SDO HMI 2011-11-25 15:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.20 | 67.17 | 16.87 | 37.50 | 17.95 | 214.10 | -22.42 | 51.98 | 0.4626 | 371.4 | 295.8 | |
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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 | 1.11 | 0.00 | 0.63 | 22.55 | 216.77 | -19.75 | 41.02 | 0.4776 | 582.0 | 408.3 | |
| 0.00 | 2.14 | 0.00 | 1.18 | 18.91 | 217.06 | -19.46 | 46.52 | 0.4362 | 831.0 | 648.9 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 20.02 | 215.75 | -20.78 | 46.39 | 0.4622 | 635.0 | 522.2 | |
| 0.00 | 3.77 | 0.00 | 2.10 | 19.33 | 215.51 | -21.02 | 47.87 | 0.4583 | 864.0 | 689.5 | |
| 7.27 | 12.07 | 4.00 | 6.64 | 17.24 | 215.74 | -20.79 | 51.36 | 0.4358 | -967.6 | -656.3 | |
| 1.88 | -5.00 | 1.04 | -5.00 | 17.26 | 215.47 | -21.06 | 51.64 | 0.4394 | -847.0 | 999999 | |
| 0.00 | 1.20 | 0.00 | 0.66 | 17.11 | 215.09 | -21.44 | 52.41 | 0.4427 | -565.0 | -481.1 | |
| 2.05 | 9.58 | 1.14 | 5.32 | 17.90 | 214.86 | -21.67 | 51.21 | 0.4527 | -793.8 | -672.5 | |
| 0.00 | 1.71 | 0.00 | 0.96 | 17.98 | 213.53 | -22.99 | 52.61 | 0.4695 | 871.0 | 729.0 | |
| 0.00 | 1.28 | 0.00 | 0.72 | 17.80 | 213.53 | -23.00 | 52.95 | 0.4681 | 670.0 | 549.5 | |
| 0.00 | 0.51 | 0.00 | 0.29 | 16.81 | 213.19 | -23.34 | 55.13 | 0.4642 | 630.0 | 450.5 | |
| 19.00 | 33.03 | 10.69 | 18.57 | 17.85 | 212.87 | -23.65 | 53.57 | 0.4766 | 970.4 | 807.9 | |
| 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. | |