SDO HMI 2014-11-04 02:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.12 | 43.04 | 4.34 | 23.32 | 5.62 | 71.42 | -23.73 | 85.24 | 0.4031 | 22.6 | -286.2 | |
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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 |
| 1.73 | 26.80 | 0.92 | 14.27 | 5.86 | 73.70 | -21.45 | 84.39 | 0.3671 | -1274.1 | -772.9 | |
| 3.37 | -1.00 | 1.80 | -1.00 | 5.91 | 73.51 | -21.64 | 84.27 | 0.3703 | -955.0 | 999999 | |
| 2.59 | -1.00 | 1.38 | -1.00 | 5.64 | 73.49 | -21.66 | 85.00 | 0.3704 | -1043.5 | 999999 | |
| 0.00 | 2.59 | 0.00 | 1.38 | 5.20 | 73.41 | -21.74 | 86.23 | 0.3713 | -641.0 | -681.4 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 3.46 | 71.91 | -23.24 | 90.76 | 0.3956 | -747.0 | -588.4 | |
| 0.00 | 1.21 | 0.00 | 0.66 | 5.36 | 70.60 | -24.54 | 86.05 | 0.4163 | -858.0 | -612.9 | |
| 0.00 | 1.12 | 0.00 | 0.63 | 6.05 | 67.68 | -27.47 | 84.76 | 0.4626 | 812.0 | 595.6 | |
| 0.00 | 1.30 | 0.00 | 0.73 | 6.06 | 67.34 | -27.81 | 84.75 | 0.4679 | 844.0 | 665.2 | |
| 0.00 | 1.47 | 0.00 | 0.82 | 5.73 | 67.12 | -28.03 | 85.49 | 0.4710 | 882.0 | 585.5 | |
| 0.43 | 1.64 | 0.24 | 0.92 | 5.75 | 66.95 | -28.20 | 85.45 | 0.4737 | 862.8 | 730.4 | |
| 0.00 | 1.12 | 0.00 | 0.63 | 4.61 | 66.42 | -28.73 | 87.88 | 0.4814 | 923.0 | 738.5 | |
| 0.00 | 2.16 | 0.00 | 1.22 | 4.48 | 66.22 | -28.92 | 88.14 | 0.4844 | 824.0 | 708.7 | |
| 0.00 | 1.21 | 0.00 | 0.69 | 5.17 | 65.58 | -29.57 | 86.73 | 0.4943 | 831.0 | 558.2 | |
| 0.00 | 1.56 | 0.00 | 0.90 | 6.23 | 64.34 | -30.81 | 84.69 | 0.5134 | 738.0 | 553.3 | |
| 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. | |