SDO HMI 2014-09-16 01:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.24 | 0.00 | 8.37 | 8.02 | 343.35 | -38.81 | 86.15 | 0.6242 | -462.7 | -403.3 | |
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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 | 1.24 | 0.00 | 0.77 | 7.73 | 345.23 | -36.93 | 86.73 | 0.5985 | -588.0 | -491.8 | |
| 0.00 | 0.89 | 0.00 | 0.55 | 10.00 | 344.89 | -37.27 | 82.92 | 0.6031 | 531.0 | 429.8 | |
| 0.00 | 1.60 | 0.00 | 0.99 | 7.82 | 344.87 | -37.28 | 86.55 | 0.6034 | -672.0 | -497.3 | |
| 0.00 | 0.80 | 0.00 | 0.50 | 8.23 | 344.21 | -37.94 | 85.86 | 0.6123 | -681.0 | -587.7 | |
| 0.00 | 0.80 | 0.00 | 0.50 | 7.76 | 344.07 | -38.08 | 86.61 | 0.6145 | -624.0 | -549.3 | |
| 0.00 | 1.24 | 0.00 | 0.79 | 6.40 | 342.88 | -39.28 | 88.72 | 0.6315 | -415.0 | -420.9 | |
| 0.00 | 0.98 | 0.00 | 0.62 | 7.23 | 342.68 | -39.47 | 87.38 | 0.6336 | -525.0 | -424.7 | |
| 0.00 | 1.69 | 0.00 | 1.08 | 7.65 | 342.60 | -39.56 | 86.72 | 0.6345 | -638.0 | -503.5 | |
| 0.00 | 1.51 | 0.00 | 0.97 | 10.13 | 342.20 | -39.96 | 82.80 | 0.6395 | -271.0 | -261.4 | |
| 0.00 | 0.89 | 0.00 | 0.57 | 7.10 | 342.50 | -39.66 | 87.58 | 0.6362 | -574.0 | -449.8 | |
| 0.00 | 1.60 | 0.00 | 1.03 | 8.06 | 341.99 | -40.16 | 86.05 | 0.6424 | -633.0 | -508.2 | |
| 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. | |