SDO HMI 2011-11-29 11:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.82 | 137.63 | 19.54 | 103.97 | 15.73 | 233.43 | 47.42 | 290.02 | 0.7567 | -732.5 | -312.6 | |
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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 | 0.80 | 16.50 | 235.24 | 49.23 | 290.51 | 0.7776 | -536.0 | -437.9 | |
| 0.00 | 0.51 | 0.00 | 0.41 | 17.67 | 235.56 | 49.56 | 291.88 | 0.7838 | -259.0 | -230.7 | |
| 0.00 | 1.20 | 0.00 | 0.94 | 16.62 | 235.19 | 49.18 | 290.68 | 0.7774 | -588.0 | -426.9 | |
| 0.00 | 1.20 | 0.00 | 0.95 | 17.48 | 235.35 | 49.35 | 291.72 | 0.7812 | -600.0 | -470.3 | |
| 0.43 | 1.62 | 0.34 | 1.29 | 17.79 | 235.42 | 49.41 | 292.08 | 0.7826 | -453.2 | -441.5 | |
| 1.62 | 4.87 | 1.29 | 3.86 | 18.07 | 235.38 | 49.38 | 292.44 | 0.7830 | -608.7 | -450.3 | |
| 0.68 | 105.99 | 0.52 | 79.88 | 15.23 | 233.57 | 47.57 | 289.34 | 0.7571 | -400.0 | -265.7 | |
| 1.71 | -7.00 | 1.29 | -7.00 | 15.11 | 233.36 | 47.35 | 289.24 | 0.7544 | -897.0 | 999999 | |
| 13.68 | -7.00 | 10.30 | -7.00 | 15.48 | 233.37 | 47.37 | 289.71 | 0.7555 | -987.4 | 999999 | |
| 0.60 | -7.00 | 0.45 | -7.00 | 15.05 | 233.11 | 47.11 | 289.23 | 0.7516 | -978.7 | 999999 | |
| 4.36 | 7.61 | 3.30 | 5.75 | 16.74 | 233.32 | 47.31 | 291.36 | 0.7581 | -583.5 | -504.1 | |
| 0.00 | 4.62 | 0.00 | 3.44 | 15.79 | 232.70 | 46.70 | 290.31 | 0.7490 | -884.0 | -751.1 | |
| 2.74 | 4.70 | 2.05 | 3.52 | 16.56 | 232.89 | 46.89 | 291.25 | 0.7531 | -678.5 | -371.5 | |
| 0.00 | 2.22 | 0.00 | 1.62 | 15.26 | 231.65 | 45.65 | 289.91 | 0.7361 | -808.0 | -664.7 | |
| 0.00 | 1.03 | 0.00 | 0.74 | 15.48 | 231.10 | 45.10 | 290.37 | 0.7305 | 264.0 | 228.7 | |
| 0.00 | 1.03 | 0.00 | 0.77 | 19.51 | 232.23 | 46.23 | 295.26 | 0.7550 | -564.0 | -475.8 | |
| 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. | |