SDO HMI 2014-09-07 16:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.13 | 88.31 | 39.62 | 140.19 | -16.52 | 64.32 | -68.44 | 110.14 | 0.9503 | 174.4 | -18.2 | |
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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 |
| 6.15 | 62.97 | 8.90 | 92.57 | -16.73 | 66.22 | -66.54 | 110.80 | 0.9412 | 585.7 | 56.8 | |
| 4.73 | -1.00 | 6.97 | -1.00 | -16.68 | 65.86 | -66.90 | 110.65 | 0.9431 | 226.2 | 999999 | |
| 1.61 | -1.00 | 2.40 | -1.00 | -17.07 | 65.57 | -67.19 | 110.98 | 0.9452 | -339.3 | 999999 | |
| 9.36 | -1.00 | 13.72 | -1.00 | -16.42 | 65.88 | -66.88 | 110.39 | 0.9426 | 453.7 | 999999 | |
| 1.34 | -1.00 | 2.02 | -1.00 | -16.94 | 65.34 | -67.42 | 110.79 | 0.9462 | -439.7 | 999999 | |
| 0.00 | 2.59 | 0.00 | 4.15 | -17.05 | 64.14 | -68.61 | 110.61 | 0.9524 | 155.0 | 90.3 | |
| 0.00 | 1.34 | 0.00 | 2.14 | -16.11 | 63.91 | -68.85 | 109.59 | 0.9524 | 142.0 | 83.7 | |
| 0.00 | 0.89 | 0.00 | 1.50 | -16.66 | 63.11 | -69.64 | 109.97 | 0.9569 | -106.0 | -44.0 | |
| 0.00 | 2.68 | 0.00 | 5.15 | -16.53 | 60.69 | -72.07 | 109.30 | 0.9676 | -476.0 | -402.6 | |
| 0.00 | 1.25 | 0.00 | 2.45 | -16.79 | 60.44 | -72.32 | 109.51 | 0.9688 | -163.0 | -189.0 | |
| 2.94 | 16.59 | 5.61 | 32.23 | -16.14 | 60.74 | -72.02 | 108.92 | 0.9670 | -548.9 | -116.8 | |
| 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. | |