SDO HMI 2014-10-13 02:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.10 | 0.00 | 11.30 | 14.08 | 57.79 | 32.49 | 286.84 | 0.5457 | 102.6 | 161.0 | |
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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 | 1.05 | 0.00 | 0.69 | 11.51 | 66.42 | 41.12 | 280.61 | 0.6580 | -569.0 | -491.4 | |
| 0.00 | 0.70 | 0.00 | 0.46 | 13.03 | 66.31 | 41.01 | 282.94 | 0.6583 | -639.0 | -563.5 | |
| 0.00 | 0.79 | 0.00 | 0.50 | 9.27 | 63.77 | 38.47 | 277.33 | 0.6214 | -695.0 | -519.3 | |
| 0.00 | 0.88 | 0.00 | 0.53 | 13.27 | 60.14 | 34.84 | 284.55 | 0.5767 | 706.0 | 611.1 | |
| 0.00 | 1.49 | 0.00 | 0.91 | 17.37 | 59.90 | 34.61 | 291.58 | 0.5851 | -445.0 | -394.5 | |
| 0.00 | 0.61 | 0.00 | 0.37 | 16.73 | 59.39 | 34.09 | 290.70 | 0.5760 | -645.0 | -600.0 | |
| 0.00 | 2.63 | 0.00 | 1.58 | 16.20 | 59.06 | 33.76 | 289.93 | 0.5698 | -620.0 | -500.0 | |
| 0.00 | 1.49 | 0.00 | 0.86 | 13.43 | 55.73 | 30.44 | 286.16 | 0.5151 | 518.0 | 445.1 | |
| 0.00 | 1.23 | 0.00 | 0.70 | 13.48 | 55.38 | 30.09 | 286.38 | 0.5102 | 788.0 | 684.5 | |
| 0.00 | 4.11 | 0.00 | 2.36 | 13.78 | 54.89 | 29.60 | 287.15 | 0.5040 | 687.0 | 614.3 | |
| 0.00 | 2.28 | 0.00 | 1.30 | 14.11 | 54.41 | 29.11 | 288.00 | 0.4981 | 742.0 | 588.7 | |
| 0.00 | 0.79 | 0.00 | 0.45 | 13.63 | 54.31 | 29.01 | 287.09 | 0.4951 | 723.0 | 657.8 | |
| 0.00 | 1.05 | 0.00 | 0.59 | 13.38 | 53.78 | 28.49 | 286.82 | 0.4867 | 783.0 | 587.2 | |
| 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. | |