SDO HMI 2014-01-10 08:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.35 | 0.00 | 12.60 | -15.91 | 73.12 | 6.54 | 208.59 | 0.2918 | -514.9 | -374.3 | |
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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 | 1.11 | 0.00 | 0.57 | -12.75 | 81.24 | 14.66 | 238.15 | 0.2920 | -668.0 | -492.1 | |
| 0.00 | 1.45 | 0.00 | 0.75 | -13.17 | 81.23 | 14.66 | 236.90 | 0.2954 | -809.0 | -629.0 | |
| 0.00 | 3.23 | 0.00 | 1.67 | -13.12 | 80.82 | 14.25 | 236.35 | 0.2892 | -885.0 | -775.7 | |
| 0.00 | 2.81 | 0.00 | 1.45 | -12.82 | 80.71 | 14.14 | 237.04 | 0.2851 | -954.0 | -803.4 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -12.68 | 80.52 | 13.94 | 237.14 | 0.2811 | -973.0 | -875.1 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -12.59 | 80.33 | 13.75 | 237.06 | 0.2776 | -871.0 | -698.4 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -16.08 | 77.43 | 10.85 | 220.84 | 0.2780 | -899.0 | -724.7 | |
| 0.00 | 3.23 | 0.00 | 1.66 | -16.81 | 76.50 | 9.92 | 216.66 | 0.2776 | 916.0 | 711.7 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -17.86 | 74.71 | 8.13 | 209.38 | 0.2757 | 942.0 | 793.1 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -21.89 | 72.26 | 5.68 | 196.68 | 0.3214 | 780.0 | 647.1 | |
| 0.00 | 1.36 | 0.00 | 0.68 | -13.31 | 69.06 | 2.48 | 194.67 | 0.1670 | -907.0 | -533.8 | |
| 0.00 | 0.77 | 0.00 | 0.39 | -16.10 | 68.87 | 2.29 | 190.44 | 0.2132 | -830.0 | -653.2 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -19.10 | 59.28 | -7.30 | 155.21 | 0.2876 | -609.0 | -511.1 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -15.67 | 54.58 | -12.00 | 135.35 | 0.2862 | -974.0 | -896.9 | |
| 0.00 | 1.19 | 0.00 | 0.64 | -24.07 | 53.66 | -12.91 | 149.31 | 0.4015 | -825.0 | -555.5 | |
| 0.00 | 0.85 | 0.00 | 0.48 | -24.80 | 45.07 | -21.51 | 137.14 | 0.4912 | -672.0 | -538.7 | |
| 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. | |