SDO HMI 2014-10-04 23:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.91 | 0.00 | 12.63 | -12.64 | 139.25 | 6.75 | 199.81 | 0.3503 | -83.5 | 160.6 | |
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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 | 1.32 | 0.00 | 0.69 | -11.02 | 141.24 | 8.74 | 206.41 | 0.3369 | 845.0 | 651.8 | |
| 0.00 | 1.85 | 0.00 | 0.95 | -7.61 | 140.70 | 8.20 | 210.16 | 0.2827 | 781.0 | 577.8 | |
| 0.00 | 1.41 | 0.00 | 0.76 | -15.83 | 140.81 | 8.32 | 200.15 | 0.4059 | 733.0 | 572.8 | |
| 0.00 | 7.65 | 0.00 | 3.99 | -10.18 | 140.35 | 7.86 | 205.14 | 0.3182 | 815.0 | 852.3 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -12.48 | 140.07 | 7.58 | 201.62 | 0.3511 | 664.0 | 551.2 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -15.74 | 139.46 | 6.96 | 197.14 | 0.3976 | -833.0 | -667.8 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -18.55 | 138.93 | 6.43 | 194.08 | 0.4383 | -806.0 | -663.7 | |
| 0.00 | 2.90 | 0.00 | 1.59 | -18.21 | 138.56 | 6.07 | 193.51 | 0.4318 | -682.0 | -615.3 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -15.10 | 138.16 | 5.66 | 194.50 | 0.3821 | -809.0 | -670.8 | |
| 0.00 | 1.14 | 0.00 | 0.59 | -10.21 | 137.93 | 5.44 | 197.95 | 0.3038 | 713.0 | 574.6 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -12.52 | 136.10 | 3.60 | 190.63 | 0.3336 | -853.0 | -662.8 | |
| 0.00 | 1.49 | 0.00 | 0.78 | -12.24 | 135.94 | 3.44 | 190.34 | 0.3285 | -910.0 | -689.4 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -12.42 | 135.85 | 3.35 | 189.97 | 0.3313 | -744.0 | -584.5 | |
| 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. | |