SDO HMI 2014-11-11 01:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.81 | 0.00 | 12.22 | -23.88 | 7.41 | 4.01 | 188.18 | 0.4671 | 442.7 | 484.3 | |
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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 |
| 0.00 | 1.03 | 0.00 | 0.58 | -23.16 | 9.87 | 6.47 | 193.07 | 0.4596 | 669.0 | 623.7 | |
| 0.00 | 1.81 | 0.00 | 1.00 | -21.97 | 9.43 | 6.02 | 192.84 | 0.4399 | 848.0 | 672.0 | |
| 0.00 | 1.55 | 0.00 | 0.86 | -22.23 | 9.37 | 5.97 | 192.59 | 0.4438 | 684.0 | 683.3 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -23.19 | 9.41 | 6.01 | 192.17 | 0.4585 | 868.0 | 662.5 | |
| 0.00 | 0.86 | 0.00 | 0.49 | -24.93 | 9.10 | 5.70 | 190.77 | 0.4838 | 691.0 | 557.6 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -23.49 | 9.04 | 5.63 | 191.29 | 0.4618 | 876.0 | 752.4 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -22.19 | 8.95 | 5.55 | 191.74 | 0.4418 | 657.0 | 483.7 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -23.75 | 8.95 | 5.55 | 191.00 | 0.4656 | 731.0 | 613.2 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -24.22 | 8.94 | 5.54 | 190.77 | 0.4726 | 691.0 | 599.8 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -24.89 | 8.87 | 5.47 | 190.36 | 0.4826 | 649.0 | 507.4 | |
| 0.00 | 7.58 | 0.00 | 4.24 | -23.88 | 8.69 | 5.29 | 190.45 | 0.4668 | 771.0 | 769.5 | |
| 0.00 | 0.86 | 0.00 | 0.49 | -26.57 | 2.69 | -0.71 | 178.73 | 0.5007 | -627.0 | -441.5 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -24.33 | 1.57 | -1.83 | 176.41 | 0.4672 | -640.0 | -489.5 | |
| 0.00 | 1.90 | 0.00 | 1.09 | -26.20 | 357.49 | -5.91 | 169.38 | 0.5034 | -670.0 | -501.0 | |
| 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. | |