SDO HMI 2014-11-24 08:16:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.80 | 0.00 | 9.03 | -12.88 | 226.34 | 38.29 | 247.79 | 0.6541 | 62.5 | 108.3 | |
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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 | 2.49 | 0.00 | 1.68 | -12.80 | 228.71 | 40.66 | 249.00 | 0.6829 | 412.0 | 419.8 | |
| 0.00 | 0.26 | 0.00 | 0.17 | -12.92 | 228.61 | 40.56 | 248.79 | 0.6822 | 524.0 | 488.0 | |
| 0.00 | 1.29 | 0.00 | 0.87 | -13.31 | 228.41 | 40.36 | 248.15 | 0.6812 | 398.0 | 358.0 | |
| 0.00 | 1.54 | 0.00 | 1.03 | -13.09 | 227.77 | 39.71 | 248.19 | 0.6727 | 859.0 | 719.4 | |
| 0.00 | 0.60 | 0.00 | 0.40 | -13.64 | 227.76 | 39.70 | 247.41 | 0.6747 | 231.0 | 358.3 | |
| 0.00 | 0.94 | 0.00 | 0.63 | -13.30 | 227.57 | 39.52 | 247.81 | 0.6711 | 522.0 | 515.0 | |
| 0.00 | 1.54 | 0.00 | 1.02 | -12.83 | 227.33 | 39.27 | 248.36 | 0.6663 | 705.0 | 644.7 | |
| 0.00 | 1.11 | 0.00 | 0.71 | -12.89 | 224.03 | 35.97 | 246.68 | 0.6258 | -665.0 | -542.8 | |
| 0.00 | 1.29 | 0.00 | 0.81 | -11.66 | 223.76 | 35.71 | 248.41 | 0.6170 | -706.0 | -580.9 | |
| 0.00 | 1.37 | 0.00 | 0.86 | -12.80 | 222.82 | 34.77 | 246.16 | 0.6102 | -824.0 | -695.8 | |
| 0.00 | 1.37 | 0.00 | 0.85 | -12.95 | 222.55 | 34.49 | 245.77 | 0.6075 | -768.0 | -636.5 | |
| 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. | |