SDO HMI 2011-10-18 10:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.99 | 87.84 | 27.76 | 48.82 | -14.58 | 2.43 | -17.87 | 139.06 | 0.4548 | -66.4 | -106.1 | |
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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 |
| 10.12 | 13.00 | 5.55 | 7.12 | -15.16 | 5.62 | -14.68 | 145.19 | 0.4303 | 890.6 | 748.4 | |
| 0.00 | 0.96 | 0.00 | 0.53 | -15.36 | 5.03 | -15.27 | 144.41 | 0.4383 | 229.0 | 230.3 | |
| 5.23 | 7.68 | 2.88 | 4.22 | -15.05 | 4.95 | -15.35 | 143.84 | 0.4350 | 944.4 | 756.6 | |
| 0.00 | 1.13 | 0.00 | 0.62 | -14.48 | 4.71 | -15.59 | 142.59 | 0.4302 | 863.0 | 714.5 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -14.70 | 4.63 | -15.67 | 142.78 | 0.4338 | 881.0 | 674.8 | |
| 0.00 | 1.31 | 0.00 | 0.72 | -14.65 | 4.47 | -15.83 | 142.42 | 0.4346 | 720.0 | 543.3 | |
| 2.44 | 7.07 | 1.35 | 3.91 | -14.73 | 3.72 | -16.58 | 141.27 | 0.4428 | 691.6 | 480.5 | |
| 1.57 | -7.00 | 0.87 | -7.00 | -15.09 | 3.50 | -16.80 | 141.42 | 0.4493 | 596.4 | 999999 | |
| 0.00 | 1.22 | 0.00 | 0.69 | -16.16 | 1.84 | -18.46 | 140.31 | 0.4781 | -772.0 | -702.3 | |
| 3.58 | 4.27 | 1.98 | 2.37 | -13.71 | 1.93 | -18.37 | 136.82 | 0.4493 | -910.2 | -782.9 | |
| 0.00 | 1.13 | 0.00 | 0.63 | -14.45 | 1.51 | -18.79 | 137.32 | 0.4620 | -599.0 | -480.6 | |
| 5.50 | 10.03 | 3.06 | 5.58 | -14.07 | 1.38 | -18.92 | 136.55 | 0.4592 | -913.2 | -701.4 | |
| 3.58 | 5.15 | 2.02 | 2.91 | -15.87 | 0.98 | -19.31 | 138.63 | 0.4833 | 790.7 | 695.0 | |
| 0.00 | 2.27 | 0.00 | 1.26 | -13.68 | 0.93 | -19.37 | 135.26 | 0.4598 | -793.0 | -703.5 | |
| 17.97 | 31.75 | 10.05 | 17.78 | -14.22 | 0.78 | -19.52 | 135.89 | 0.4672 | -890.9 | -438.9 | |
| 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. | |