SDO HMI 2014-11-14 07:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.21 | 0.00 | 8.18 | -9.11 | 339.59 | 19.02 | 236.53 | 0.3865 | -18.2 | -67.2 | |
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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 | 1.98 | 0.00 | 1.09 | -6.27 | 344.74 | 24.18 | 249.08 | 0.4377 | 2.0 | 79.3 | |
| 0.00 | 0.77 | 0.00 | 0.42 | -7.62 | 343.18 | 22.62 | 244.79 | 0.4231 | 889.0 | 734.4 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -8.10 | 343.18 | 22.61 | 243.75 | 0.4262 | 681.0 | 521.5 | |
| 0.00 | 0.86 | 0.00 | 0.47 | -9.89 | 343.07 | 22.50 | 239.93 | 0.4375 | 656.0 | 561.5 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -9.61 | 342.88 | 22.32 | 240.30 | 0.4329 | 752.0 | 581.8 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -9.60 | 342.36 | 21.80 | 239.74 | 0.4257 | 822.0 | 659.1 | |
| 0.00 | 1.20 | 0.00 | 0.66 | -10.91 | 341.00 | 20.43 | 235.42 | 0.4181 | 738.0 | 600.7 | |
| 0.00 | 1.20 | 0.00 | 0.64 | -10.09 | 337.76 | 17.19 | 232.50 | 0.3684 | -671.0 | -632.4 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -9.75 | 337.49 | 16.92 | 232.82 | 0.3616 | -707.0 | -601.1 | |
| 0.00 | 1.20 | 0.00 | 0.63 | -9.29 | 335.15 | 14.59 | 229.76 | 0.3270 | -751.0 | -632.7 | |
| 0.00 | 1.46 | 0.00 | 0.76 | -7.56 | 334.78 | 14.21 | 233.40 | 0.3045 | -855.0 | -652.1 | |
| 0.00 | 1.64 | 0.00 | 0.86 | -10.90 | 334.88 | 14.32 | 225.61 | 0.3413 | -950.0 | -756.9 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -10.80 | 334.60 | 14.03 | 225.24 | 0.3369 | -843.0 | -731.7 | |
| 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. | |