SDO HMI 2014-08-03 10:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.96 | 0.00 | 8.61 | 15.11 | 258.68 | 20.07 | 300.15 | 0.3840 | 403.7 | 336.5 | |
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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 | 0.91 | 0.00 | 0.53 | 14.04 | 269.94 | 31.33 | 287.13 | 0.5300 | -675.0 | -568.8 | |
| 0.00 | 1.36 | 0.00 | 0.79 | 17.11 | 268.69 | 30.08 | 293.38 | 0.5239 | -668.0 | -583.1 | |
| 0.00 | 1.63 | 0.00 | 0.94 | 15.85 | 268.47 | 29.86 | 291.15 | 0.5156 | -650.0 | -547.0 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 9.25 | 260.78 | 22.17 | 279.95 | 0.3798 | 718.0 | 569.0 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 11.73 | 259.96 | 21.36 | 286.83 | 0.3742 | 771.0 | 606.7 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 9.76 | 258.69 | 20.09 | 282.14 | 0.3478 | 779.0 | 666.8 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 9.52 | 258.58 | 19.98 | 281.51 | 0.3453 | 819.0 | 700.3 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 17.70 | 257.77 | 19.16 | 303.80 | 0.3779 | 702.0 | 536.7 | |
| 0.00 | 1.72 | 0.00 | 0.91 | 14.69 | 256.90 | 18.29 | 297.39 | 0.3434 | 861.0 | 659.5 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 17.66 | 257.09 | 18.48 | 304.59 | 0.3685 | 721.0 | 632.2 | |
| 0.00 | 0.54 | 0.00 | 0.32 | 30.84 | 259.11 | 20.51 | 324.81 | 0.5241 | 678.0 | 615.7 | |
| 0.00 | 2.90 | 0.00 | 1.47 | 17.14 | 243.67 | 5.06 | 336.58 | 0.2131 | 788.0 | 754.1 | |
| 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. | |