SDO HMI 2011-11-25 23:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.97 | 78.22 | 23.36 | 42.41 | 17.79 | 214.13 | -17.97 | 46.27 | 0.4083 | 478.8 | 129.5 | |
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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 | 1.28 | 0.00 | 0.68 | 17.53 | 217.83 | -14.28 | 40.48 | 0.3639 | 864.0 | 724.1 | |
| 0.00 | 1.88 | 0.00 | 1.01 | 18.58 | 217.42 | -14.69 | 39.35 | 0.3808 | 809.0 | 702.4 | |
| 0.00 | 1.80 | 0.00 | 0.95 | 16.30 | 217.57 | -14.54 | 43.37 | 0.3523 | 838.0 | 598.2 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 13.41 | 216.98 | -15.12 | 50.95 | 0.3283 | 714.0 | 553.4 | |
| 9.76 | 10.61 | 5.22 | 5.67 | 17.15 | 216.12 | -15.98 | 44.32 | 0.3782 | -972.2 | -690.5 | |
| 0.00 | 1.97 | 0.00 | 1.08 | 21.72 | 215.25 | -16.85 | 37.95 | 0.4398 | 718.0 | 642.0 | |
| 0.00 | 0.60 | 0.00 | 0.32 | 18.78 | 215.52 | -16.59 | 42.33 | 0.4032 | 579.0 | 471.6 | |
| 0.00 | 3.77 | 0.00 | 2.02 | 17.27 | 215.53 | -16.57 | 45.09 | 0.3863 | -486.0 | -607.7 | |
| 0.00 | 1.71 | 0.00 | 0.92 | 17.51 | 215.35 | -16.76 | 44.93 | 0.3910 | -823.0 | -641.5 | |
| 0.00 | 5.65 | 0.00 | 3.05 | 18.07 | 215.10 | -17.01 | 44.30 | 0.3999 | -825.0 | -744.5 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 21.02 | 214.44 | -17.67 | 40.30 | 0.4398 | 644.0 | 484.9 | |
| 0.00 | 1.88 | 0.00 | 1.02 | 18.03 | 214.74 | -17.36 | 44.93 | 0.4035 | -739.0 | -561.8 | |
| 33.21 | 44.76 | 18.14 | 24.45 | 17.83 | 212.83 | -19.27 | 48.16 | 0.4236 | 1060.3 | 662.6 | |
| 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. | |