SDO HMI 2011-11-24 05:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.45 | 166.90 | 27.49 | 180.31 | 19.15 | 193.57 | -61.61 | 69.30 | 0.8893 | -434.0 | -144.4 | |
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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 | 0.94 | 0.00 | 0.90 | 17.19 | 197.46 | -57.72 | 70.91 | 0.8568 | -392.0 | -347.5 | |
| 1.20 | 145.83 | 1.27 | 152.87 | 19.28 | 194.25 | -60.92 | 69.05 | 0.8853 | -178.6 | -198.3 | |
| 20.91 | -2.00 | 21.87 | -2.00 | 18.79 | 194.50 | -60.68 | 69.57 | 0.8828 | -786.5 | 999999 | |
| 0.51 | 3.77 | 0.57 | 4.16 | 18.59 | 192.77 | -62.41 | 70.05 | 0.8956 | -276.8 | -263.3 | |
| 0.00 | 0.77 | 0.00 | 0.86 | 18.77 | 192.65 | -62.53 | 69.86 | 0.8966 | -201.0 | -231.4 | |
| 0.00 | 0.86 | 0.00 | 1.22 | 24.79 | 186.78 | -68.39 | 64.16 | 0.9393 | 116.0 | 141.8 | |
| 0.00 | 1.11 | 0.00 | 1.36 | 20.97 | 190.16 | -65.02 | 67.80 | 0.9159 | 233.0 | 210.0 | |
| 0.00 | 1.37 | 0.00 | 1.62 | 19.79 | 190.94 | -64.24 | 68.98 | 0.9096 | 398.0 | 334.9 | |
| 1.46 | 3.00 | 1.92 | 3.95 | 21.23 | 188.19 | -66.99 | 67.77 | 0.9285 | 498.9 | 362.2 | |
| 1.37 | 2.06 | 1.86 | 2.79 | 21.66 | 187.54 | -67.64 | 67.39 | 0.9327 | 457.2 | 454.4 | |
| 0.00 | 1.88 | 0.00 | 2.74 | 22.25 | 185.95 | -69.22 | 66.95 | 0.9420 | 377.0 | 354.8 | |
| 0.00 | 5.31 | 0.00 | 7.84 | 21.92 | 185.58 | -69.60 | 67.33 | 0.9438 | 279.0 | 253.6 | |
| 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. | |