SDO HMI 2014-08-22 06:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.12 | 140.78 | 14.80 | 89.61 | 16.48 | 28.10 | 38.48 | 287.79 | 0.6286 | -598.8 | -289.0 | |
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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 |
| 21.23 | 123.32 | 13.60 | 79.05 | 16.34 | 28.70 | 39.08 | 287.36 | 0.6361 | -1095.1 | -333.6 | |
| 1.89 | -1.00 | 1.20 | -1.00 | 16.40 | 28.31 | 38.69 | 287.55 | 0.6312 | -1104.0 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.78 | 13.95 | 26.74 | 37.13 | 283.97 | 0.6059 | -565.0 | -459.1 | |
| 0.00 | 1.44 | 0.00 | 0.90 | 17.60 | 26.66 | 37.04 | 289.93 | 0.6130 | -737.0 | -505.6 | |
| 0.00 | 2.79 | 0.00 | 1.75 | 17.88 | 26.73 | 37.11 | 290.35 | 0.6147 | -540.0 | -587.5 | |
| 0.00 | 1.26 | 0.00 | 0.79 | 17.68 | 26.44 | 36.82 | 290.13 | 0.6104 | -746.0 | -568.5 | |
| 0.00 | 1.17 | 0.00 | 0.72 | 17.07 | 25.86 | 36.24 | 289.32 | 0.6011 | -781.0 | -643.8 | |
| 0.00 | 1.08 | 0.00 | 0.67 | 17.44 | 25.87 | 36.25 | 289.93 | 0.6023 | -693.0 | -503.8 | |
| 0.00 | 1.08 | 0.00 | 0.64 | 18.66 | 21.58 | 31.97 | 293.73 | 0.5500 | 480.0 | 395.8 | |
| 0.00 | 2.52 | 0.00 | 1.48 | 17.37 | 21.28 | 31.67 | 291.59 | 0.5409 | 768.0 | 615.5 | |
| 0.00 | 1.08 | 0.00 | 0.63 | 18.49 | 20.87 | 31.25 | 293.78 | 0.5397 | 716.0 | 582.8 | |
| 0.00 | 1.08 | 0.00 | 0.63 | 18.34 | 20.73 | 31.11 | 293.59 | 0.5372 | 751.0 | 663.3 | |
| 0.00 | 0.99 | 0.00 | 0.58 | 18.88 | 20.61 | 30.99 | 294.60 | 0.5380 | 770.0 | 588.8 | |
| 0.00 | 1.71 | 0.00 | 0.99 | 17.25 | 19.70 | 30.08 | 292.11 | 0.5188 | 747.0 | 613.8 | |
| 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. | |