SDO HMI 2014-03-06 01:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.03 | 70.99 | 15.08 | 38.20 | -16.83 | 44.84 | -21.30 | 116.78 | 0.3908 | -58.0 | -14.5 | |
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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 |
| 1.04 | 19.11 | 0.55 | 10.13 | -17.19 | 47.34 | -18.81 | 120.15 | 0.3577 | 864.8 | 732.5 | |
| 3.89 | -1.00 | 2.06 | -1.00 | -16.91 | 47.24 | -18.91 | 119.33 | 0.3572 | 1119.2 | 999999 | |
| 2.08 | -1.00 | 1.10 | -1.00 | -17.06 | 47.19 | -18.96 | 119.65 | 0.3589 | 981.5 | 999999 | |
| 2.25 | 4.32 | 1.19 | 2.29 | -16.38 | 46.77 | -19.38 | 117.45 | 0.3603 | 1079.8 | 827.6 | |
| 0.52 | 1.73 | 0.28 | 0.92 | -16.52 | 46.52 | -19.62 | 117.55 | 0.3647 | 914.0 | 773.7 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -17.06 | 46.33 | -19.81 | 118.68 | 0.3710 | 737.0 | 608.4 | |
| 4.06 | 7.35 | 2.17 | 3.92 | -16.13 | 45.94 | -20.21 | 115.98 | 0.3707 | 940.0 | 614.4 | |
| 0.35 | 1.73 | 0.19 | 0.93 | -17.40 | 45.19 | -20.95 | 118.34 | 0.3893 | 786.2 | 573.9 | |
| 0.00 | 1.64 | 0.00 | 0.89 | -16.32 | 44.06 | -22.09 | 114.75 | 0.3991 | -941.0 | -799.1 | |
| 1.82 | 4.93 | 0.98 | 2.67 | -15.91 | 43.64 | -22.51 | 113.44 | 0.4030 | -1121.0 | -785.2 | |
| 0.00 | 1.30 | 0.00 | 0.70 | -16.21 | 43.57 | -22.58 | 114.08 | 0.4056 | -689.0 | -462.7 | |
| 0.00 | 2.08 | 0.00 | 1.13 | -17.68 | 42.83 | -23.31 | 116.83 | 0.4243 | -557.0 | -522.6 | |
| 12.02 | 22.91 | 6.56 | 12.50 | -17.20 | 42.83 | -23.31 | 115.76 | 0.4216 | -960.0 | -721.2 | |
| 0.00 | 1.30 | 0.00 | 0.71 | -16.51 | 42.45 | -23.70 | 113.93 | 0.4233 | -868.0 | -716.2 | |
| 0.00 | 1.38 | 0.00 | 0.76 | -16.33 | 42.34 | -23.81 | 113.43 | 0.4240 | -916.0 | -795.5 | |
| 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. | |