SDO HMI 2014-09-05 03:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.80 | 0.00 | 8.20 | 8.47 | 181.41 | 15.10 | 263.45 | 0.2733 | -306.5 | -240.8 | |
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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 | 1.61 | 0.00 | 0.85 | 6.88 | 187.71 | 21.40 | 270.34 | 0.3637 | -733.0 | -615.2 | |
| 0.00 | 2.23 | 0.00 | 1.19 | 11.41 | 187.83 | 21.52 | 282.73 | 0.3703 | -862.0 | -635.4 | |
| 0.00 | 0.80 | 0.00 | 0.43 | 11.63 | 187.06 | 20.75 | 283.68 | 0.3586 | -798.0 | -652.6 | |
| 0.00 | 2.77 | 0.00 | 1.47 | 11.74 | 186.74 | 20.43 | 284.13 | 0.3539 | -693.0 | -648.4 | |
| 0.00 | 0.89 | 0.00 | 0.47 | 11.59 | 186.63 | 20.32 | 283.78 | 0.3517 | -768.0 | -658.8 | |
| 0.00 | 1.34 | 0.00 | 0.71 | 10.67 | 186.20 | 19.89 | 281.34 | 0.3424 | -682.0 | -578.9 | |
| 0.00 | 0.80 | 0.00 | 0.42 | 11.26 | 185.94 | 19.63 | 283.16 | 0.3399 | -672.0 | -569.6 | |
| 0.00 | 0.63 | 0.00 | 0.31 | 11.66 | 171.43 | 5.12 | 311.52 | 0.1172 | 795.0 | 633.4 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 2.86 | 170.95 | 4.64 | 226.73 | 0.1116 | -870.0 | -664.0 | |
| 0.00 | 2.23 | 0.00 | 1.11 | 2.81 | 169.35 | 3.04 | 214.45 | 0.0940 | 1021.0 | 854.7 | |
| 0.00 | 1.70 | 0.00 | 0.84 | 2.54 | 169.10 | 2.79 | 210.74 | 0.0957 | 890.0 | 727.2 | |
| 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. | |