SDO HMI 2014-11-10 05:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.16 | 0.00 | 9.03 | -15.62 | 18.32 | 3.93 | 191.66 | 0.3425 | -329.3 | -215.2 | |
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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 | 0.95 | 0.00 | 0.50 | -12.66 | 26.79 | 12.40 | 217.24 | 0.3477 | 677.0 | 544.4 | |
| 0.00 | 1.81 | 0.00 | 0.95 | -14.54 | 23.36 | 8.97 | 206.12 | 0.3441 | 779.0 | 674.4 | |
| 0.00 | 1.38 | 0.00 | 0.73 | -14.35 | 23.29 | 8.90 | 206.20 | 0.3409 | 900.0 | 733.7 | |
| 0.00 | 1.72 | 0.00 | 0.90 | -13.40 | 21.71 | 7.32 | 203.22 | 0.3158 | 914.0 | 755.3 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -15.05 | 20.43 | 6.04 | 197.81 | 0.3338 | -933.0 | -713.7 | |
| 0.00 | 0.78 | 0.00 | 0.41 | -15.75 | 17.05 | 2.66 | 187.74 | 0.3327 | -805.0 | -620.7 | |
| 0.00 | 2.33 | 0.00 | 1.22 | -16.12 | 16.71 | 2.32 | 186.63 | 0.3382 | -1045.0 | -848.7 | |
| 0.00 | 1.29 | 0.00 | 0.69 | -18.44 | 16.46 | 2.07 | 185.25 | 0.3755 | -876.0 | -731.9 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -17.10 | 16.44 | 2.05 | 185.58 | 0.3537 | -680.0 | -476.5 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -16.66 | 15.98 | 1.58 | 184.41 | 0.3458 | -782.0 | -613.5 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -18.50 | 15.18 | 0.78 | 181.99 | 0.3751 | -928.0 | -724.8 | |
| 0.00 | 2.16 | 0.00 | 1.13 | -15.42 | 14.06 | -0.34 | 179.00 | 0.3244 | -832.0 | -639.6 | |
| 0.00 | 0.78 | 0.00 | 0.41 | -16.51 | 7.97 | -6.42 | 162.52 | 0.3585 | -670.0 | -578.8 | |
| 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. | |