SDO HMI 2011-10-22 20:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.17 | 24.16 | 1.10 | 12.30 | 17.55 | 320.65 | -1.39 | 6.41 | 0.2258 | 350.0 | 286.1 | |
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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 |
| 0.00 | 1.39 | 0.00 | 0.71 | 17.83 | 326.26 | 4.23 | 342.11 | 0.2295 | -823.0 | -613.8 | |
| 0.00 | 1.48 | 0.00 | 0.74 | 14.22 | 325.91 | 3.87 | 337.15 | 0.1695 | 951.0 | 764.7 | |
| 1.30 | 2.43 | 0.66 | 1.24 | 17.96 | 324.98 | 2.94 | 347.45 | 0.2259 | 788.7 | 795.7 | |
| 0.00 | 1.65 | 0.00 | 0.84 | 18.27 | 324.42 | 2.38 | 350.03 | 0.2292 | 749.0 | 608.7 | |
| 0.87 | 2.17 | 0.44 | 1.11 | 18.94 | 324.27 | 2.24 | 351.12 | 0.2401 | 1015.2 | 933.1 | |
| 0.00 | 1.30 | 0.00 | 0.67 | 18.82 | 324.08 | 2.04 | 351.79 | 0.2375 | 950.0 | 795.2 | |
| 0.00 | 1.65 | 0.00 | 0.85 | 21.29 | 320.72 | -1.32 | 4.44 | 0.2778 | 808.0 | 663.7 | |
| 0.00 | 1.91 | 0.00 | 0.98 | 19.68 | 319.85 | -2.19 | 8.23 | 0.2523 | 783.0 | 501.5 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 16.73 | 317.01 | -5.02 | 22.88 | 0.2166 | -875.0 | -683.9 | |
| 0.00 | 2.35 | 0.00 | 1.19 | 16.58 | 316.86 | -5.17 | 23.79 | 0.2152 | -1011.0 | -710.1 | |
| 0.00 | 2.26 | 0.00 | 1.15 | 16.73 | 316.76 | -5.27 | 23.89 | 0.2183 | -802.0 | -532.1 | |
| 0.00 | 2.96 | 0.00 | 1.50 | 15.75 | 315.86 | -6.18 | 29.65 | 0.2104 | 1001.0 | 821.1 | |
| 0.00 | 1.48 | 0.00 | 0.75 | 15.93 | 315.63 | -6.40 | 30.08 | 0.2149 | 872.0 | 680.7 | |
| 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. | |