SDO HMI 2014-11-02 03:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.20 | 27.78 | 1.78 | 16.33 | -17.54 | 97.11 | -23.86 | 134.15 | 0.5336 | -346.9 | -42.8 | |
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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 |
| 0.78 | 5.37 | 0.43 | 2.99 | -16.35 | 102.97 | -18.01 | 139.64 | 0.4600 | 1032.2 | 778.7 | |
| 2.42 | 7.44 | 1.35 | 4.15 | -16.27 | 102.65 | -18.32 | 139.02 | 0.4622 | 967.9 | 832.9 | |
| 0.00 | 1.73 | 0.00 | 1.04 | -17.53 | 94.22 | -26.75 | 130.31 | 0.5650 | -795.0 | -637.5 | |
| 0.00 | 1.64 | 0.00 | 1.00 | -18.79 | 93.94 | -27.03 | 131.77 | 0.5791 | -790.0 | -653.9 | |
| 0.00 | 0.87 | 0.00 | 0.52 | -17.76 | 94.01 | -26.96 | 130.42 | 0.5693 | -636.0 | -497.3 | |
| 0.00 | 1.21 | 0.00 | 0.74 | -18.83 | 93.72 | -27.25 | 131.61 | 0.5818 | -535.0 | -502.5 | |
| 0.00 | 0.87 | 0.00 | 0.53 | -18.90 | 93.57 | -27.41 | 131.55 | 0.5841 | -611.0 | -503.1 | |
| 0.00 | 1.21 | 0.00 | 0.73 | -17.56 | 93.41 | -27.56 | 129.53 | 0.5742 | -839.0 | -637.7 | |
| 0.00 | 1.38 | 0.00 | 0.84 | -17.69 | 93.28 | -27.69 | 129.59 | 0.5767 | -439.0 | -412.2 | |
| 0.00 | 0.78 | 0.00 | 0.49 | -19.56 | 91.43 | -29.54 | 130.39 | 0.6123 | -591.0 | -541.6 | |
| 0.00 | 1.38 | 0.00 | 0.85 | -17.01 | 91.87 | -29.10 | 127.29 | 0.5868 | -806.0 | -522.5 | |
| 0.00 | 0.78 | 0.00 | 0.49 | -19.41 | 91.28 | -29.69 | 130.04 | 0.6126 | -504.0 | -479.4 | |
| 0.00 | 2.25 | 0.00 | 1.41 | -19.55 | 90.96 | -30.01 | 129.94 | 0.6171 | -721.0 | -472.7 | |
| 0.00 | 0.87 | 0.00 | 0.55 | -20.06 | 90.48 | -30.49 | 130.18 | 0.6261 | -643.0 | -576.3 | |
| 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. | |