SDO HMI 2014-11-03 05:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.59 | 0.00 | 12.80 | -20.41 | 78.44 | -28.25 | 132.75 | 0.6056 | 571.3 | 558.2 | |
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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 | 2.42 | 0.00 | 1.43 | -20.98 | 85.08 | -21.61 | 140.70 | 0.5451 | 727.0 | 718.5 | |
| 0.00 | 0.43 | 0.00 | 0.25 | -16.53 | 84.71 | -21.98 | 134.16 | 0.5022 | 263.0 | 340.0 | |
| 0.00 | 0.69 | 0.00 | 0.43 | -24.32 | 81.12 | -25.57 | 140.11 | 0.6156 | 408.0 | 395.6 | |
| 0.00 | 1.30 | 0.00 | 0.80 | -21.48 | 80.45 | -26.24 | 135.99 | 0.5944 | 441.0 | 382.9 | |
| 0.00 | 4.76 | 0.00 | 2.95 | -20.56 | 78.55 | -28.14 | 132.90 | 0.6050 | 664.0 | 614.9 | |
| 0.00 | 2.77 | 0.00 | 1.74 | -19.96 | 76.90 | -29.79 | 130.57 | 0.6171 | 667.0 | 511.8 | |
| 0.00 | 0.87 | 0.00 | 0.55 | -20.10 | 76.68 | -30.01 | 130.56 | 0.6205 | 266.0 | 353.7 | |
| 0.00 | 1.30 | 0.00 | 0.82 | -20.33 | 76.60 | -30.09 | 130.78 | 0.6232 | 691.0 | 583.8 | |
| 0.00 | 1.99 | 0.00 | 1.26 | -20.21 | 76.40 | -30.29 | 130.45 | 0.6242 | 728.0 | 618.7 | |
| 0.00 | 1.21 | 0.00 | 0.76 | -19.92 | 76.39 | -30.30 | 130.06 | 0.6220 | 802.0 | 696.3 | |
| 0.00 | 0.95 | 0.00 | 0.60 | -19.80 | 75.98 | -30.71 | 129.54 | 0.6255 | 562.0 | 482.8 | |
| 0.00 | 1.90 | 0.00 | 1.21 | -19.72 | 75.63 | -31.07 | 129.13 | 0.6285 | 637.0 | 478.1 | |
| 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. | |