SDO HMI 2014-11-23 14:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.23 | 0.00 | 13.41 | -12.52 | 225.60 | 27.49 | 241.42 | 0.5147 | -212.6 | -38.5 | |
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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 | 3.51 | 0.00 | 2.08 | -12.69 | 228.28 | 30.17 | 243.29 | 0.5510 | 628.0 | 608.3 | |
| 0.00 | 1.29 | 0.00 | 0.76 | -12.84 | 228.23 | 30.12 | 243.01 | 0.5513 | 730.0 | 589.2 | |
| 0.00 | 1.80 | 0.00 | 1.07 | -13.08 | 228.05 | 29.94 | 242.47 | 0.5504 | 668.0 | 543.7 | |
| 0.00 | 2.91 | 0.00 | 1.72 | -12.81 | 227.91 | 29.80 | 242.83 | 0.5469 | 896.0 | 791.8 | |
| 0.00 | 0.69 | 0.00 | 0.40 | -12.81 | 226.58 | 28.48 | 241.81 | 0.5297 | 647.0 | 573.1 | |
| 0.00 | 2.06 | 0.00 | 1.17 | -11.82 | 223.92 | 25.81 | 241.32 | 0.4878 | -624.0 | -514.2 | |
| 0.00 | 1.29 | 0.00 | 0.73 | -12.68 | 223.94 | 25.83 | 239.79 | 0.4940 | -515.0 | -472.5 | |
| 0.00 | 1.29 | 0.00 | 0.73 | -11.76 | 223.71 | 25.60 | 241.25 | 0.4845 | -765.0 | -628.5 | |
| 0.00 | 2.91 | 0.00 | 1.64 | -11.51 | 223.55 | 25.45 | 241.57 | 0.4807 | -827.0 | -650.5 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -14.27 | 223.82 | 25.71 | 236.87 | 0.5042 | -649.0 | -543.3 | |
| 0.00 | 1.20 | 0.00 | 0.68 | -12.43 | 223.54 | 25.44 | 239.87 | 0.4870 | -802.0 | -675.1 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -12.00 | 223.46 | 25.36 | 240.59 | 0.4829 | -863.0 | -708.8 | |
| 0.00 | 1.37 | 0.00 | 0.78 | -12.64 | 223.23 | 25.12 | 239.19 | 0.4843 | -862.0 | -700.9 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -13.19 | 223.29 | 25.18 | 238.25 | 0.4892 | -638.0 | -433.5 | |
| 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. | |