SDO HMI 2011-10-24 09:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.82 | 0.00 | 12.99 | 23.84 | 330.73 | 29.02 | 306.79 | 0.5560 | -647.3 | -556.4 | |
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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 | 0.87 | 0.00 | 0.54 | 22.23 | 336.25 | 34.54 | 300.46 | 0.6111 | -470.0 | -457.9 | |
| 0.00 | 0.61 | 0.00 | 0.38 | 22.34 | 336.05 | 34.33 | 300.74 | 0.6092 | -432.0 | -516.7 | |
| 0.00 | 1.91 | 0.00 | 1.16 | 24.72 | 332.27 | 30.56 | 306.89 | 0.5796 | -406.0 | -390.0 | |
| 0.00 | 1.13 | 0.00 | 0.67 | 22.33 | 331.25 | 29.54 | 303.91 | 0.5516 | -698.0 | -581.9 | |
| 0.00 | 2.09 | 0.00 | 1.24 | 22.96 | 331.25 | 29.54 | 304.92 | 0.5558 | -718.0 | -559.5 | |
| 0.00 | 1.65 | 0.00 | 0.98 | 23.41 | 330.24 | 28.53 | 306.45 | 0.5470 | -783.0 | -668.5 | |
| 0.00 | 0.87 | 0.00 | 0.52 | 24.52 | 330.29 | 28.58 | 308.16 | 0.5556 | -514.0 | -515.3 | |
| 0.00 | 0.87 | 0.00 | 0.51 | 23.70 | 330.09 | 28.38 | 307.04 | 0.5473 | -666.0 | -543.6 | |
| 0.00 | 3.74 | 0.00 | 2.21 | 24.15 | 330.08 | 28.37 | 307.74 | 0.5505 | -560.0 | -557.3 | |
| 0.00 | 1.30 | 0.00 | 0.77 | 23.88 | 329.72 | 28.01 | 307.62 | 0.5443 | -884.0 | -775.1 | |
| 0.00 | 0.87 | 0.00 | 0.52 | 24.69 | 329.92 | 28.21 | 308.74 | 0.5527 | -633.0 | -570.7 | |
| 0.00 | 1.04 | 0.00 | 0.62 | 24.45 | 329.79 | 28.07 | 308.46 | 0.5493 | -777.0 | -559.4 | |
| 0.00 | 1.22 | 0.00 | 0.72 | 23.76 | 329.58 | 27.87 | 307.55 | 0.5418 | -691.0 | -476.4 | |
| 0.00 | 2.35 | 0.00 | 1.38 | 24.20 | 329.54 | 27.83 | 308.29 | 0.5446 | -742.0 | -589.1 | |
| 0.00 | 1.30 | 0.00 | 0.77 | 24.72 | 329.33 | 27.62 | 309.29 | 0.5462 | -736.0 | -546.4 | |
| 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. | |