SDO HMI 2011-06-06 21:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.10 | 156.16 | 17.31 | 79.51 | 9.56 | 336.42 | -8.99 | 42.57 | 0.2278 | -747.1 | -318.4 | |
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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 | 1.09 | 0.00 | 0.55 | 8.12 | 339.07 | -6.35 | 37.71 | 0.1797 | -905.0 | -713.4 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 11.36 | 337.75 | -7.66 | 33.52 | 0.2377 | -894.0 | -678.5 | |
| 30.58 | 128.73 | 15.52 | 65.37 | 9.38 | 336.96 | -8.45 | 41.60 | 0.2194 | -1339.3 | -389.2 | |
| 0.90 | 4.79 | 0.46 | 2.43 | 8.03 | 336.22 | -9.20 | 48.51 | 0.2122 | -1031.5 | -934.4 | |
| 2.62 | 4.34 | 1.33 | 2.20 | 8.49 | 336.11 | -9.30 | 47.22 | 0.2188 | -978.9 | -825.7 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 8.21 | 336.02 | -9.39 | 48.44 | 0.2167 | -971.0 | -731.5 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 10.46 | 335.65 | -9.76 | 42.51 | 0.2479 | -796.0 | -647.7 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 8.40 | 335.40 | -10.02 | 49.62 | 0.2269 | -865.0 | -720.9 | |
| 0.00 | 1.90 | 0.00 | 0.98 | 10.37 | 333.20 | -12.22 | 49.10 | 0.2766 | 986.0 | 745.9 | |
| 0.00 | 3.53 | 0.00 | 1.82 | 10.25 | 332.92 | -12.50 | 50.08 | 0.2789 | 760.0 | 790.8 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 9.85 | 332.42 | -12.99 | 52.28 | 0.2812 | 836.0 | 662.3 | |
| 0.00 | 2.44 | 0.00 | 1.30 | 14.70 | 329.51 | -15.90 | 46.20 | 0.3687 | 798.0 | 650.6 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 13.70 | 329.06 | -16.35 | 49.07 | 0.3635 | 582.0 | 555.4 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 16.03 | 327.22 | -18.19 | 47.35 | 0.4097 | 713.0 | 530.3 | |
| 0.00 | 0.54 | 0.00 | 0.30 | 17.53 | 326.16 | -19.25 | 46.21 | 0.4373 | 705.0 | 552.2 | |
| 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. | |