SDO HMI 2014-12-10 03:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.14 | 0.00 | 8.99 | 15.83 | 15.38 | 35.30 | 297.19 | 0.6267 | -244.4 | -265.5 | |
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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 | 0.51 | 0.00 | 0.35 | 9.15 | 22.76 | 42.69 | 283.63 | 0.6911 | -549.0 | -521.0 | |
| 0.00 | 1.19 | 0.00 | 0.79 | 12.79 | 20.17 | 40.10 | 289.69 | 0.6695 | -586.0 | -532.7 | |
| 0.00 | 1.88 | 0.00 | 1.25 | 16.77 | 19.26 | 39.19 | 295.75 | 0.6741 | -664.0 | -514.1 | |
| 0.00 | 0.77 | 0.00 | 0.49 | 11.70 | 18.03 | 37.95 | 288.90 | 0.6389 | -609.0 | -474.9 | |
| 0.00 | 0.85 | 0.00 | 0.54 | 11.63 | 17.67 | 37.60 | 288.95 | 0.6341 | -689.0 | -600.8 | |
| 0.00 | 0.85 | 0.00 | 0.56 | 15.29 | 18.01 | 37.94 | 294.24 | 0.6527 | -397.0 | -426.1 | |
| 0.00 | 1.02 | 0.00 | 0.66 | 14.95 | 17.82 | 37.75 | 293.84 | 0.6490 | -742.0 | -672.1 | |
| 0.00 | 1.53 | 0.00 | 1.00 | 15.68 | 17.98 | 37.91 | 294.84 | 0.6541 | -635.0 | -542.8 | |
| 0.00 | 1.11 | 0.00 | 0.72 | 15.71 | 17.29 | 37.22 | 295.23 | 0.6459 | -572.0 | -516.6 | |
| 0.00 | 0.77 | 0.00 | 0.49 | 15.62 | 16.92 | 36.85 | 295.28 | 0.6410 | -685.0 | -574.3 | |
| 0.00 | 1.28 | 0.00 | 0.76 | 20.27 | 6.69 | 26.61 | 309.80 | 0.5492 | 681.0 | 578.3 | |
| 0.00 | 0.34 | 0.00 | 0.20 | 20.46 | 6.55 | 26.47 | 310.22 | 0.5492 | 571.0 | 659.5 | |
| 0.00 | 1.02 | 0.00 | 0.59 | 19.92 | 4.33 | 24.25 | 311.73 | 0.5196 | 629.0 | 506.3 | |
| 0.00 | 1.02 | 0.00 | 0.59 | 19.85 | 4.01 | 23.93 | 311.99 | 0.5155 | 825.0 | 728.4 | |
| 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. | |