SDO HMI 2014-01-12 09:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 78.31 | 476.82 | 44.04 | 268.59 | -16.44 | 13.56 | -26.14 | 117.33 | 0.4775 | 984.5 | 371.4 | |
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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 | 1.28 | 0.00 | 0.70 | -16.19 | 16.42 | -23.27 | 119.23 | 0.4367 | -866.0 | -739.0 | |
| 47.87 | 468.64 | 26.81 | 263.71 | -16.49 | 14.19 | -25.51 | 117.88 | 0.4692 | 1359.6 | 392.4 | |
| 0.85 | -2.00 | 0.48 | -2.00 | -16.40 | 13.45 | -26.25 | 117.14 | 0.4788 | 1019.5 | 999999 | |
| 6.97 | -2.00 | 3.94 | -2.00 | -16.57 | 13.15 | -26.55 | 117.24 | 0.4838 | 1171.1 | 999999 | |
| 1.87 | -2.00 | 1.06 | -2.00 | -16.69 | 12.92 | -26.77 | 117.29 | 0.4875 | 755.9 | 999999 | |
| 20.75 | -2.00 | 11.75 | -2.00 | -16.26 | 12.75 | -26.95 | 116.34 | 0.4875 | 1251.5 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.45 | -16.82 | 8.17 | -31.53 | 114.46 | 0.5521 | -869.0 | -636.6 | |
| 0.00 | 0.77 | 0.00 | 0.45 | -16.53 | 7.89 | -31.80 | 113.82 | 0.5544 | -766.0 | -614.9 | |
| 0.00 | 1.02 | 0.00 | 0.61 | -16.27 | 6.67 | -33.03 | 112.75 | 0.5696 | -713.0 | -581.1 | |
| 0.00 | 1.19 | 0.00 | 0.72 | -16.15 | 6.51 | -33.19 | 112.46 | 0.5712 | -643.0 | -522.0 | |
| 0.00 | 0.68 | 0.00 | 0.42 | -19.02 | 5.22 | -34.48 | 116.50 | 0.6003 | -693.0 | -582.6 | |
| 0.00 | 1.02 | 0.00 | 0.62 | -15.27 | 5.75 | -33.94 | 110.64 | 0.5779 | -750.0 | -611.2 | |
| 0.00 | 1.45 | 0.00 | 0.91 | -17.85 | 3.67 | -36.03 | 113.91 | 0.6148 | -560.0 | -406.2 | |
| 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. | |