SDO HMI 2014-11-24 10:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.22 | 0.00 | 11.31 | -12.65 | 225.80 | 38.69 | 248.32 | 0.6580 | -17.4 | -5.8 | |
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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 | 2.48 | 0.00 | 1.70 | -12.83 | 228.74 | 41.63 | 249.36 | 0.6944 | 448.0 | 377.2 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -12.92 | 228.59 | 41.48 | 249.18 | 0.6930 | 557.0 | 526.3 | |
| 0.00 | 0.60 | 0.00 | 0.41 | -12.57 | 228.12 | 41.01 | 249.48 | 0.6862 | 638.0 | 547.0 | |
| 0.00 | 2.91 | 0.00 | 1.97 | -13.12 | 227.83 | 40.71 | 248.59 | 0.6847 | 731.0 | 663.0 | |
| 0.00 | 0.43 | 0.00 | 0.29 | -13.70 | 227.90 | 40.79 | 247.81 | 0.6878 | 545.0 | 570.2 | |
| 0.00 | 1.63 | 0.00 | 1.09 | -12.86 | 227.33 | 40.22 | 248.74 | 0.6778 | 681.0 | 573.4 | |
| 0.00 | 1.80 | 0.00 | 1.16 | -12.98 | 224.35 | 37.24 | 247.19 | 0.6419 | -419.0 | -389.4 | |
| 0.00 | 1.63 | 0.00 | 1.03 | -10.45 | 223.88 | 36.76 | 250.80 | 0.6256 | -689.0 | -577.3 | |
| 0.00 | 0.94 | 0.00 | 0.60 | -11.60 | 223.90 | 36.78 | 249.04 | 0.6304 | -613.0 | -511.2 | |
| 0.00 | 1.03 | 0.00 | 0.66 | -12.95 | 224.08 | 36.96 | 247.11 | 0.6384 | -693.0 | -531.4 | |
| 0.00 | 1.80 | 0.00 | 1.14 | -12.86 | 222.89 | 35.78 | 246.63 | 0.6232 | -752.0 | -680.3 | |
| 0.00 | 1.71 | 0.00 | 1.08 | -12.95 | 222.60 | 35.49 | 246.34 | 0.6200 | -643.0 | -601.4 | |
| 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. | |