SDO HMI 2011-07-01 03:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.45 | 48.68 | 10.35 | 24.72 | 15.26 | 25.08 | 0.66 | 356.46 | 0.2177 | 33.8 | -258.4 | |
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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 | 2.00 | 0.00 | 1.03 | 18.94 | 28.47 | 4.04 | 346.48 | 0.2864 | -780.0 | -563.8 | |
| 11.54 | 15.72 | 5.82 | 7.92 | 13.30 | 26.47 | 2.05 | 349.16 | 0.1856 | 1057.2 | 816.8 | |
| 0.00 | 1.91 | 0.00 | 0.96 | 13.68 | 26.16 | 1.74 | 351.09 | 0.1910 | 642.0 | 396.7 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 15.73 | 24.94 | 0.52 | 357.77 | 0.2242 | -880.0 | -741.7 | |
| 1.73 | 8.99 | 0.88 | 4.58 | 16.36 | 24.72 | 0.30 | 358.78 | 0.2347 | -937.7 | -747.5 | |
| 1.64 | 2.91 | 0.83 | 1.47 | 14.36 | 24.50 | 0.07 | 359.64 | 0.2005 | -959.1 | -753.4 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 16.45 | 24.50 | 0.07 | 359.70 | 0.2363 | -675.0 | -473.7 | |
| 0.00 | 3.18 | 0.00 | 1.62 | 15.92 | 24.44 | 0.01 | 359.95 | 0.2272 | -641.0 | -654.0 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 13.43 | 24.22 | -0.21 | 1.10 | 0.1845 | 841.0 | 561.1 | |
| 4.36 | 4.72 | 2.21 | 2.40 | 15.26 | 23.99 | -0.43 | 1.93 | 0.2161 | -999.9 | -877.0 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 17.08 | 23.29 | -1.14 | 4.41 | 0.2477 | -1006.0 | -862.9 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 20.47 | 22.52 | -1.91 | 5.88 | 0.3057 | -581.0 | -452.4 | |
| 1.18 | 1.36 | 0.61 | 0.70 | 18.02 | 21.49 | -2.94 | 10.55 | 0.2675 | 762.5 | 463.5 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 17.71 | 21.11 | -3.32 | 12.13 | 0.2635 | 947.0 | 721.4 | |
| 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. | |