SDO HMI 2014-11-19 02:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.74 | 0.00 | 7.15 | 17.22 | 260.09 | 2.71 | 351.25 | 0.2979 | 562.7 | 427.4 | |
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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 | 0.86 | 0.00 | 0.48 | 12.83 | 283.15 | 25.76 | 293.61 | 0.4644 | 779.0 | 695.4 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 13.73 | 280.04 | 22.65 | 298.10 | 0.4259 | 545.0 | 635.6 | |
| 0.00 | 1.55 | 0.00 | 0.79 | 14.65 | 262.46 | 5.07 | 338.09 | 0.2301 | 943.0 | 785.9 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 14.35 | 262.45 | 5.06 | 337.60 | 0.2252 | 911.0 | 715.3 | |
| 0.00 | 2.06 | 0.00 | 1.05 | 16.73 | 260.03 | 2.64 | 349.89 | 0.2527 | 1022.0 | 729.1 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 16.49 | 259.93 | 2.55 | 350.08 | 0.2484 | 812.0 | 626.2 | |
| 0.00 | 1.97 | 0.00 | 1.05 | 23.20 | 258.96 | 1.57 | 355.95 | 0.3577 | -733.0 | -634.4 | |
| 0.00 | 1.03 | 0.00 | 0.52 | 15.79 | 257.37 | -0.02 | 0.08 | 0.2328 | -831.0 | -569.3 | |
| 0.00 | 1.55 | 0.00 | 0.79 | 16.49 | 256.29 | -1.10 | 4.32 | 0.2454 | 980.0 | 760.3 | |
| 0.00 | 0.60 | 0.00 | 0.32 | 22.94 | 248.85 | -8.54 | 21.26 | 0.3787 | 775.0 | 633.6 | |
| 0.00 | 1.55 | 0.00 | 0.81 | 18.15 | 246.17 | -11.22 | 34.18 | 0.3306 | 987.0 | 754.7 | |
| 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. | |