SDO HMI 2011-10-21 23:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.18 | 48.48 | 9.31 | 24.95 | 18.20 | 324.61 | -8.96 | 33.01 | 0.2691 | 449.9 | 320.6 | |
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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 | 1.31 | 0.00 | 0.66 | 14.40 | 327.27 | -6.30 | 33.98 | 0.1910 | 819.0 | 555.6 | |
| 7.57 | 12.36 | 3.86 | 6.29 | 17.01 | 326.78 | -6.79 | 29.18 | 0.2329 | -1055.7 | -877.1 | |
| 2.61 | 5.66 | 1.33 | 2.89 | 17.19 | 326.40 | -7.17 | 30.12 | 0.2387 | -954.1 | -704.8 | |
| 0.00 | 2.61 | 0.00 | 1.34 | 18.12 | 325.28 | -8.29 | 31.71 | 0.2618 | 860.0 | 594.3 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 17.56 | 324.87 | -8.70 | 34.19 | 0.2578 | 814.0 | 685.8 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 19.03 | 324.54 | -9.03 | 32.02 | 0.2812 | 666.0 | 579.5 | |
| 0.00 | 1.39 | 0.00 | 0.72 | 19.21 | 324.53 | -9.04 | 31.69 | 0.2838 | 663.0 | 556.2 | |
| 0.78 | 5.92 | 0.40 | 3.06 | 18.78 | 324.07 | -9.50 | 33.83 | 0.2819 | 1244.3 | 874.0 | |
| 7.22 | 8.96 | 3.72 | 4.62 | 18.44 | 323.99 | -9.57 | 34.76 | 0.2780 | 1173.5 | 898.2 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 18.49 | 323.54 | -10.02 | 35.85 | 0.2831 | 896.0 | 724.7 | |
| 0.00 | 1.65 | 0.00 | 0.85 | 18.31 | 323.49 | -10.08 | 36.40 | 0.2812 | 906.0 | 756.5 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 20.25 | 320.19 | -13.38 | 39.96 | 0.3396 | 926.0 | 684.8 | |
| 0.00 | 1.22 | 0.00 | 0.64 | 20.15 | 319.80 | -13.77 | 40.93 | 0.3425 | 898.0 | 753.9 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 20.38 | 319.26 | -14.31 | 41.51 | 0.3512 | 653.0 | 517.4 | |
| 0.00 | 2.18 | 0.00 | 1.17 | 22.98 | 318.49 | -15.08 | 38.10 | 0.3899 | 722.0 | 586.2 | |
| 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. | |