SDO HMI 2011-10-17 12:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.91 | 36.57 | 6.68 | 22.35 | -15.24 | 3.04 | -29.36 | 126.17 | 0.5878 | 47.9 | 119.3 | |
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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 | 1.57 | 0.00 | 0.94 | -15.16 | 5.36 | -27.03 | 128.24 | 0.5607 | 806.0 | 714.5 | |
| 1.92 | 9.77 | 1.15 | 5.87 | -15.09 | 4.74 | -27.65 | 127.52 | 0.5672 | 931.8 | 761.2 | |
| 2.53 | -2.00 | 1.52 | -2.00 | -15.32 | 4.67 | -27.72 | 127.78 | 0.5698 | 748.4 | 999999 | |
| 0.00 | 1.66 | 0.00 | 1.00 | -15.59 | 4.46 | -27.93 | 127.95 | 0.5745 | 597.0 | 499.3 | |
| 0.00 | 1.57 | 0.00 | 0.95 | -14.99 | 4.34 | -28.06 | 126.97 | 0.5709 | 684.0 | 583.2 | |
| 0.00 | 1.40 | 0.00 | 0.84 | -14.64 | 4.24 | -28.15 | 126.38 | 0.5691 | 628.0 | 583.6 | |
| 0.00 | 1.05 | 0.00 | 0.63 | -14.55 | 3.52 | -28.87 | 125.57 | 0.5768 | 566.0 | 443.2 | |
| 0.00 | 2.18 | 0.00 | 1.33 | -15.24 | 3.17 | -29.22 | 126.23 | 0.5862 | 672.0 | 495.8 | |
| 0.00 | 1.40 | 0.00 | 0.87 | -15.90 | 2.10 | -30.30 | 126.20 | 0.6035 | -700.0 | -585.1 | |
| 0.00 | 0.96 | 0.00 | 0.59 | -14.46 | 2.11 | -30.28 | 124.18 | 0.5925 | -579.0 | -401.3 | |
| 4.45 | 8.55 | 2.76 | 5.31 | -15.72 | 1.84 | -30.56 | 125.73 | 0.6051 | -836.4 | -629.9 | |
| 0.00 | 1.66 | 0.00 | 1.03 | -15.18 | 1.13 | -31.26 | 124.37 | 0.6091 | -395.0 | -401.9 | |
| 0.00 | 1.40 | 0.00 | 0.87 | -14.88 | 0.89 | -31.50 | 123.75 | 0.6096 | -528.0 | -512.7 | |
| 2.01 | 3.40 | 1.25 | 2.12 | -14.66 | 0.89 | -31.50 | 123.43 | 0.6080 | -682.3 | -586.4 | |
| 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. | |