SDO HMI 2014-10-01 18:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.07 | 0.00 | 10.64 | -4.95 | 139.25 | -35.60 | 107.25 | 0.6096 | -662.9 | -554.2 | |
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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 | 1.67 | 0.00 | 1.03 | -4.23 | 140.11 | -34.73 | 106.55 | 0.5950 | -785.0 | -646.9 | |
| 0.00 | 0.97 | 0.00 | 0.60 | -5.37 | 139.97 | -34.88 | 108.30 | 0.6019 | -725.0 | -591.7 | |
| 0.00 | 0.97 | 0.00 | 0.60 | -3.87 | 140.02 | -34.83 | 105.92 | 0.5947 | -740.0 | -647.1 | |
| 0.00 | 1.32 | 0.00 | 0.82 | -4.96 | 139.70 | -35.15 | 107.51 | 0.6036 | -871.0 | -734.0 | |
| 0.00 | 1.67 | 0.00 | 1.04 | -4.96 | 139.22 | -35.63 | 107.27 | 0.6099 | -713.0 | -568.4 | |
| 0.00 | 1.41 | 0.00 | 0.87 | -3.71 | 139.21 | -35.63 | 105.29 | 0.6049 | -606.0 | -475.0 | |
| 0.00 | 1.85 | 0.00 | 1.15 | -5.12 | 139.13 | -35.71 | 107.47 | 0.6117 | -376.0 | -371.0 | |
| 0.00 | 1.32 | 0.00 | 0.82 | -3.96 | 139.13 | -35.72 | 105.64 | 0.6070 | -790.0 | -623.9 | |
| 0.00 | 1.50 | 0.00 | 0.94 | -6.06 | 138.91 | -35.93 | 108.81 | 0.6187 | -539.0 | -517.0 | |
| 0.00 | 1.67 | 0.00 | 1.05 | -6.46 | 138.84 | -36.00 | 109.39 | 0.6214 | -803.0 | -747.6 | |
| 0.00 | 1.23 | 0.00 | 0.77 | -5.49 | 138.73 | -36.11 | 107.84 | 0.6185 | -673.0 | -367.9 | |
| 0.00 | 0.79 | 0.00 | 0.50 | -3.72 | 138.69 | -36.15 | 105.06 | 0.6119 | -534.0 | -449.4 | |
| 0.00 | 0.70 | 0.00 | 0.45 | -5.86 | 138.22 | -36.63 | 108.15 | 0.6268 | -463.0 | -364.6 | |
| 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. | |