SDO HMI 2011-11-29 04:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.31 | 101.00 | 17.65 | 62.88 | 18.14 | 223.63 | 33.81 | 299.21 | 0.6080 | -615.9 | -324.6 | |
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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 | 0.66 | 19.62 | 225.14 | 35.32 | 300.44 | 0.6340 | 670.0 | 585.9 | |
| 4.79 | 22.58 | 3.00 | 14.19 | 17.82 | 224.45 | 34.62 | 298.20 | 0.6161 | -958.3 | -401.4 | |
| 1.20 | 1.28 | 0.76 | 0.81 | 19.00 | 224.61 | 34.78 | 299.87 | 0.6243 | -482.1 | -334.0 | |
| 0.00 | 1.54 | 0.00 | 0.96 | 17.85 | 224.16 | 34.33 | 298.43 | 0.6127 | -865.0 | -723.5 | |
| 0.00 | 1.45 | 0.00 | 0.91 | 17.55 | 223.98 | 34.15 | 298.07 | 0.6089 | -752.0 | -608.0 | |
| 0.00 | 1.45 | 0.00 | 0.91 | 17.76 | 223.91 | 34.08 | 298.44 | 0.6092 | -760.0 | -696.2 | |
| 0.00 | 1.97 | 0.00 | 1.23 | 17.95 | 223.91 | 34.09 | 298.72 | 0.6102 | -794.0 | -704.4 | |
| 1.11 | 2.48 | 0.69 | 1.54 | 17.68 | 223.55 | 33.73 | 298.52 | 0.6044 | -852.0 | -819.9 | |
| 0.00 | 1.20 | 0.00 | 0.73 | 15.10 | 222.98 | 33.15 | 294.81 | 0.5839 | 679.0 | 570.3 | |
| 21.21 | 60.89 | 13.20 | 37.86 | 18.23 | 223.56 | 33.74 | 299.37 | 0.6075 | -967.1 | -331.0 | |
| 0.00 | 1.62 | 0.00 | 0.99 | 19.28 | 221.34 | 31.51 | 302.46 | 0.5870 | -697.0 | -581.8 | |
| 0.00 | 0.77 | 0.00 | 0.46 | 19.01 | 220.29 | 30.47 | 302.82 | 0.5727 | 570.0 | 494.7 | |
| 0.00 | 1.37 | 0.00 | 0.82 | 18.83 | 220.11 | 30.29 | 302.67 | 0.5692 | 751.0 | 593.0 | |
| 0.00 | 1.37 | 0.00 | 0.81 | 20.47 | 217.56 | 27.74 | 307.36 | 0.5507 | 763.0 | 602.0 | |
| 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. | |