SDO HMI 2014-09-26 09:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.89 | 105.71 | 43.50 | 196.60 | 12.27 | 170.04 | -75.73 | 79.11 | 0.9650 | -37.7 | -17.0 | |
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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 |
| 2.47 | 15.29 | 4.05 | 25.00 | 12.55 | 172.42 | -73.36 | 78.98 | 0.9541 | -588.7 | -334.3 | |
| 0.00 | 1.77 | 0.00 | 2.98 | 12.11 | 171.85 | -73.92 | 79.40 | 0.9571 | -408.0 | -350.3 | |
| 9.55 | 36.77 | 16.17 | 61.94 | 11.74 | 171.79 | -73.98 | 79.79 | 0.9575 | -450.6 | -284.9 | |
| 0.88 | 8.13 | 1.60 | 14.61 | 12.09 | 170.58 | -75.19 | 79.34 | 0.9632 | 198.2 | 94.9 | |
| 0.00 | 1.24 | 0.00 | 2.34 | 12.17 | 169.89 | -75.89 | 79.22 | 0.9662 | -146.0 | -67.6 | |
| 0.00 | 1.68 | 0.00 | 3.05 | 11.32 | 170.58 | -75.20 | 80.14 | 0.9634 | -90.0 | -46.8 | |
| 0.00 | 1.77 | 0.00 | 3.25 | 11.48 | 170.33 | -75.44 | 79.96 | 0.9645 | 161.0 | 97.5 | |
| 0.00 | 1.59 | 0.00 | 3.06 | 11.37 | 169.65 | -76.12 | 80.03 | 0.9675 | 430.0 | 365.7 | |
| 0.00 | 1.50 | 0.00 | 3.38 | 13.45 | 167.32 | -78.45 | 77.72 | 0.9762 | 422.0 | 384.1 | |
| 9.99 | 31.55 | 21.68 | 67.49 | 12.78 | 167.76 | -78.01 | 78.43 | 0.9748 | 300.9 | 265.9 | |
| 0.00 | 2.30 | 0.00 | 4.88 | 12.45 | 168.11 | -77.67 | 78.79 | 0.9735 | 281.0 | 275.5 | |
| 0.00 | 2.12 | 0.00 | 4.62 | 11.96 | 167.86 | -77.91 | 79.28 | 0.9746 | 239.0 | 279.6 | |
| 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. | |