SDO HMI 2011-10-24 06:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.89 | 0.00 | 14.13 | 23.26 | 332.00 | 28.65 | 306.31 | 0.5482 | -714.0 | -580.1 | |
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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 | 2.00 | 0.00 | 1.26 | 21.55 | 338.77 | 35.42 | 298.92 | 0.6181 | -635.0 | -446.9 | |
| 0.00 | 0.87 | 0.00 | 0.53 | 20.41 | 337.11 | 33.75 | 298.05 | 0.5923 | -547.0 | -442.8 | |
| 0.00 | 1.48 | 0.00 | 0.90 | 21.48 | 336.19 | 32.84 | 300.28 | 0.5865 | -805.0 | -618.7 | |
| 0.00 | 0.87 | 0.00 | 0.53 | 22.30 | 336.13 | 32.78 | 301.60 | 0.5904 | -701.0 | -576.0 | |
| 0.00 | 1.04 | 0.00 | 0.62 | 24.84 | 332.39 | 29.04 | 308.24 | 0.5630 | -697.0 | -572.4 | |
| 0.00 | 1.74 | 0.00 | 1.02 | 22.20 | 331.25 | 27.89 | 304.96 | 0.5307 | -835.0 | -625.2 | |
| 0.00 | 1.30 | 0.00 | 0.76 | 22.89 | 331.33 | 27.97 | 306.03 | 0.5365 | -838.0 | -657.0 | |
| 0.00 | 1.04 | 0.00 | 0.61 | 22.64 | 331.16 | 27.81 | 305.77 | 0.5328 | -815.0 | -658.3 | |
| 0.00 | 2.78 | 0.00 | 1.62 | 23.46 | 330.32 | 26.97 | 307.84 | 0.5289 | -698.0 | -492.2 | |
| 0.00 | 1.04 | 0.00 | 0.61 | 24.69 | 330.60 | 27.25 | 309.55 | 0.5416 | -523.0 | -379.8 | |
| 0.00 | 2.09 | 0.00 | 1.22 | 24.07 | 330.09 | 26.74 | 309.04 | 0.5310 | -802.0 | -606.9 | |
| 0.00 | 1.04 | 0.00 | 0.61 | 24.83 | 330.12 | 26.77 | 310.22 | 0.5374 | -646.0 | -512.6 | |
| 0.00 | 4.17 | 0.00 | 2.42 | 23.80 | 329.70 | 26.35 | 308.96 | 0.5243 | -693.0 | -707.3 | |
| 0.00 | 1.30 | 0.00 | 0.76 | 24.53 | 329.83 | 26.47 | 310.01 | 0.5316 | -888.0 | -705.4 | |
| 0.00 | 1.13 | 0.00 | 0.66 | 25.06 | 329.91 | 26.56 | 310.77 | 0.5369 | -587.0 | -476.5 | |
| 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. | |