SDO HMI 2014-01-14 23:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 84.81 | 447.25 | 43.25 | 228.05 | -16.33 | 12.71 | 7.05 | 209.63 | 0.2380 | 1076.2 | 408.5 | |
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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 |
| 43.43 | 259.46 | 22.20 | 132.61 | -16.59 | 13.51 | 7.85 | 211.98 | 0.2484 | 1380.9 | 455.6 | |
| 4.50 | -1.00 | 2.30 | -1.00 | -16.69 | 12.86 | 7.20 | 209.63 | 0.2441 | 1090.8 | 999999 | |
| 0.00 | 1.95 | 0.00 | 0.99 | -15.94 | 12.56 | 6.90 | 210.22 | 0.2306 | 852.0 | 648.7 | |
| 0.00 | 2.04 | 0.00 | 1.04 | -15.76 | 12.52 | 6.86 | 210.50 | 0.2277 | 763.0 | 645.7 | |
| 0.68 | 163.76 | 0.35 | 83.26 | -16.79 | 12.27 | 6.62 | 207.42 | 0.2408 | 661.2 | 410.2 | |
| 0.00 | 9.69 | 0.00 | 4.92 | -15.25 | 12.23 | 6.57 | 210.62 | 0.2177 | 791.0 | 416.4 | |
| 0.00 | 2.12 | 0.00 | 1.08 | -14.72 | 11.87 | 6.22 | 210.58 | 0.2068 | -810.0 | -502.0 | |
| 35.10 | -5.00 | 17.84 | -5.00 | -16.07 | 11.79 | 6.13 | 207.13 | 0.2262 | 1314.6 | 999999 | |
| 1.10 | -5.00 | 0.56 | -5.00 | -15.80 | 11.47 | 5.82 | 206.48 | 0.2197 | 1229.3 | 999999 | |
| 0.00 | 3.48 | 0.00 | 1.76 | -14.42 | 11.34 | 5.69 | 209.16 | 0.1980 | -1019.0 | -771.6 | |
| 0.00 | 0.93 | 0.00 | 0.47 | -16.50 | 8.10 | 2.45 | 191.16 | 0.2125 | -967.0 | -819.5 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -16.90 | 6.01 | 0.36 | 181.59 | 0.2152 | -729.0 | -594.5 | |
| 0.00 | 2.97 | 0.00 | 1.49 | -12.43 | 4.26 | -1.40 | 170.18 | 0.1402 | -848.0 | -705.5 | |
| 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. | |