | |
| 0.00 | 1.36 | 0.00 | 0.84 | 31.78 | 190.10 | -9.29 | 13.39 | 0.5949 | -434.0 | -275.2 | |
| 67.64 | 392.73 | 41.58 | 241.61 | 31.26 | 188.33 | -11.06 | 16.09 | 0.5943 | -1302.1 | -347.0 | |
| 1.02 | -4.00 | 0.63 | -4.00 | 30.97 | 187.87 | -11.52 | 16.87 | 0.5924 | -1059.9 | 999999 | |
| 0.00 | 3.57 | 0.00 | 2.32 | 35.21 | 187.18 | -12.21 | 15.48 | 0.6499 | 797.0 | 694.9 | |
| 0.00 | 0.85 | 0.00 | 0.55 | 34.54 | 186.73 | -12.66 | 16.37 | 0.6430 | -397.0 | -344.6 | |
| 0.00 | 1.10 | 0.00 | 0.67 | 30.28 | 186.80 | -12.59 | 18.75 | 0.5877 | -458.0 | -368.5 | |
| 0.00 | 1.36 | 0.00 | 0.81 | 28.38 | 187.01 | -12.39 | 19.72 | 0.5616 | -631.0 | -417.4 | |
| 0.00 | 0.93 | 0.00 | 0.57 | 30.24 | 186.70 | -12.69 | 18.91 | 0.5878 | -451.0 | -393.2 | |
| 0.00 | 1.53 | 0.00 | 0.92 | 28.80 | 186.58 | -12.82 | 20.05 | 0.5693 | -451.0 | -275.8 | |
| 0.00 | 0.68 | 0.00 | 0.42 | 31.76 | 186.03 | -13.36 | 18.85 | 0.6105 | -371.0 | -383.2 | |
| 4.33 | 6.20 | 2.81 | 4.02 | 34.42 | 184.95 | -14.45 | 18.57 | 0.6487 | 797.9 | 600.5 | |
| 0.00 | 0.34 | 0.00 | 0.22 | 33.13 | 182.68 | -16.71 | 22.06 | 0.6434 | 444.0 | 510.0 | |
| 0.00 | 0.93 | 0.00 | 0.61 | 33.86 | 181.20 | -18.20 | 23.24 | 0.6597 | 626.0 | 435.1 | |
| 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. | |