SDO HMI 2011-09-05 11:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.89 | 102.64 | 17.59 | 67.04 | -19.52 | 258.57 | 31.31 | 228.52 | 0.6559 | 391.1 | 343.6 | |
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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 | 1.25 | 0.00 | 0.87 | -21.90 | 261.91 | 34.64 | 228.54 | 0.7061 | 584.0 | 440.1 | |
| 0.00 | 1.16 | 0.00 | 0.81 | -22.10 | 261.80 | 34.54 | 228.23 | 0.7067 | 592.0 | 486.9 | |
| 0.00 | 0.71 | 0.00 | 0.49 | -21.29 | 260.72 | 33.46 | 228.28 | 0.6906 | 663.0 | 545.5 | |
| 0.00 | 0.71 | 0.00 | 0.47 | -18.87 | 259.00 | 31.74 | 229.70 | 0.6549 | 703.0 | 516.2 | |
| 1.61 | 5.00 | 1.06 | 3.31 | -19.96 | 259.21 | 31.94 | 228.56 | 0.6656 | 483.1 | 157.7 | |
| 15.54 | 74.51 | 10.21 | 48.74 | -19.50 | 258.91 | 31.65 | 228.86 | 0.6591 | 919.4 | 513.8 | |
| 5.09 | -6.00 | 3.34 | -6.00 | -19.74 | 258.44 | 31.17 | 228.15 | 0.6563 | 775.8 | 999999 | |
| 3.04 | 6.79 | 1.96 | 4.38 | -18.50 | 257.99 | 30.73 | 229.26 | 0.6418 | -534.1 | 166.6 | |
| 0.00 | 0.80 | 0.00 | 0.54 | -22.70 | 258.26 | 31.00 | 224.57 | 0.6793 | 646.0 | 581.9 | |
| 0.00 | 4.38 | 0.00 | 2.81 | -18.92 | 257.30 | 30.03 | 228.11 | 0.6383 | -619.0 | -570.1 | |
| 1.61 | 1.97 | 1.02 | 1.24 | -18.38 | 256.24 | 28.97 | 227.77 | 0.6231 | -743.2 | -543.0 | |
| 0.00 | 1.25 | 0.00 | 0.80 | -19.35 | 256.20 | 28.94 | 226.54 | 0.6312 | -452.0 | -422.4 | |
| 0.00 | 0.98 | 0.00 | 0.62 | -19.51 | 255.58 | 28.31 | 225.73 | 0.6266 | -619.0 | -504.3 | |
| 0.00 | 1.61 | 0.00 | 1.02 | -19.50 | 255.36 | 28.09 | 225.53 | 0.6243 | -772.0 | -612.6 | |
| 0.00 | 1.52 | 0.00 | 0.94 | -17.63 | 254.91 | 27.65 | 227.40 | 0.6031 | -621.0 | -474.3 | |
| 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. | |