SDO HMI 2011-06-02 11:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.35 | 164.49 | 19.35 | 95.42 | -20.64 | 19.15 | -24.74 | 131.38 | 0.5235 | 634.3 | 396.1 | |
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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 | 2.08 | 0.00 | 1.16 | -18.40 | 22.83 | -21.05 | 132.05 | 0.4609 | -719.0 | -543.7 | |
| 0.00 | 1.54 | 0.00 | 0.86 | -19.23 | 22.55 | -21.34 | 133.08 | 0.4723 | -735.0 | -543.1 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -19.43 | 22.35 | -21.54 | 133.14 | 0.4764 | -749.0 | -498.1 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -19.94 | 21.68 | -22.20 | 133.15 | 0.4888 | -632.0 | -445.4 | |
| 29.10 | 146.23 | 16.86 | 84.66 | -20.55 | 19.36 | -24.53 | 131.43 | 0.5205 | 1162.6 | 473.3 | |
| 2.89 | -5.00 | 1.69 | -5.00 | -20.84 | 18.70 | -25.19 | 131.17 | 0.5304 | 816.2 | 999999 | |
| 1.36 | 2.62 | 0.80 | 1.54 | -21.42 | 18.34 | -25.55 | 131.68 | 0.5396 | 730.6 | 623.0 | |
| 0.00 | 1.99 | 0.00 | 1.17 | -21.16 | 18.17 | -25.72 | 131.11 | 0.5392 | 727.0 | 607.9 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -20.97 | 18.21 | -25.68 | 130.86 | 0.5371 | 680.0 | 559.7 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -20.67 | 17.94 | -25.95 | 130.14 | 0.5376 | 566.0 | 439.7 | |
| 0.00 | 0.90 | 0.00 | 0.54 | -21.45 | 17.17 | -26.72 | 130.54 | 0.5528 | 575.0 | 435.4 | |
| 0.00 | 1.72 | 0.00 | 1.08 | -23.37 | 12.66 | -31.23 | 129.29 | 0.6171 | -745.0 | -641.1 | |
| 0.00 | 1.36 | 0.00 | 0.86 | -24.03 | 12.05 | -31.83 | 129.70 | 0.6284 | -673.0 | -580.7 | |
| 0.00 | 1.17 | 0.00 | 0.74 | -23.57 | 12.06 | -31.82 | 129.08 | 0.6249 | -610.0 | -524.5 | |
| 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. | |