SDO HMI 2011-11-29 03:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.02 | 158.04 | 25.88 | 110.57 | 15.79 | 233.42 | 43.05 | 291.42 | 0.7080 | -780.9 | -335.5 | |
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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 | 1.03 | 0.00 | 0.74 | 16.74 | 235.36 | 44.99 | 292.05 | 0.7328 | -353.0 | -334.5 | |
| 0.00 | 3.16 | 0.00 | 2.30 | 17.61 | 235.33 | 44.95 | 293.20 | 0.7350 | -619.0 | -447.6 | |
| 0.00 | 1.71 | 0.00 | 1.24 | 17.73 | 235.15 | 44.77 | 293.43 | 0.7335 | -697.0 | -595.5 | |
| 0.34 | 3.51 | 0.25 | 2.54 | 17.95 | 234.95 | 44.58 | 293.79 | 0.7321 | -689.2 | -644.2 | |
| 27.96 | 126.57 | 19.51 | 88.37 | 15.42 | 233.40 | 43.03 | 290.92 | 0.7066 | -989.3 | -287.3 | |
| 1.37 | 2.05 | 0.99 | 1.48 | 19.08 | 234.32 | 43.95 | 295.51 | 0.7290 | 358.0 | 275.0 | |
| 5.13 | 8.89 | 3.59 | 6.21 | 16.59 | 233.25 | 42.88 | 292.57 | 0.7086 | -619.4 | -581.5 | |
| 2.22 | -5.00 | 1.54 | -5.00 | 15.79 | 232.91 | 42.54 | 291.60 | 0.7021 | -900.0 | 999999 | |
| 0.00 | 4.53 | 0.00 | 3.15 | 16.25 | 232.87 | 42.50 | 292.25 | 0.7031 | -876.0 | -724.6 | |
| 0.00 | 2.31 | 0.00 | 1.60 | 16.01 | 232.64 | 42.26 | 292.00 | 0.6996 | -450.0 | -424.4 | |
| 0.00 | 0.77 | 0.00 | 0.52 | 14.92 | 232.07 | 41.70 | 290.68 | 0.6894 | -554.0 | -541.7 | |
| 0.00 | 0.34 | 0.00 | 0.24 | 19.04 | 232.80 | 42.42 | 296.06 | 0.7123 | -506.0 | -547.5 | |
| 0.00 | 1.03 | 0.00 | 0.69 | 15.17 | 231.44 | 41.06 | 291.26 | 0.6827 | -207.0 | -148.7 | |
| 0.00 | 1.37 | 0.00 | 0.96 | 19.33 | 232.21 | 41.84 | 296.70 | 0.7069 | -590.0 | -506.4 | |
| 0.00 | 0.77 | 0.00 | 0.53 | 20.31 | 231.14 | 40.76 | 298.50 | 0.6992 | -529.0 | -439.2 | |
| 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. | |