SDO HMI 2014-11-24 03:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.01 | 0.00 | 9.56 | -12.84 | 227.16 | 36.22 | 246.81 | 0.6287 | 315.8 | 302.9 | |
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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 | 1.20 | 0.00 | 0.78 | -12.62 | 228.73 | 37.79 | 247.95 | 0.6475 | 630.0 | 542.1 | |
| 0.00 | 2.23 | 0.00 | 1.45 | -13.20 | 228.64 | 37.70 | 247.06 | 0.6489 | 463.0 | 371.2 | |
| 0.00 | 1.37 | 0.00 | 0.89 | -12.98 | 228.41 | 37.47 | 247.27 | 0.6451 | 561.0 | 534.0 | |
| 0.00 | 0.26 | 0.00 | 0.17 | -12.70 | 228.36 | 37.42 | 247.65 | 0.6433 | 638.0 | 661.3 | |
| 0.00 | 0.86 | 0.00 | 0.55 | -12.64 | 228.23 | 37.30 | 247.69 | 0.6415 | 659.0 | 627.9 | |
| 0.00 | 1.29 | 0.00 | 0.83 | -12.57 | 228.03 | 37.10 | 247.68 | 0.6387 | 680.0 | 607.0 | |
| 0.00 | 0.94 | 0.00 | 0.61 | -13.76 | 227.82 | 36.89 | 245.82 | 0.6414 | 710.0 | 568.3 | |
| 0.00 | 1.97 | 0.00 | 1.26 | -13.05 | 227.58 | 36.65 | 246.74 | 0.6352 | 774.0 | 658.4 | |
| 0.00 | 1.29 | 0.00 | 0.82 | -12.83 | 227.24 | 36.31 | 246.90 | 0.6299 | 746.0 | 674.1 | |
| 0.00 | 1.11 | 0.00 | 0.68 | -12.96 | 224.22 | 33.29 | 245.01 | 0.5923 | -596.0 | -548.2 | |
| 0.00 | 1.46 | 0.00 | 0.89 | -11.73 | 223.86 | 32.93 | 246.76 | 0.5815 | -648.0 | -499.9 | |
| 0.00 | 1.03 | 0.00 | 0.63 | -12.80 | 223.83 | 32.90 | 245.03 | 0.5865 | -828.0 | -653.8 | |
| 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. | |