SDO HMI 2014-09-24 05:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.34 | 32.01 | 2.66 | 19.46 | -15.45 | 246.76 | -27.60 | 129.61 | 0.5816 | -555.6 | -566.1 | |
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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 | 0.97 | 0.00 | 0.57 | -19.10 | 254.14 | -20.22 | 142.97 | 0.5443 | 704.0 | 570.7 | |
| 0.00 | 1.24 | 0.00 | 0.71 | -15.11 | 252.80 | -21.56 | 136.07 | 0.5134 | 758.0 | 592.3 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -14.48 | 247.51 | -26.85 | 128.95 | 0.5644 | -803.0 | -659.2 | |
| 0.00 | 1.06 | 0.00 | 0.64 | -15.30 | 247.26 | -27.10 | 129.84 | 0.5744 | -762.0 | -596.3 | |
| 0.00 | 3.72 | 0.00 | 2.25 | -15.51 | 247.05 | -27.31 | 129.91 | 0.5785 | -829.0 | -669.0 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -14.21 | 247.13 | -27.23 | 128.17 | 0.5664 | -769.0 | -661.1 | |
| 0.00 | 0.97 | 0.00 | 0.59 | -15.36 | 246.90 | -27.46 | 129.54 | 0.5788 | -730.0 | -604.1 | |
| 0.00 | 1.50 | 0.00 | 0.92 | -15.70 | 246.49 | -27.86 | 129.61 | 0.5862 | -635.0 | -519.8 | |
| 0.00 | 0.62 | 0.00 | 0.38 | -15.51 | 246.49 | -27.87 | 129.34 | 0.5846 | -686.0 | -637.9 | |
| 0.00 | 2.74 | 0.00 | 1.66 | -14.71 | 246.36 | -28.00 | 128.10 | 0.5793 | -903.0 | -694.8 | |
| 0.71 | 3.19 | 0.44 | 1.96 | -16.00 | 245.88 | -28.48 | 129.41 | 0.5954 | -813.5 | -624.9 | |
| 0.00 | 1.50 | 0.00 | 0.93 | -16.13 | 245.86 | -28.50 | 129.56 | 0.5968 | -330.0 | -306.2 | |
| 2.39 | 12.74 | 1.46 | 7.79 | -15.38 | 245.94 | -28.42 | 128.62 | 0.5895 | -890.0 | -756.3 | |
| 1.24 | -13.00 | 0.76 | -13.00 | -15.09 | 245.88 | -28.48 | 128.17 | 0.5878 | -907.7 | 999999 | |
| 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. | |