SDO HMI 2014-11-15 15:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.99 | 63.19 | 26.70 | 105.58 | 13.86 | 15.83 | 72.82 | 283.65 | 0.9556 | -348.2 | -21.0 | |
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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 | 1.46 | 0.00 | 2.72 | 13.04 | 17.78 | 74.77 | 282.76 | 0.9650 | 310.0 | 308.7 | |
| 1.03 | 14.44 | 1.83 | 25.98 | 13.23 | 17.02 | 74.01 | 282.96 | 0.9615 | -281.8 | -54.8 | |
| 1.38 | -2.00 | 2.46 | -2.00 | 13.40 | 17.17 | 74.16 | 283.14 | 0.9622 | -292.3 | 999999 | |
| 0.00 | 0.26 | 0.00 | 0.42 | 12.48 | 15.37 | 72.37 | 282.21 | 0.9534 | -285.0 | -327.3 | |
| 3.52 | 8.77 | 5.76 | 14.26 | 13.39 | 15.53 | 72.52 | 283.16 | 0.9543 | -441.5 | -415.3 | |
| 10.06 | 33.01 | 16.65 | 55.09 | 14.20 | 15.77 | 72.76 | 284.01 | 0.9556 | -447.7 | 57.8 | |
| 0.00 | 0.52 | 0.00 | 0.81 | 14.12 | 14.78 | 71.78 | 283.96 | 0.9506 | -324.0 | -322.5 | |
| 0.00 | 0.26 | 0.00 | 0.39 | 14.82 | 14.25 | 71.25 | 284.71 | 0.9479 | -346.0 | -315.0 | |
| 0.00 | 0.52 | 0.00 | 0.78 | 15.23 | 14.00 | 71.00 | 285.15 | 0.9466 | -424.0 | -373.7 | |
| 0.00 | 1.03 | 0.00 | 1.35 | 14.16 | 10.69 | 67.68 | 284.16 | 0.9267 | 240.0 | 196.6 | |
| 0.00 | 2.15 | 0.00 | 2.75 | 13.97 | 10.17 | 67.16 | 283.98 | 0.9233 | 367.0 | 340.3 | |
| 0.00 | 0.77 | 0.00 | 1.03 | 15.73 | 11.16 | 68.15 | 285.83 | 0.9302 | -390.0 | -376.4 | |
| 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. | |