SDO HMI 2014-09-29 05:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.53 | 0.00 | 7.17 | -19.34 | 201.14 | -7.23 | 168.25 | 0.4746 | -280.5 | -183.4 | |
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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 | 0.62 | 0.00 | 0.34 | -17.79 | 214.78 | 6.40 | 194.34 | 0.4307 | 650.0 | 506.6 | |
| 0.00 | 2.21 | 0.00 | 1.21 | -18.21 | 214.47 | 6.10 | 193.44 | 0.4361 | 656.0 | 561.8 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -8.89 | 209.59 | 1.21 | 184.42 | 0.2727 | -928.0 | -780.5 | |
| 0.00 | 1.41 | 0.00 | 0.73 | -8.89 | 209.25 | 0.88 | 183.20 | 0.2723 | -692.0 | -651.6 | |
| 0.00 | 1.32 | 0.00 | 0.79 | -27.13 | 205.95 | -2.42 | 176.14 | 0.5616 | 641.0 | 431.8 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -16.21 | 201.18 | -7.19 | 162.87 | 0.4099 | -743.0 | -562.8 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -14.41 | 200.02 | -8.35 | 158.70 | 0.3888 | -685.0 | -501.9 | |
| 0.00 | 0.62 | 0.00 | 0.41 | -31.93 | 191.74 | -16.63 | 158.66 | 0.6697 | -603.0 | -573.3 | |
| 0.00 | 1.50 | 0.00 | 0.80 | -9.97 | 193.94 | -14.43 | 139.28 | 0.3778 | -814.0 | -661.8 | |
| 0.00 | 1.06 | 0.00 | 0.75 | -33.44 | 186.52 | -21.86 | 154.07 | 0.7128 | -129.0 | -145.6 | |
| 0.00 | 1.15 | 0.00 | 0.74 | -24.26 | 183.29 | -25.08 | 142.63 | 0.6390 | -439.0 | -406.5 | |
| 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. | |