SDO HMI 2014-11-02 07:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.11 | 24.49 | 2.81 | 14.03 | -17.35 | 97.96 | -20.82 | 137.73 | 0.4998 | -329.7 | -94.2 | |
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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 |
| 1.39 | 12.64 | 0.76 | 6.95 | -16.14 | 102.84 | -15.94 | 142.66 | 0.4369 | 1130.5 | 823.3 | |
| 3.72 | -1.00 | 2.05 | -1.00 | -16.27 | 102.77 | -16.02 | 142.72 | 0.4392 | 931.3 | 999999 | |
| 0.00 | 0.78 | 0.00 | 0.45 | -17.14 | 94.89 | -23.89 | 132.83 | 0.5299 | -653.0 | -490.7 | |
| 0.00 | 1.64 | 0.00 | 0.97 | -17.77 | 94.19 | -24.60 | 132.93 | 0.5435 | -672.0 | -673.7 | |
| 0.00 | 1.21 | 0.00 | 0.72 | -18.78 | 93.93 | -24.86 | 134.03 | 0.5558 | -875.0 | -727.1 | |
| 0.00 | 1.04 | 0.00 | 0.61 | -17.58 | 94.11 | -24.67 | 132.57 | 0.5425 | -860.0 | -719.1 | |
| 0.00 | 1.21 | 0.00 | 0.72 | -17.71 | 93.92 | -24.87 | 132.55 | 0.5459 | -713.0 | -644.2 | |
| 0.00 | 1.47 | 0.00 | 0.88 | -18.75 | 93.69 | -25.10 | 133.74 | 0.5580 | -806.0 | -672.3 | |
| 0.00 | 0.78 | 0.00 | 0.46 | -17.64 | 93.34 | -25.44 | 131.80 | 0.5514 | -570.0 | -477.2 | |
| 0.00 | 2.68 | 0.00 | 1.63 | -19.40 | 91.82 | -26.96 | 132.63 | 0.5835 | -791.0 | -607.3 | |
| 0.00 | 1.04 | 0.00 | 0.64 | -19.49 | 91.06 | -27.73 | 131.98 | 0.5923 | -722.0 | -574.3 | |
| 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. | |