SDO HMI 2014-09-27 03:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.36 | 0.00 | 9.59 | -16.68 | 208.13 | -27.73 | 131.67 | 0.6046 | 89.3 | 25.1 | |
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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 | 1.32 | 0.00 | 0.78 | -18.00 | 215.06 | -20.80 | 140.78 | 0.5361 | 770.0 | 606.9 | |
| 0.00 | 1.41 | 0.00 | 0.83 | -17.71 | 215.10 | -20.76 | 140.45 | 0.5324 | 779.0 | 655.5 | |
| 0.00 | 1.32 | 0.00 | 0.79 | -19.15 | 213.99 | -21.87 | 140.77 | 0.5586 | -693.0 | -611.5 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -16.26 | 214.36 | -21.50 | 137.60 | 0.5238 | 796.0 | 596.0 | |
| 0.00 | 1.68 | 0.00 | 0.99 | -16.20 | 212.81 | -23.05 | 135.55 | 0.5389 | -814.0 | -675.9 | |
| 0.00 | 0.71 | 0.00 | 0.45 | -23.33 | 211.24 | -24.62 | 142.22 | 0.6267 | 486.0 | 456.4 | |
| 0.00 | 0.97 | 0.00 | 0.62 | -23.31 | 211.07 | -24.79 | 142.00 | 0.6279 | 621.0 | 614.1 | |
| 0.00 | 1.77 | 0.00 | 1.12 | -23.49 | 211.00 | -24.87 | 142.11 | 0.6303 | 680.0 | 589.2 | |
| 0.00 | 0.79 | 0.00 | 0.49 | -16.63 | 207.81 | -28.05 | 130.57 | 0.5954 | 532.0 | 442.6 | |
| 0.00 | 1.50 | 0.00 | 0.97 | -15.35 | 202.01 | -33.85 | 123.75 | 0.6484 | -685.0 | -583.9 | |
| 0.00 | 0.71 | 0.00 | 0.46 | -15.69 | 201.72 | -34.15 | 123.98 | 0.6540 | -495.0 | -429.2 | |
| 0.00 | 0.62 | 0.00 | 0.44 | -21.35 | 199.06 | -36.80 | 128.95 | 0.7198 | -411.0 | -454.3 | |
| 0.00 | 1.77 | 0.00 | 1.19 | -1.39 | 194.08 | -41.78 | 99.69 | 0.6781 | -405.0 | -331.5 | |
| 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. | |