SDO HMI 2014-10-02 13:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.73 | 0.00 | 13.85 | -4.93 | 139.10 | -25.30 | 113.97 | 0.4683 | -727.6 | -614.7 | |
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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 | 0.49 | -4.34 | 140.47 | -23.94 | 114.05 | 0.4448 | -812.0 | -664.4 | |
| 0.00 | 1.58 | 0.00 | 0.88 | -4.58 | 139.83 | -24.57 | 113.96 | 0.4555 | -865.0 | -751.9 | |
| 0.00 | 1.85 | 0.00 | 1.04 | -6.37 | 139.52 | -24.89 | 117.16 | 0.4720 | -772.0 | -530.5 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -4.16 | 139.58 | -24.82 | 112.90 | 0.4564 | -802.0 | -637.0 | |
| 0.00 | 1.32 | 0.00 | 0.74 | -5.83 | 139.24 | -25.16 | 115.87 | 0.4720 | -908.0 | -769.7 | |
| 0.00 | 4.84 | 0.00 | 2.71 | -5.47 | 139.16 | -25.24 | 115.10 | 0.4707 | -831.0 | -654.3 | |
| 0.00 | 0.97 | 0.00 | 0.54 | -4.67 | 139.16 | -25.24 | 113.55 | 0.4655 | -676.0 | -507.0 | |
| 0.00 | 2.55 | 0.00 | 1.44 | -6.37 | 139.02 | -25.39 | 116.67 | 0.4788 | -736.0 | -697.4 | |
| 0.00 | 2.11 | 0.00 | 1.18 | -4.07 | 139.09 | -25.32 | 112.28 | 0.4629 | -416.0 | -369.1 | |
| 0.00 | 3.70 | 0.00 | 2.06 | -3.37 | 139.04 | -25.36 | 110.83 | 0.4594 | -762.0 | -668.3 | |
| 0.00 | 1.76 | 0.00 | 1.00 | -6.49 | 138.51 | -25.90 | 116.42 | 0.4865 | -654.0 | -501.2 | |
| 0.00 | 0.97 | 0.00 | 0.54 | -2.92 | 138.32 | -26.08 | 109.36 | 0.4673 | -666.0 | -588.6 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -3.51 | 136.85 | -27.55 | 109.47 | 0.4916 | -559.0 | -513.4 | |
| 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. | |