SDO HMI 2014-09-29 07:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.52 | 0.00 | 13.59 | -15.54 | 165.33 | -41.94 | 118.54 | 0.7371 | 281.2 | 311.0 | |
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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 |
| 0.00 | 2.21 | 0.00 | 1.49 | -17.32 | 171.47 | -35.80 | 124.74 | 0.6819 | 659.0 | 483.4 | |
| 0.00 | 1.06 | 0.00 | 0.82 | -23.47 | 166.49 | -40.79 | 128.56 | 0.7686 | 544.0 | 485.2 | |
| 0.00 | 3.00 | 0.00 | 2.30 | -22.62 | 166.33 | -40.95 | 127.52 | 0.7650 | 576.0 | 382.4 | |
| 0.00 | 3.09 | 0.00 | 2.15 | -13.22 | 167.17 | -40.11 | 116.69 | 0.7043 | 740.0 | 569.7 | |
| 0.00 | 0.79 | 0.00 | 0.53 | -6.08 | 167.41 | -39.87 | 107.06 | 0.6691 | 585.0 | 561.3 | |
| 0.00 | 1.32 | 0.00 | 0.88 | -6.19 | 167.24 | -40.04 | 107.14 | 0.6716 | 479.0 | 357.5 | |
| 0.00 | 1.94 | 0.00 | 1.46 | -16.25 | 163.85 | -43.43 | 118.65 | 0.7543 | 658.0 | 549.4 | |
| 0.00 | 0.88 | 0.00 | 0.65 | -14.72 | 164.13 | -43.15 | 116.92 | 0.7441 | 318.0 | 190.3 | |
| 0.00 | 0.71 | 0.00 | 0.53 | -14.84 | 163.75 | -43.52 | 116.88 | 0.7486 | 279.0 | 340.4 | |
| 0.00 | 0.88 | 0.00 | 0.67 | -16.69 | 163.25 | -44.03 | 118.85 | 0.7624 | 468.0 | 401.5 | |
| 0.00 | 0.26 | 0.00 | 0.21 | -13.46 | 159.53 | -47.75 | 113.20 | 0.7854 | -443.0 | -433.7 | |
| 0.00 | 1.59 | 0.00 | 1.22 | -10.13 | 160.07 | -47.20 | 109.37 | 0.7679 | -728.0 | -513.6 | |
| 0.00 | 0.79 | 0.00 | 0.68 | -14.00 | 156.07 | -51.20 | 112.43 | 0.8203 | -479.0 | -379.4 | |
| 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. | |