SDO HMI 2014-11-14 08:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.70 | 0.00 | 9.02 | -9.41 | 339.17 | 19.15 | 235.90 | 0.3932 | -97.6 | -77.3 | |
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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 | 1.72 | 0.00 | 0.96 | -5.45 | 346.10 | 26.08 | 252.18 | 0.4616 | 641.0 | 527.5 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -5.24 | 346.09 | 26.07 | 252.61 | 0.4605 | 740.0 | 624.0 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -7.61 | 343.19 | 23.17 | 245.35 | 0.4308 | 775.0 | 693.1 | |
| 0.00 | 1.38 | 0.00 | 0.76 | -8.09 | 343.12 | 23.10 | 244.26 | 0.4330 | 690.0 | 567.2 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -10.07 | 342.20 | 22.18 | 239.23 | 0.4345 | 775.0 | 624.4 | |
| 0.00 | 1.38 | 0.00 | 0.75 | -10.62 | 341.01 | 20.99 | 236.71 | 0.4230 | 730.0 | 588.5 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -10.11 | 337.78 | 17.76 | 233.36 | 0.3758 | -752.0 | -570.3 | |
| 0.00 | 1.38 | 0.00 | 0.74 | -12.93 | 336.40 | 16.38 | 225.36 | 0.3880 | -769.0 | -615.8 | |
| 0.00 | 2.15 | 0.00 | 1.15 | -12.77 | 336.14 | 16.12 | 225.20 | 0.3832 | -830.0 | -628.0 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -9.27 | 335.04 | 15.02 | 230.64 | 0.3323 | -664.0 | -522.2 | |
| 0.00 | 1.20 | 0.00 | 0.64 | -10.91 | 334.87 | 14.84 | 226.62 | 0.3477 | -820.0 | -680.6 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -8.60 | 334.61 | 14.59 | 231.46 | 0.3198 | -728.0 | -610.7 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -10.79 | 334.61 | 14.59 | 226.39 | 0.3432 | -879.0 | -683.4 | |
| 0.00 | 0.52 | 0.00 | 0.26 | -5.76 | 331.98 | 11.95 | 233.92 | 0.2562 | -276.0 | -460.3 | |
| 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. | |