SDO HMI 2014-11-16 20:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.33 | 33.77 | 9.92 | 37.75 | -12.42 | 224.79 | -62.27 | 105.30 | 0.8973 | -123.7 | 50.0 | |
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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 | 1.89 | 0.00 | 1.88 | -13.41 | 228.54 | -58.52 | 107.11 | 0.8700 | 340.0 | 294.4 | |
| 0.77 | 2.32 | 0.77 | 2.31 | -12.83 | 228.53 | -58.53 | 106.45 | 0.8691 | 515.6 | 450.8 | |
| 0.00 | 1.55 | 0.00 | 1.60 | -13.73 | 227.45 | -59.61 | 107.24 | 0.8793 | 471.0 | 277.1 | |
| 0.00 | 0.69 | 0.00 | 0.68 | -11.40 | 228.28 | -58.78 | 104.78 | 0.8690 | 396.0 | 369.8 | |
| 0.00 | 1.12 | 0.00 | 1.13 | -11.12 | 227.72 | -59.34 | 104.35 | 0.8733 | 500.0 | 376.4 | |
| 0.00 | 1.80 | 0.00 | 1.90 | -12.91 | 226.57 | -60.50 | 106.14 | 0.8851 | -160.0 | -134.4 | |
| 0.00 | 0.26 | 0.00 | 0.28 | -13.73 | 226.02 | -61.04 | 106.95 | 0.8904 | -223.0 | -344.7 | |
| 0.00 | 1.12 | 0.00 | 1.20 | -13.39 | 226.11 | -60.95 | 106.59 | 0.8893 | -468.0 | -467.7 | |
| 0.00 | 0.94 | 0.00 | 0.99 | -11.89 | 226.72 | -60.34 | 105.04 | 0.8825 | 327.0 | 306.6 | |
| 0.00 | 4.64 | 0.00 | 4.82 | -11.37 | 226.85 | -60.21 | 104.47 | 0.8807 | 509.0 | 336.7 | |
| 0.00 | 2.41 | 0.00 | 2.77 | -12.41 | 223.85 | -63.21 | 105.10 | 0.9048 | -284.0 | -279.2 | |
| 6.53 | 11.25 | 7.91 | 13.67 | -12.56 | 222.53 | -64.53 | 105.04 | 0.9142 | -459.8 | -7.3 | |
| 1.03 | 3.78 | 1.24 | 4.52 | -12.12 | 222.73 | -64.33 | 104.60 | 0.9124 | -509.4 | -356.8 | |
| 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. | |