SDO HMI 2014-05-26 23:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.23 | 0.00 | 7.11 | -18.87 | 50.41 | -14.11 | 143.12 | 0.3826 | 545.9 | 459.5 | |
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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 | 0.99 | 0.00 | 0.52 | -18.40 | 55.23 | -9.30 | 152.48 | 0.3332 | 738.0 | 594.0 | |
| 0.00 | 1.44 | 0.00 | 0.75 | -15.80 | 53.34 | -11.18 | 143.34 | 0.3139 | 743.0 | 547.9 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -18.74 | 52.43 | -12.09 | 146.53 | 0.3612 | 930.0 | 778.9 | |
| 0.00 | 1.89 | 0.00 | 1.01 | -18.89 | 51.96 | -12.56 | 145.79 | 0.3676 | 961.0 | 683.3 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -19.05 | 51.65 | -12.87 | 145.41 | 0.3725 | 730.0 | 627.0 | |
| 0.00 | 1.53 | 0.00 | 0.82 | -19.53 | 51.58 | -12.94 | 146.03 | 0.3794 | 968.0 | 760.6 | |
| 0.00 | 0.81 | 0.00 | 0.43 | -18.99 | 51.36 | -13.16 | 144.71 | 0.3743 | 659.0 | 588.1 | |
| 0.00 | 1.80 | 0.00 | 0.95 | -14.85 | 50.72 | -13.80 | 135.52 | 0.3305 | 845.0 | 564.7 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -22.81 | 49.24 | -15.28 | 146.52 | 0.4422 | 754.0 | 618.5 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -22.01 | 42.48 | -22.04 | 135.58 | 0.4991 | -631.0 | -549.4 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -22.33 | 41.78 | -22.74 | 135.22 | 0.5096 | -692.0 | -571.9 | |
| 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. | |