SDO HMI 2014-01-09 13:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.80 | 0.00 | 9.43 | -18.77 | 67.41 | -9.61 | 156.57 | 0.3205 | -198.4 | -216.4 | |
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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 | 1.27 | 0.00 | 0.64 | -13.69 | 80.28 | 3.27 | 198.15 | 0.1787 | -960.0 | -779.1 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -13.45 | 80.19 | 3.17 | 198.09 | 0.1743 | -842.0 | -760.7 | |
| 0.00 | 1.10 | 0.00 | 0.56 | -17.08 | 75.98 | -1.03 | 175.67 | 0.2287 | 798.0 | 605.4 | |
| 0.00 | 1.10 | 0.00 | 0.57 | -19.76 | 74.59 | -2.43 | 171.67 | 0.2764 | 825.0 | 634.5 | |
| 0.00 | 1.44 | 0.00 | 0.74 | -17.87 | 74.18 | -2.83 | 168.93 | 0.2461 | 915.0 | 814.5 | |
| 0.00 | 1.78 | 0.00 | 0.92 | -19.94 | 73.80 | -3.22 | 169.16 | 0.2816 | 833.0 | 573.7 | |
| 0.00 | 2.80 | 0.00 | 1.44 | -18.47 | 72.89 | -4.12 | 164.79 | 0.2609 | -1038.0 | -873.4 | |
| 0.00 | 0.93 | 0.00 | 0.48 | -14.66 | 66.65 | -10.36 | 137.02 | 0.2564 | 939.0 | 761.5 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -15.22 | 65.75 | -11.26 | 136.20 | 0.2735 | -690.0 | -618.5 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -15.73 | 63.53 | -13.48 | 132.51 | 0.3058 | -700.0 | -540.3 | |
| 0.00 | 1.27 | 0.00 | 0.68 | -18.28 | 59.40 | -17.61 | 131.08 | 0.3828 | -803.0 | -625.8 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -24.11 | 53.57 | -23.45 | 133.92 | 0.5062 | -773.0 | -646.7 | |
| 0.00 | 0.85 | 0.00 | 0.49 | -23.86 | 53.51 | -23.50 | 133.46 | 0.5045 | -731.0 | -595.8 | |
| 0.00 | 0.85 | 0.00 | 0.57 | -28.82 | 40.61 | -36.41 | 129.73 | 0.6785 | -551.0 | -496.2 | |
| 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. | |