SDO HMI 2014-10-08 22:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.56 | 0.00 | 11.00 | -20.47 | 73.51 | -6.76 | 167.67 | 0.4694 | 277.6 | 224.0 | |
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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 | 2.10 | 0.00 | 1.13 | -16.15 | 80.46 | 0.19 | 180.47 | 0.3837 | 976.0 | 762.3 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -16.61 | 80.46 | 0.19 | 180.46 | 0.3911 | 735.0 | 620.3 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -21.09 | 82.11 | 1.84 | 183.73 | 0.4630 | 699.0 | 586.2 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -16.95 | 77.91 | -2.36 | 174.30 | 0.3986 | 686.0 | 516.6 | |
| 0.00 | 2.10 | 0.00 | 1.14 | -16.93 | 77.22 | -3.05 | 172.66 | 0.3995 | 771.0 | 704.0 | |
| 0.00 | 1.32 | 0.00 | 0.72 | -19.02 | 79.11 | -1.16 | 177.44 | 0.4301 | 811.0 | 639.1 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -17.71 | 75.09 | -5.18 | 168.06 | 0.4175 | 753.0 | 576.6 | |
| 0.00 | 0.61 | 0.00 | 0.34 | -18.37 | 74.89 | -5.38 | 167.96 | 0.4283 | 724.0 | 577.3 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -15.83 | 68.69 | -11.58 | 152.74 | 0.4234 | 754.0 | 636.6 | |
| 0.00 | 1.32 | 0.00 | 0.74 | -20.71 | 72.17 | -8.10 | 163.78 | 0.4740 | 762.0 | 718.5 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -20.45 | 70.72 | -9.55 | 160.89 | 0.4770 | -507.0 | -345.1 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -21.33 | 68.23 | -12.04 | 157.17 | 0.5030 | -822.0 | -641.5 | |
| 0.00 | 1.05 | 0.00 | 0.61 | -23.48 | 68.25 | -12.03 | 158.88 | 0.5324 | -853.0 | -591.9 | |
| 0.00 | 1.84 | 0.00 | 1.09 | -24.80 | 68.79 | -11.49 | 160.65 | 0.5476 | -715.0 | -506.2 | |
| 0.00 | 1.93 | 0.00 | 1.23 | -29.18 | 63.38 | -16.90 | 156.24 | 0.6321 | -610.0 | -461.2 | |
| 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. | |