SDO HMI 2014-11-08 10:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.86 | 17.50 | 0.47 | 9.81 | -15.27 | 17.67 | -20.36 | 133.96 | 0.4651 | -343.5 | -252.1 | |
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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 | 1.29 | 0.00 | 0.70 | -13.49 | 21.97 | -16.06 | 137.32 | 0.3985 | 932.0 | 760.9 | |
| 0.00 | 3.02 | 0.00 | 1.63 | -13.28 | 21.80 | -16.24 | 136.63 | 0.3980 | 943.0 | 770.0 | |
| 0.86 | 2.07 | 0.47 | 1.13 | -14.03 | 20.01 | -18.02 | 134.98 | 0.4261 | -951.6 | -859.6 | |
| 0.00 | 1.55 | 0.00 | 0.85 | -14.21 | 20.00 | -18.04 | 135.28 | 0.4284 | -759.0 | -615.1 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -15.73 | 18.00 | -20.03 | 134.80 | 0.4666 | 730.0 | 563.8 | |
| 0.00 | 1.04 | 0.00 | 0.59 | -16.30 | 16.35 | -21.69 | 133.47 | 0.4907 | -840.0 | -648.9 | |
| 0.00 | 3.36 | 0.00 | 1.92 | -16.25 | 15.85 | -22.18 | 132.76 | 0.4957 | -878.0 | -817.0 | |
| 0.00 | 1.12 | 0.00 | 0.64 | -16.60 | 15.71 | -22.32 | 133.12 | 0.5007 | -753.0 | -647.8 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -16.67 | 15.50 | -22.53 | 132.96 | 0.5037 | -677.0 | -537.8 | |
| 0.00 | 1.29 | 0.00 | 0.75 | -17.65 | 14.25 | -23.78 | 132.93 | 0.5270 | -670.0 | -555.5 | |
| 0.00 | 0.95 | 0.00 | 0.58 | -16.42 | 8.60 | -29.44 | 125.37 | 0.5804 | -569.0 | -430.5 | |
| 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. | |