SDO HMI 2011-06-07 22:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.45 | 57.01 | 17.69 | 44.67 | 17.43 | 20.14 | 48.52 | 292.69 | 0.7765 | -366.3 | -178.0 | |
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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 |
| 5.16 | 10.41 | 4.16 | 8.37 | 17.07 | 21.65 | 50.02 | 291.75 | 0.7910 | -455.3 | -291.7 | |
| 2.99 | 7.15 | 2.39 | 5.70 | 17.13 | 21.22 | 49.60 | 291.95 | 0.7869 | -586.8 | -563.2 | |
| 4.07 | 19.09 | 3.22 | 15.02 | 16.68 | 20.82 | 49.20 | 291.52 | 0.7817 | -599.1 | -516.9 | |
| 5.61 | -3.00 | 4.40 | -3.00 | 16.68 | 20.38 | 48.76 | 291.65 | 0.7772 | -751.4 | 999999 | |
| 1.90 | 8.14 | 1.54 | 6.62 | 19.38 | 21.36 | 49.73 | 294.67 | 0.7943 | 393.4 | 186.6 | |
| 0.00 | 1.09 | 0.00 | 0.89 | 19.86 | 21.51 | 49.89 | 295.21 | 0.7972 | -444.0 | -373.8 | |
| 1.36 | 2.44 | 1.01 | 1.82 | 16.85 | 17.74 | 46.12 | 292.69 | 0.7501 | -638.1 | -255.6 | |
| 0.00 | 1.09 | 0.00 | 0.80 | 17.00 | 17.15 | 45.53 | 293.11 | 0.7442 | -695.0 | -614.6 | |
| 1.36 | 5.34 | 0.97 | 3.83 | 17.68 | 15.07 | 43.45 | 294.77 | 0.7239 | 603.0 | 485.9 | |
| 0.00 | 1.36 | 0.00 | 0.97 | 17.90 | 15.05 | 43.43 | 295.07 | 0.7245 | 564.0 | 505.3 | |
| 0.00 | 0.90 | 0.00 | 0.65 | 18.93 | 15.20 | 43.58 | 296.35 | 0.7300 | 615.0 | 496.1 | |
| 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. | |