SDO HMI 2014-09-29 00:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.32 | 31.91 | 0.66 | 15.86 | 7.88 | 207.87 | -3.25 | 68.69 | 0.0601 | -318.5 | 73.4 | |
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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 | 0.44 | 7.72 | 210.86 | -0.26 | 15.84 | 0.0163 | -831.0 | -601.6 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 7.39 | 210.74 | -0.38 | 33.63 | 0.0118 | -887.0 | -683.3 | |
| 0.00 | 1.41 | 0.00 | 0.70 | 7.33 | 210.50 | -0.62 | 50.73 | 0.0139 | -997.0 | -787.5 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 7.69 | 210.07 | -1.04 | 50.16 | 0.0236 | -997.0 | -805.7 | |
| 0.00 | 3.35 | 0.00 | 1.66 | 7.39 | 209.59 | -1.53 | 69.61 | 0.0283 | -1104.0 | -906.6 | |
| 0.00 | 1.23 | 0.00 | 0.61 | 7.60 | 208.53 | -2.59 | 73.20 | 0.0470 | -762.0 | -539.7 | |
| 0.00 | 1.15 | 0.00 | 0.57 | 7.81 | 208.26 | -2.86 | 70.84 | 0.0526 | -861.0 | -668.4 | |
| 0.00 | 1.50 | 0.00 | 0.74 | 6.52 | 208.05 | -3.07 | 95.73 | 0.0537 | -907.0 | -731.5 | |
| 0.00 | 2.29 | 0.00 | 1.14 | 7.36 | 207.99 | -3.13 | 80.23 | 0.0553 | -571.0 | -510.7 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 7.26 | 207.80 | -3.31 | 82.29 | 0.0581 | -988.0 | -803.8 | |
| 0.00 | 1.41 | 0.00 | 0.70 | 7.89 | 207.13 | -3.99 | 74.74 | 0.0717 | 847.0 | 648.9 | |
| 0.00 | 1.15 | 0.00 | 0.57 | 8.70 | 206.88 | -4.24 | 65.73 | 0.0805 | 734.0 | 576.2 | |
| 0.00 | 6.79 | 0.00 | 3.37 | 8.10 | 206.73 | -4.38 | 73.47 | 0.0793 | 896.0 | 919.8 | |
| 0.00 | 0.88 | 0.00 | 0.44 | 8.37 | 206.73 | -4.39 | 70.24 | 0.0808 | 950.0 | 710.0 | |
| 1.32 | 6.79 | 0.66 | 3.38 | 8.55 | 206.64 | -4.48 | 68.56 | 0.0834 | 1224.8 | 827.6 | |
| 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. | |