SDO HMI 2014-10-13 05:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.96 | 0.00 | 10.18 | 14.98 | 356.73 | -26.92 | 68.75 | 0.4653 | -533.5 | -471.5 | |
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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 | 2.63 | 0.00 | 1.38 | 10.86 | 4.81 | -18.84 | 74.17 | 0.3312 | -652.0 | -604.0 | |
| 0.00 | 1.93 | 0.00 | 1.03 | 14.21 | 2.98 | -20.67 | 66.48 | 0.3749 | -936.0 | -833.0 | |
| 0.00 | 1.23 | 0.00 | 0.66 | 14.41 | 2.76 | -20.89 | 66.16 | 0.3792 | -728.0 | -569.5 | |
| 0.00 | 3.06 | 0.00 | 1.66 | 15.21 | 1.41 | -22.24 | 65.39 | 0.4034 | -984.0 | -757.5 | |
| 0.00 | 1.75 | 0.00 | 0.96 | 14.63 | 359.80 | -23.86 | 67.96 | 0.4240 | -887.0 | -655.2 | |
| 0.00 | 1.58 | 0.00 | 0.86 | 14.71 | 359.51 | -24.14 | 67.97 | 0.4285 | -815.0 | -673.5 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 13.93 | 359.57 | -24.08 | 69.71 | 0.4240 | -728.0 | -632.7 | |
| 0.00 | 1.23 | 0.00 | 0.70 | 15.71 | 354.59 | -29.06 | 68.84 | 0.5035 | -722.0 | -548.0 | |
| 0.00 | 1.40 | 0.00 | 0.94 | 22.04 | 342.59 | -41.06 | 63.77 | 0.6811 | 226.0 | 279.1 | |
| 0.00 | 0.96 | 0.00 | 0.67 | 21.25 | 340.65 | -43.00 | 65.55 | 0.7006 | 726.0 | 572.5 | |
| 0.00 | 1.23 | 0.00 | 0.79 | 10.24 | 343.25 | -40.40 | 81.24 | 0.6476 | -368.0 | -250.4 | |
| 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. | |