SDO HMI 2014-11-08 08:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.46 | 0.00 | 11.44 | -14.14 | 18.21 | -20.91 | 131.12 | 0.4606 | -359.3 | -246.8 | |
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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 | 1.64 | 0.00 | 0.87 | -8.07 | 22.37 | -16.76 | 125.00 | 0.3500 | 1.0 | -0.4 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -12.79 | 21.90 | -17.22 | 134.10 | 0.4037 | 635.0 | 514.2 | |
| 0.00 | 3.19 | 0.00 | 1.74 | -13.57 | 21.81 | -17.31 | 135.34 | 0.4133 | 862.0 | 739.8 | |
| 0.00 | 1.73 | 0.00 | 0.94 | -13.32 | 21.74 | -17.39 | 134.78 | 0.4114 | 958.0 | 805.2 | |
| 0.00 | 1.29 | 0.00 | 0.71 | -14.16 | 20.06 | -19.07 | 133.64 | 0.4395 | -829.0 | -703.7 | |
| 0.00 | 1.29 | 0.00 | 0.71 | -13.94 | 20.08 | -19.05 | 133.29 | 0.4370 | -957.0 | -805.3 | |
| 0.00 | 1.47 | 0.00 | 0.81 | -10.16 | 16.98 | -22.15 | 122.18 | 0.4403 | -789.0 | -636.9 | |
| 0.00 | 1.38 | 0.00 | 0.79 | -16.29 | 16.30 | -22.82 | 132.04 | 0.5034 | -833.0 | -666.2 | |
| 0.00 | 3.62 | 0.00 | 2.08 | -16.23 | 15.87 | -23.25 | 131.44 | 0.5077 | -889.0 | -774.1 | |
| 0.00 | 1.04 | 0.00 | 0.60 | -16.59 | 15.69 | -23.43 | 131.76 | 0.5131 | -689.0 | -633.8 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -17.67 | 15.30 | -23.82 | 132.93 | 0.5277 | -758.0 | -594.6 | |
| 0.00 | 1.04 | 0.00 | 0.61 | -17.48 | 14.13 | -24.99 | 131.33 | 0.5388 | -655.0 | -528.0 | |
| 0.00 | 1.04 | 0.00 | 0.61 | -13.27 | 11.06 | -28.06 | 121.74 | 0.5405 | -728.0 | -524.2 | |
| 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. | |