SDO HMI 2014-11-23 18:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.24 | 0.00 | 9.06 | -12.63 | 226.28 | 30.38 | 243.49 | 0.5531 | -62.0 | 138.9 | |
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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 | 1.11 | 0.00 | 0.68 | -13.29 | 228.72 | 32.82 | 244.12 | 0.5886 | 606.0 | 524.6 | |
| 0.00 | 1.63 | 0.00 | 0.99 | -12.49 | 228.50 | 32.60 | 245.25 | 0.5814 | 660.0 | 591.7 | |
| 0.00 | 3.34 | 0.00 | 2.03 | -12.73 | 228.24 | 32.34 | 244.70 | 0.5794 | 782.0 | 619.3 | |
| 0.00 | 1.28 | 0.00 | 0.78 | -12.67 | 227.91 | 32.01 | 244.60 | 0.5748 | 845.0 | 748.1 | |
| 0.00 | 1.88 | 0.00 | 1.13 | -13.87 | 226.58 | 30.69 | 241.75 | 0.5647 | 571.0 | 492.7 | |
| 0.00 | 1.63 | 0.00 | 0.94 | -11.74 | 223.80 | 27.91 | 243.25 | 0.5152 | -756.0 | -635.5 | |
| 0.00 | 0.77 | 0.00 | 0.44 | -10.61 | 223.69 | 27.79 | 245.18 | 0.5069 | -597.0 | -484.6 | |
| 0.00 | 1.11 | 0.00 | 0.64 | -11.52 | 223.47 | 27.57 | 243.37 | 0.5094 | -686.0 | -581.3 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -12.80 | 223.58 | 27.68 | 241.20 | 0.5191 | -686.0 | -613.4 | |
| 0.00 | 0.86 | 0.00 | 0.49 | -12.68 | 223.43 | 27.53 | 241.29 | 0.5163 | -828.0 | -735.5 | |
| 0.00 | 0.77 | 0.00 | 0.44 | -13.47 | 222.94 | 27.04 | 239.50 | 0.5153 | -593.0 | -505.9 | |
| 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. | |