SDO HMI 2014-09-12 22:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.20 | 145.80 | 17.36 | 78.62 | -15.83 | 65.81 | 2.39 | 185.88 | 0.3966 | 597.9 | 397.0 | |
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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 |
| 1.51 | 131.91 | 0.82 | 71.10 | -15.95 | 66.96 | 3.54 | 188.59 | 0.3997 | 1014.4 | 524.2 | |
| 0.00 | 1.16 | 0.00 | 0.62 | -15.26 | 66.76 | 3.34 | 188.37 | 0.3883 | 178.0 | 188.0 | |
| 12.45 | -1.00 | 6.72 | -1.00 | -15.85 | 66.58 | 3.16 | 187.72 | 0.3973 | 1156.5 | 999999 | |
| 8.81 | -1.00 | 4.75 | -1.00 | -15.85 | 66.24 | 2.82 | 186.88 | 0.3965 | 1196.4 | 999999 | |
| 5.34 | -1.00 | 2.87 | -1.00 | -15.55 | 66.08 | 2.66 | 186.58 | 0.3915 | 1399.4 | 999999 | |
| 1.78 | -1.00 | 0.96 | -1.00 | -15.81 | 65.89 | 2.47 | 186.06 | 0.3953 | 919.0 | 999999 | |
| 2.31 | -1.00 | 1.24 | -1.00 | -15.65 | 65.83 | 2.41 | 185.94 | 0.3926 | 998.6 | 999999 | |
| 0.00 | 0.80 | 0.00 | 0.43 | -14.89 | 63.98 | 0.56 | 181.43 | 0.3784 | 768.0 | 653.3 | |
| 0.00 | 2.05 | 0.00 | 1.11 | -17.09 | 62.05 | -1.36 | 176.84 | 0.4143 | -813.0 | -768.4 | |
| 0.00 | 3.11 | 0.00 | 1.69 | -17.05 | 61.74 | -1.68 | 176.11 | 0.4141 | -768.0 | -657.3 | |
| 0.00 | 1.33 | 0.00 | 0.71 | -13.11 | 60.41 | -3.01 | 171.64 | 0.3529 | -726.0 | -483.9 | |
| 0.00 | 1.25 | 0.00 | 0.69 | -18.66 | 59.94 | -3.48 | 172.50 | 0.4422 | -854.0 | -781.4 | |
| 0.00 | 1.25 | 0.00 | 0.66 | -13.82 | 59.84 | -3.57 | 170.43 | 0.3658 | -846.0 | -638.6 | |
| 0.00 | 1.69 | 0.00 | 0.92 | -16.29 | 57.91 | -5.51 | 166.98 | 0.4109 | -800.0 | -642.2 | |
| 0.00 | 1.25 | 0.00 | 0.69 | -17.70 | 56.56 | -6.86 | 164.87 | 0.4377 | -802.0 | -576.3 | |
| 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. | |