SDO HMI 2014-09-24 06:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.80 | 26.27 | 2.31 | 15.93 | -15.30 | 246.34 | -27.47 | 129.44 | 0.5784 | -789.7 | -682.5 | |
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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 | 0.88 | 0.00 | 0.53 | -15.34 | 247.27 | -26.54 | 130.47 | 0.5687 | -475.0 | -598.5 | |
| 0.00 | 3.36 | 0.00 | 2.03 | -15.55 | 247.06 | -26.75 | 130.54 | 0.5728 | -802.0 | -696.3 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -14.25 | 247.17 | -26.64 | 128.83 | 0.5601 | -669.0 | -574.8 | |
| 0.00 | 1.77 | 0.00 | 1.06 | -14.10 | 247.05 | -26.76 | 128.49 | 0.5601 | -762.0 | -600.8 | |
| 0.00 | 1.24 | 0.00 | 0.75 | -15.71 | 246.48 | -27.33 | 130.16 | 0.5805 | -691.0 | -552.5 | |
| 0.00 | 0.71 | 0.00 | 0.43 | -15.45 | 246.48 | -27.33 | 129.80 | 0.5782 | -718.0 | -640.0 | |
| 0.35 | 4.42 | 0.21 | 2.68 | -15.27 | 246.29 | -27.52 | 129.36 | 0.5786 | -935.0 | -779.4 | |
| 0.00 | 1.24 | 0.00 | 0.75 | -14.71 | 246.37 | -27.44 | 128.67 | 0.5730 | -943.0 | -735.6 | |
| 0.00 | 3.98 | 0.00 | 2.44 | -15.94 | 245.88 | -27.93 | 129.86 | 0.5890 | -748.0 | -628.0 | |
| 2.65 | 6.55 | 1.62 | 3.98 | -15.36 | 245.93 | -27.88 | 129.11 | 0.5834 | -913.0 | -787.1 | |
| 0.80 | -10.00 | 0.48 | -10.00 | -15.10 | 245.93 | -27.88 | 128.76 | 0.5812 | -942.2 | 999999 | |
| 0.00 | 1.15 | 0.00 | 0.70 | -15.34 | 245.65 | -28.16 | 128.81 | 0.5863 | -698.0 | -594.7 | |
| 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. | |