SDO HMI 2014-01-10 05:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.70 | 0.00 | 9.21 | -18.28 | 70.27 | 2.06 | 192.46 | 0.3067 | 11.0 | -51.8 | |
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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 | 1.28 | 0.00 | 0.67 | -19.40 | 81.63 | 13.42 | 219.41 | 0.3464 | 886.0 | 756.4 | |
| 0.00 | 2.55 | 0.00 | 1.31 | -12.77 | 80.57 | 12.36 | 233.72 | 0.2602 | -882.0 | -812.6 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -13.25 | 80.50 | 12.29 | 232.07 | 0.2639 | -922.0 | -723.1 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -16.72 | 76.48 | 8.27 | 212.04 | 0.2608 | 840.0 | 645.1 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -18.85 | 75.60 | 7.39 | 205.42 | 0.2848 | 788.0 | 622.1 | |
| 0.00 | 2.21 | 0.00 | 1.13 | -17.86 | 74.59 | 6.38 | 203.87 | 0.2626 | 817.0 | 647.5 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -18.04 | 74.29 | 6.07 | 202.57 | 0.2634 | 1032.0 | 750.2 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -21.95 | 72.20 | 3.99 | 191.86 | 0.3155 | 684.0 | 580.4 | |
| 0.00 | 1.96 | 0.00 | 1.01 | -18.33 | 59.41 | -8.80 | 149.59 | 0.2883 | -925.0 | -702.1 | |
| 0.00 | 0.68 | 0.00 | 0.37 | -24.40 | 53.80 | -14.42 | 147.05 | 0.4187 | -716.0 | -587.8 | |
| 0.00 | 1.62 | 0.00 | 0.89 | -25.09 | 53.07 | -15.14 | 146.78 | 0.4336 | -739.0 | -589.2 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -18.61 | 52.16 | -16.05 | 134.11 | 0.3666 | -731.0 | -508.2 | |
| 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. | |