SDO HMI 2014-11-23 05:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.64 | 0.00 | 10.94 | -12.61 | 225.99 | 22.97 | 236.81 | 0.4562 | -71.2 | 50.1 | |
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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 | 1.20 | 0.00 | 0.69 | -13.32 | 228.90 | 25.88 | 238.63 | 0.4995 | 687.0 | 589.6 | |
| 0.00 | 0.77 | 0.00 | 0.44 | -12.00 | 228.46 | 25.44 | 240.60 | 0.4842 | 789.0 | 645.4 | |
| 0.00 | 1.89 | 0.00 | 1.07 | -13.13 | 228.48 | 25.45 | 238.56 | 0.4926 | 715.0 | 601.5 | |
| 0.00 | 1.97 | 0.00 | 1.12 | -12.76 | 228.20 | 25.18 | 238.97 | 0.4862 | 824.0 | 745.3 | |
| 0.00 | 1.80 | 0.00 | 1.02 | -13.52 | 228.15 | 25.13 | 237.55 | 0.4913 | 773.0 | 606.9 | |
| 0.00 | 1.46 | 0.00 | 0.82 | -13.03 | 227.93 | 24.91 | 238.21 | 0.4847 | 699.0 | 677.8 | |
| 0.00 | 1.29 | 0.00 | 0.73 | -12.81 | 227.87 | 24.85 | 238.55 | 0.4823 | 788.0 | 653.7 | |
| 0.00 | 1.20 | 0.00 | 0.66 | -12.97 | 223.63 | 20.61 | 233.46 | 0.4288 | -735.0 | -528.4 | |
| 0.00 | 0.94 | 0.00 | 0.51 | -11.47 | 223.42 | 20.39 | 236.18 | 0.4129 | -714.0 | -570.0 | |
| 0.00 | 1.20 | 0.00 | 0.65 | -10.86 | 223.34 | 20.32 | 237.35 | 0.4068 | -650.0 | -535.8 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -12.53 | 223.43 | 20.41 | 234.05 | 0.4224 | -884.0 | -720.2 | |
| 0.00 | 1.29 | 0.00 | 0.70 | -11.86 | 223.35 | 20.33 | 235.28 | 0.4154 | -980.0 | -821.5 | |
| 0.00 | 1.20 | 0.00 | 0.66 | -12.93 | 223.43 | 20.41 | 233.27 | 0.4260 | -684.0 | -601.9 | |
| 0.00 | 1.46 | 0.00 | 0.79 | -11.40 | 223.22 | 20.20 | 236.05 | 0.4097 | -961.0 | -765.2 | |
| 0.00 | 0.94 | 0.00 | 0.52 | -13.42 | 222.93 | 19.90 | 231.66 | 0.4240 | -735.0 | -586.5 | |
| 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. | |