SDO HMI 2014-11-03 00:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.00 | 0.00 | 8.78 | -19.62 | 79.84 | -29.60 | 130.61 | 0.6123 | 518.7 | 455.0 | |
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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 | 1.30 | 0.00 | 0.75 | -17.23 | 87.20 | -22.23 | 134.92 | 0.5124 | -662.0 | -451.5 | |
| 0.00 | 1.38 | 0.00 | 0.83 | -20.89 | 84.83 | -24.61 | 137.06 | 0.5732 | 718.0 | 636.9 | |
| 0.00 | 1.21 | 0.00 | 0.71 | -17.66 | 84.56 | -24.88 | 132.40 | 0.5450 | 742.0 | 510.4 | |
| 0.00 | 0.61 | 0.00 | 0.35 | -16.67 | 84.49 | -24.94 | 130.90 | 0.5366 | 448.0 | 425.4 | |
| 0.00 | 1.04 | 0.00 | 0.64 | -20.77 | 81.47 | -27.96 | 133.38 | 0.6055 | 530.0 | 493.1 | |
| 0.00 | 0.95 | 0.00 | 0.60 | -20.00 | 79.46 | -29.98 | 130.48 | 0.6197 | 634.0 | 512.9 | |
| 0.00 | 1.12 | 0.00 | 0.72 | -20.43 | 78.36 | -31.07 | 130.09 | 0.6344 | 716.0 | 625.2 | |
| 0.00 | 0.86 | 0.00 | 0.56 | -20.07 | 76.88 | -32.56 | 128.38 | 0.6471 | 526.0 | 506.5 | |
| 0.00 | 2.68 | 0.00 | 1.75 | -20.37 | 76.66 | -32.78 | 128.59 | 0.6516 | 671.0 | 523.8 | |
| 0.00 | 1.21 | 0.00 | 0.79 | -19.74 | 76.05 | -33.39 | 127.30 | 0.6534 | 627.0 | 573.9 | |
| 0.00 | 0.78 | 0.00 | 0.51 | -19.45 | 76.12 | -33.32 | 126.97 | 0.6506 | 606.0 | 490.2 | |
| 0.00 | 0.86 | 0.00 | 0.57 | -19.75 | 75.78 | -33.65 | 127.11 | 0.6563 | 668.0 | 551.2 | |
| 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. | |