SDO HMI 2014-04-06 22:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.69 | 0.00 | 9.18 | -15.85 | 352.11 | -13.76 | 126.93 | 0.2921 | -835.5 | -666.7 | |
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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 | 2.11 | 0.00 | 1.08 | -17.35 | 356.54 | -9.33 | 141.48 | 0.2497 | -880.0 | -675.8 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -17.74 | 355.98 | -9.90 | 140.88 | 0.2606 | -798.0 | -670.9 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -12.84 | 354.02 | -11.85 | 120.41 | 0.2332 | -767.0 | -661.7 | |
| 0.00 | 2.64 | 0.00 | 1.36 | -15.83 | 353.57 | -12.30 | 129.55 | 0.2671 | -920.0 | -674.9 | |
| 0.00 | 2.11 | 0.00 | 1.10 | -18.14 | 353.02 | -12.85 | 134.69 | 0.2986 | -843.0 | -699.5 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -21.74 | 352.52 | -13.36 | 141.56 | 0.3467 | -797.0 | -638.3 | |
| 0.00 | 1.94 | 0.00 | 1.00 | -15.72 | 352.97 | -12.90 | 127.97 | 0.2739 | -921.0 | -721.8 | |
| 0.00 | 2.55 | 0.00 | 1.31 | -9.69 | 350.27 | -15.60 | 103.69 | 0.2741 | -893.0 | -634.1 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -17.97 | 348.36 | -17.51 | 126.07 | 0.3557 | -821.0 | -628.1 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -15.73 | 346.21 | -19.66 | 117.87 | 0.3680 | -822.0 | -642.4 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -17.61 | 344.96 | -20.91 | 120.98 | 0.3985 | -728.0 | -630.1 | |
| 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. | |