SDO HMI 2014-11-15 03:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 11.37 | 0.00 | 6.71 | -9.50 | 339.76 | 30.19 | 246.48 | 0.5405 | -375.1 | -324.9 | |
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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 | 0.26 | 0.00 | 0.18 | -5.88 | 352.07 | 42.50 | 258.32 | 0.6886 | -452.0 | -354.7 | |
| 0.00 | 1.38 | 0.00 | 0.91 | -8.58 | 349.26 | 39.69 | 253.50 | 0.6609 | -546.0 | -459.4 | |
| 0.00 | 0.52 | 0.00 | 0.33 | -8.36 | 347.99 | 38.42 | 253.35 | 0.6441 | 359.0 | 319.2 | |
| 0.00 | 1.20 | 0.00 | 0.75 | -5.60 | 345.48 | 35.91 | 256.72 | 0.6020 | 496.0 | 427.9 | |
| 0.00 | 0.95 | 0.00 | 0.57 | -10.69 | 340.91 | 31.34 | 246.03 | 0.5615 | 356.0 | 307.5 | |
| 0.00 | 0.60 | 0.00 | 0.34 | -11.42 | 335.77 | 26.20 | 240.83 | 0.4977 | -458.0 | -509.0 | |
| 0.00 | 0.86 | 0.00 | 0.49 | -11.29 | 335.62 | 26.05 | 240.92 | 0.4948 | -822.0 | -720.5 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -9.09 | 335.40 | 25.83 | 244.82 | 0.4773 | -686.0 | -612.2 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -13.04 | 335.67 | 26.10 | 237.89 | 0.5081 | -639.0 | -553.7 | |
| 0.00 | 1.38 | 0.00 | 0.77 | -8.57 | 334.93 | 25.36 | 245.45 | 0.4675 | -720.0 | -523.4 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -10.97 | 334.82 | 25.25 | 240.77 | 0.4819 | -607.0 | -428.9 | |
| 0.00 | 1.29 | 0.00 | 0.72 | -10.37 | 334.14 | 24.57 | 241.24 | 0.4684 | -782.0 | -674.3 | |
| 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. | |