SDO HMI 2014-09-08 14:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.74 | 161.93 | 31.58 | 162.48 | -16.43 | 64.51 | -56.15 | 113.64 | 0.8704 | 190.8 | 27.3 | |
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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 |
| 21.13 | 108.34 | 20.06 | 102.91 | -16.34 | 66.51 | -54.15 | 114.22 | 0.8549 | 663.2 | 172.1 | |
| 2.05 | -1.00 | 1.97 | -1.00 | -16.76 | 66.16 | -54.49 | 114.56 | 0.8590 | -228.0 | 999999 | |
| 0.00 | 1.16 | 0.00 | 1.14 | -16.46 | 65.36 | -55.30 | 113.93 | 0.8646 | 179.0 | 173.2 | |
| 0.00 | 1.25 | 0.00 | 1.20 | -14.97 | 65.63 | -55.02 | 112.39 | 0.8581 | -460.0 | -336.6 | |
| 0.00 | 1.34 | 0.00 | 1.34 | -16.62 | 64.72 | -55.93 | 113.88 | 0.8701 | 409.0 | 330.5 | |
| 0.89 | 2.14 | 0.89 | 2.13 | -16.23 | 64.72 | -55.93 | 113.46 | 0.8690 | 319.5 | 267.6 | |
| 0.00 | 2.50 | 0.00 | 2.53 | -16.59 | 64.11 | -56.55 | 113.63 | 0.8748 | 362.0 | 124.0 | |
| 0.00 | 1.16 | 0.00 | 1.28 | -16.48 | 61.35 | -59.30 | 112.59 | 0.8949 | -659.0 | -622.8 | |
| 0.00 | 0.71 | 0.00 | 0.85 | -19.05 | 59.70 | -60.95 | 114.79 | 0.9119 | -266.0 | -310.0 | |
| 2.32 | 40.48 | 2.60 | 45.75 | -16.23 | 60.66 | -59.99 | 112.11 | 0.8993 | -625.2 | -253.8 | |
| 5.35 | -10.00 | 6.06 | -10.00 | -16.54 | 60.50 | -60.15 | 112.39 | 0.9011 | -499.7 | 999999 | |
| 0.00 | 0.98 | 0.00 | 1.14 | -17.34 | 60.07 | -60.59 | 113.10 | 0.9058 | -363.0 | -378.2 | |
| 0.00 | 1.87 | 0.00 | 2.21 | -17.83 | 59.72 | -60.94 | 113.52 | 0.9092 | -136.0 | -150.6 | |
| 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. | |