SDO HMI 2014-01-11 01:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.92 | 76.70 | 11.29 | 39.44 | -13.13 | 44.18 | -13.05 | 125.79 | 0.2722 | -277.6 | -299.2 | |
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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 | 1.36 | 0.00 | 0.69 | -12.71 | 47.24 | -9.99 | 131.58 | 0.2273 | 1050.0 | 833.6 | |
| 0.00 | 1.70 | 0.00 | 0.87 | -13.02 | 46.55 | -10.68 | 130.79 | 0.2396 | 967.0 | 600.6 | |
| 0.00 | 1.10 | 0.00 | 0.56 | -13.47 | 46.53 | -10.70 | 132.16 | 0.2447 | 562.0 | 453.8 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -13.14 | 46.48 | -10.75 | 131.00 | 0.2417 | 952.0 | 737.4 | |
| 0.34 | 1.27 | 0.17 | 0.65 | -13.76 | 46.12 | -11.11 | 132.01 | 0.2531 | 970.5 | 825.5 | |
| 0.00 | 1.70 | 0.00 | 0.87 | -12.66 | 46.14 | -11.09 | 128.55 | 0.2412 | 958.0 | 880.3 | |
| 0.00 | 1.10 | 0.00 | 0.56 | -12.53 | 45.71 | -11.52 | 127.12 | 0.2456 | 872.0 | 615.3 | |
| 0.00 | 3.48 | 0.00 | 1.78 | -12.61 | 45.06 | -12.17 | 125.93 | 0.2552 | -888.0 | -774.9 | |
| 0.00 | 1.27 | 0.00 | 0.65 | -12.49 | 44.85 | -12.38 | 125.08 | 0.2570 | -955.0 | -767.8 | |
| 0.00 | 1.61 | 0.00 | 0.83 | -13.97 | 44.18 | -13.05 | 128.24 | 0.2803 | 871.0 | 655.8 | |
| 3.40 | 58.46 | 1.75 | 30.11 | -13.01 | 44.05 | -13.18 | 125.11 | 0.2729 | -1191.6 | -577.8 | |
| 0.00 | 2.29 | 0.00 | 1.18 | -14.03 | 43.93 | -13.30 | 127.89 | 0.2842 | 489.0 | 431.4 | |
| 0.68 | -11.00 | 0.35 | -11.00 | -13.58 | 43.80 | -13.43 | 126.32 | 0.2816 | -887.0 | 999999 | |
| 17.50 | -11.00 | 9.02 | -11.00 | -13.10 | 43.70 | -13.53 | 124.70 | 0.2784 | -1019.5 | 999999 | |
| 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. | |