SDO HMI 2014-11-06 02:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.78 | 0.00 | 7.95 | -18.34 | 98.66 | 29.88 | 231.46 | 0.6055 | -161.6 | 7.9 | |
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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 | 1.12 | 0.00 | 0.74 | -15.89 | 105.04 | 36.26 | 240.21 | 0.6578 | 372.0 | 253.6 | |
| 0.00 | 1.38 | 0.00 | 0.90 | -17.05 | 104.18 | 35.40 | 238.05 | 0.6550 | 729.0 | 593.0 | |
| 0.00 | 1.12 | 0.00 | 0.73 | -17.21 | 104.09 | 35.32 | 237.79 | 0.6550 | 638.0 | 567.8 | |
| 0.00 | 1.04 | 0.00 | 0.66 | -18.01 | 101.07 | 32.29 | 234.46 | 0.6266 | 350.0 | 314.6 | |
| 0.00 | 2.07 | 0.00 | 1.31 | -17.72 | 100.90 | 32.12 | 234.73 | 0.6226 | 600.0 | 501.5 | |
| 0.00 | 0.86 | 0.00 | 0.54 | -21.07 | 98.25 | 29.48 | 227.98 | 0.6203 | -580.0 | -444.5 | |
| 0.00 | 0.95 | 0.00 | 0.58 | -17.38 | 97.08 | 28.30 | 231.88 | 0.5773 | -626.0 | -502.3 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -17.38 | 95.11 | 26.33 | 229.94 | 0.5553 | -746.0 | -558.1 | |
| 0.00 | 0.52 | 0.00 | 0.31 | -18.86 | 93.29 | 24.52 | 225.88 | 0.5492 | -622.0 | -569.8 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -18.12 | 92.09 | 23.31 | 225.52 | 0.5292 | -641.0 | -563.1 | |
| 0.00 | 0.78 | 0.00 | 0.46 | -22.52 | 90.04 | 21.27 | 217.26 | 0.5555 | -748.0 | -593.8 | |
| 0.00 | 1.04 | 0.00 | 0.61 | -22.36 | 89.09 | 20.31 | 216.22 | 0.5454 | -665.0 | -543.8 | |
| 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. | |