SDO HMI 2014-09-16 03:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.44 | 0.00 | 8.56 | 8.19 | 341.79 | -39.26 | 85.90 | 0.6295 | -563.8 | -500.3 | |
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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 | 1.07 | 0.00 | 0.65 | 7.72 | 345.23 | -35.83 | 86.79 | 0.5832 | -646.0 | -488.9 | |
| 0.00 | 0.36 | 0.00 | 0.22 | 9.84 | 344.92 | -36.14 | 83.14 | 0.5875 | 353.0 | 279.0 | |
| 0.00 | 1.16 | 0.00 | 0.71 | 7.84 | 344.87 | -36.18 | 86.56 | 0.5881 | -697.0 | -548.2 | |
| 0.00 | 0.71 | 0.00 | 0.44 | 8.22 | 344.23 | -36.83 | 85.90 | 0.5970 | -703.0 | -606.4 | |
| 0.00 | 0.98 | 0.00 | 0.60 | 7.76 | 344.09 | -36.97 | 86.67 | 0.5991 | -656.0 | -520.5 | |
| 0.00 | 0.98 | 0.00 | 0.61 | 7.57 | 343.22 | -37.83 | 86.94 | 0.6111 | -726.0 | -611.4 | |
| 0.00 | 1.33 | 0.00 | 0.84 | 7.42 | 342.89 | -38.17 | 87.16 | 0.6158 | -617.0 | -557.4 | |
| 0.00 | 1.07 | 0.00 | 0.67 | 7.57 | 342.80 | -38.26 | 86.92 | 0.6170 | -756.0 | -596.4 | |
| 0.00 | 0.89 | 0.00 | 0.56 | 7.68 | 342.63 | -38.43 | 86.73 | 0.6192 | -619.0 | -520.3 | |
| 0.00 | 0.98 | 0.00 | 0.62 | 8.02 | 342.01 | -39.05 | 86.15 | 0.6275 | -656.0 | -577.8 | |
| 0.00 | 0.71 | 0.00 | 0.47 | 9.35 | 339.30 | -41.75 | 84.01 | 0.6630 | -599.0 | -497.4 | |
| 0.00 | 1.33 | 0.00 | 0.88 | 9.19 | 339.16 | -41.89 | 84.26 | 0.6648 | -597.0 | -463.6 | |
| 0.00 | 1.87 | 0.00 | 1.29 | 8.85 | 336.26 | -44.79 | 84.68 | 0.7015 | -410.0 | -406.5 | |
| 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. | |