SDO HMI 2014-11-24 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 | 14.65 | 0.00 | 10.12 | -13.12 | 227.04 | 42.11 | 249.12 | 0.7008 | 311.6 | 245.8 | |
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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 | 1.37 | 0.00 | 0.97 | -12.88 | 228.71 | 43.78 | 250.12 | 0.7196 | 340.0 | 323.4 | |
| 0.00 | 1.46 | 0.00 | 1.03 | -13.03 | 228.61 | 43.69 | 249.89 | 0.7190 | 523.0 | 390.7 | |
| 0.00 | 1.54 | 0.00 | 1.09 | -12.72 | 228.46 | 43.54 | 250.25 | 0.7163 | 636.0 | 479.3 | |
| 0.00 | 0.51 | 0.00 | 0.36 | -13.30 | 228.34 | 43.41 | 249.42 | 0.7167 | 455.0 | 426.7 | |
| 0.00 | 1.11 | 0.00 | 0.78 | -12.53 | 228.13 | 43.20 | 250.39 | 0.7118 | 549.0 | 479.2 | |
| 0.00 | 2.23 | 0.00 | 1.56 | -13.04 | 227.90 | 42.98 | 249.60 | 0.7109 | 784.0 | 682.2 | |
| 0.00 | 1.03 | 0.00 | 0.72 | -13.59 | 227.86 | 42.93 | 248.84 | 0.7123 | 600.0 | 561.1 | |
| 0.00 | 0.77 | 0.00 | 0.54 | -14.08 | 227.80 | 42.88 | 248.16 | 0.7134 | 417.0 | 365.1 | |
| 0.00 | 1.20 | 0.00 | 0.84 | -14.11 | 227.56 | 42.63 | 248.03 | 0.7107 | 546.0 | 466.5 | |
| 0.00 | 1.97 | 0.00 | 1.28 | -12.82 | 223.05 | 38.12 | 247.87 | 0.6521 | -701.0 | -630.1 | |
| 0.00 | 1.46 | 0.00 | 0.95 | -13.09 | 223.02 | 38.09 | 247.46 | 0.6529 | -721.0 | -559.6 | |
| 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. | |