SDO HMI 2014-10-02 00:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.92 | 0.00 | 11.33 | -5.09 | 139.33 | -32.20 | 109.33 | 0.5648 | -788.8 | -641.5 | |
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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 | 1.94 | 0.00 | 1.15 | -4.36 | 140.09 | -31.44 | 108.57 | 0.5507 | -973.0 | -753.9 | |
| 0.00 | 1.14 | 0.00 | 0.68 | -4.96 | 139.78 | -31.75 | 109.40 | 0.5580 | -760.0 | -613.5 | |
| 0.00 | 1.32 | 0.00 | 0.78 | -4.10 | 139.79 | -31.74 | 107.94 | 0.5537 | -872.0 | -735.5 | |
| 0.00 | 1.32 | 0.00 | 0.79 | -4.33 | 139.60 | -31.93 | 108.22 | 0.5574 | -698.0 | -587.3 | |
| 0.00 | 1.14 | 0.00 | 0.68 | -4.82 | 139.50 | -32.03 | 109.00 | 0.5611 | -862.0 | -605.8 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -4.95 | 139.39 | -32.14 | 109.15 | 0.5632 | -713.0 | -628.1 | |
| 0.00 | 2.47 | 0.00 | 1.48 | -5.12 | 139.24 | -32.29 | 109.33 | 0.5661 | -641.0 | -478.2 | |
| 0.00 | 2.29 | 0.00 | 1.38 | -6.41 | 139.12 | -32.41 | 111.40 | 0.5743 | -880.0 | -753.5 | |
| 0.00 | 1.58 | 0.00 | 0.95 | -3.96 | 139.12 | -32.41 | 107.32 | 0.5623 | -862.0 | -677.5 | |
| 0.00 | 1.58 | 0.00 | 0.96 | -5.93 | 138.93 | -32.60 | 110.50 | 0.5742 | -764.0 | -636.6 | |
| 0.00 | 1.41 | 0.00 | 0.85 | -6.64 | 138.88 | -32.65 | 111.62 | 0.5786 | -718.0 | -587.1 | |
| 0.00 | 1.06 | 0.00 | 0.63 | -4.09 | 138.97 | -32.56 | 107.46 | 0.5649 | -699.0 | -594.4 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -5.51 | 138.82 | -32.71 | 109.74 | 0.5737 | -813.0 | -685.2 | |
| 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. | |