SDO HMI 2011-10-20 15:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.97 | 234.47 | 68.97 | 368.26 | 15.60 | 279.07 | -72.10 | 75.33 | 0.9475 | -116.2 | -3.9 | |
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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 | 0.87 | 0.00 | 0.91 | 15.54 | 289.05 | -62.13 | 75.27 | 0.8825 | -419.0 | -388.7 | |
| 0.00 | 0.44 | 0.00 | 0.50 | 12.66 | 286.11 | -65.06 | 78.56 | 0.9045 | -383.0 | -345.4 | |
| 9.23 | 173.69 | 12.82 | 251.44 | 15.78 | 281.34 | -69.83 | 75.17 | 0.9360 | -673.9 | -28.9 | |
| 0.00 | 2.44 | 0.00 | 3.51 | 16.73 | 280.56 | -70.61 | 74.16 | 0.9405 | -160.0 | -83.4 | |
| 3.66 | -3.00 | 5.24 | -3.00 | 16.18 | 280.65 | -70.53 | 74.74 | 0.9400 | -249.0 | 999999 | |
| 2.44 | -3.00 | 3.48 | -3.00 | 15.64 | 280.81 | -70.37 | 75.32 | 0.9391 | -380.5 | 999999 | |
| 3.22 | -3.00 | 4.62 | -3.00 | 15.29 | 280.70 | -70.47 | 75.69 | 0.9397 | -418.3 | 999999 | |
| 8.53 | -3.00 | 12.36 | -3.00 | 14.87 | 280.47 | -70.71 | 76.14 | 0.9411 | -465.3 | 999999 | |
| 7.75 | 25.60 | 12.37 | 40.76 | 17.07 | 278.43 | -72.74 | 73.80 | 0.9520 | 509.4 | 415.5 | |
| 2.96 | -3.00 | 4.36 | -3.00 | 14.96 | 280.11 | -71.07 | 76.04 | 0.9431 | 162.6 | 999999 | |
| 0.00 | 1.48 | 0.00 | 3.05 | 15.69 | 274.12 | -77.05 | 75.16 | 0.9717 | 460.0 | 362.2 | |
| 0.00 | 2.09 | 0.00 | 4.32 | 15.43 | 274.01 | -77.16 | 75.42 | 0.9722 | 371.0 | 292.2 | |
| 6.18 | 27.86 | 13.72 | 63.77 | 15.35 | 273.09 | -78.09 | 75.47 | 0.9757 | 253.5 | -169.7 | |
| 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. | |