SDO HMI 2014-12-09 12:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.85 | 340.65 | 30.47 | 173.49 | -3.86 | 1.27 | 12.93 | 253.95 | 0.2334 | 1103.7 | 395.1 | |
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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 | 1.70 | 0.00 | 0.88 | -4.94 | 4.93 | 16.59 | 253.72 | 0.2977 | 867.0 | 713.2 | |
| 0.00 | 1.45 | 0.00 | 0.75 | -5.20 | 4.84 | 16.50 | 252.77 | 0.2975 | 871.0 | 723.8 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -5.38 | 4.57 | 16.23 | 251.93 | 0.2940 | 825.0 | 669.2 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -5.77 | 4.18 | 15.84 | 250.25 | 0.2899 | 802.0 | 670.2 | |
| 0.94 | 316.61 | 0.48 | 161.23 | -3.78 | 1.81 | 13.47 | 254.85 | 0.2419 | 855.5 | 402.8 | |
| 32.74 | -5.00 | 16.69 | -5.00 | -3.99 | 1.48 | 13.14 | 253.65 | 0.2374 | 1364.3 | 999999 | |
| 0.85 | 11.42 | 0.43 | 5.81 | -2.42 | 1.19 | 12.85 | 259.99 | 0.2266 | 847.0 | 569.4 | |
| 7.50 | -5.00 | 3.82 | -5.00 | -4.11 | 1.15 | 12.81 | 252.77 | 0.2326 | 1386.9 | 999999 | |
| 0.00 | 2.05 | 0.00 | 1.04 | -1.95 | 1.06 | 12.72 | 261.99 | 0.2233 | 644.0 | 467.7 | |
| 17.82 | -5.00 | 9.05 | -5.00 | -3.60 | 0.78 | 12.44 | 254.45 | 0.2241 | 1431.5 | 999999 | |
| 0.00 | 2.30 | 0.00 | 1.17 | -1.56 | 0.73 | 12.39 | 263.54 | 0.2168 | -976.0 | -814.1 | |
| 0.00 | 1.88 | 0.00 | 0.95 | -7.19 | 358.06 | 9.72 | 233.91 | 0.2082 | -964.0 | -614.5 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -7.31 | 357.85 | 9.51 | 232.85 | 0.2065 | -904.0 | -796.8 | |
| 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. | |