SDO HMI 2014-10-08 11:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.73 | 0.00 | 7.25 | -16.34 | 104.14 | 17.80 | 217.02 | 0.4954 | -13.4 | 21.5 | |
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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 | 0.88 | 0.00 | 0.52 | -16.46 | 111.45 | 25.12 | 227.19 | 0.5570 | 458.0 | 379.9 | |
| 0.00 | 1.05 | 0.00 | 0.61 | -13.88 | 110.65 | 24.32 | 229.98 | 0.5241 | 740.0 | 615.7 | |
| 0.00 | 2.02 | 0.00 | 1.17 | -13.36 | 110.49 | 24.16 | 230.58 | 0.5175 | 762.0 | 676.6 | |
| 0.00 | 1.05 | 0.00 | 0.61 | -15.17 | 110.26 | 23.92 | 227.62 | 0.5319 | 723.0 | 541.6 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -14.20 | 109.40 | 23.07 | 228.00 | 0.5132 | 650.0 | 501.2 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -20.02 | 104.16 | 17.83 | 213.26 | 0.5266 | 411.0 | 279.1 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -9.25 | 102.72 | 16.38 | 226.54 | 0.3852 | -807.0 | -718.8 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -18.96 | 99.38 | 13.04 | 206.70 | 0.4770 | -808.0 | -692.7 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -19.02 | 97.92 | 11.59 | 204.03 | 0.4682 | -731.0 | -582.1 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -22.24 | 93.97 | 7.63 | 194.45 | 0.4946 | -825.0 | -673.3 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -18.82 | 89.35 | 3.01 | 186.69 | 0.4293 | -720.0 | -618.4 | |
| 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. | |