SDO HMI 2014-09-13 10:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.41 | 104.31 | 14.95 | 56.86 | -15.84 | 66.07 | 9.24 | 201.60 | 0.4218 | 767.7 | 527.2 | |
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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 | 1.87 | 0.00 | 1.03 | -16.12 | 68.62 | 11.79 | 206.52 | 0.4416 | -808.0 | -583.1 | |
| 0.89 | 1.60 | 0.49 | 0.88 | -16.35 | 67.55 | 10.72 | 204.17 | 0.4377 | 646.7 | 568.9 | |
| 3.29 | 7.21 | 1.80 | 3.95 | -15.94 | 66.95 | 10.12 | 203.35 | 0.4281 | 891.2 | 611.7 | |
| 0.00 | 1.07 | 0.00 | 0.59 | -16.36 | 66.85 | 10.02 | 202.74 | 0.4336 | 745.0 | 588.0 | |
| 0.00 | 1.25 | 0.00 | 0.68 | -16.30 | 66.71 | 9.89 | 202.53 | 0.4318 | 719.0 | 630.7 | |
| 3.47 | 84.99 | 1.90 | 46.27 | -15.87 | 66.60 | 9.77 | 202.69 | 0.4248 | 913.1 | 584.5 | |
| 0.36 | -6.00 | 0.19 | -6.00 | -16.06 | 66.32 | 9.49 | 201.94 | 0.4260 | 741.2 | 999999 | |
| 6.05 | -6.00 | 3.30 | -6.00 | -15.76 | 66.27 | 9.45 | 202.11 | 0.4213 | 1033.7 | 999999 | |
| 4.72 | -6.00 | 2.57 | -6.00 | -15.66 | 66.08 | 9.25 | 201.79 | 0.4187 | 1136.4 | 999999 | |
| 0.00 | 1.69 | 0.00 | 0.92 | -16.02 | 66.00 | 9.17 | 201.30 | 0.4235 | 247.0 | 259.6 | |
| 8.63 | -6.00 | 4.70 | -6.00 | -15.52 | 65.82 | 8.99 | 201.36 | 0.4152 | 1264.7 | 999999 | |
| 0.00 | 1.25 | 0.00 | 0.68 | -16.26 | 64.99 | 8.16 | 198.95 | 0.4216 | 896.0 | 753.9 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -18.46 | 63.81 | 6.98 | 194.92 | 0.4493 | 685.0 | 641.1 | |
| 0.00 | 1.78 | 0.00 | 0.98 | -18.34 | 59.46 | 2.63 | 185.78 | 0.4353 | -113.0 | -188.0 | |
| 0.00 | 0.62 | 0.00 | 0.34 | -18.10 | 58.57 | 1.74 | 183.87 | 0.4303 | -678.0 | -508.7 | |
| 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. | |