SDO HMI 2014-08-05 11:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.75 | 0.00 | 7.84 | 6.75 | 210.03 | -1.57 | 204.57 | 0.0822 | -261.9 | -199.6 | |
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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 | 1.18 | 0.00 | 0.58 | 7.43 | 214.81 | 3.20 | 293.22 | 0.0606 | -840.0 | -673.8 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 7.06 | 214.68 | 3.08 | 288.10 | 0.0563 | -973.0 | -764.6 | |
| 0.00 | 1.81 | 0.00 | 0.90 | 7.52 | 214.50 | 2.90 | 296.86 | 0.0564 | -950.0 | -800.5 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 6.91 | 214.41 | 2.80 | 286.93 | 0.0510 | -811.0 | -676.7 | |
| 0.00 | 0.99 | 0.00 | 0.49 | 6.64 | 214.13 | 2.52 | 282.88 | 0.0451 | -830.0 | -560.7 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 6.07 | 213.24 | 1.63 | 269.88 | 0.0285 | -986.0 | -861.5 | |
| 0.00 | 0.99 | 0.00 | 0.49 | 6.16 | 212.63 | 1.02 | 274.98 | 0.0179 | -941.0 | -751.2 | |
| 0.00 | 1.72 | 0.00 | 0.86 | 8.24 | 206.39 | -5.21 | 66.94 | 0.0982 | 903.0 | 630.4 | |
| 0.00 | 2.17 | 0.00 | 1.09 | 7.06 | 203.85 | -7.76 | 82.27 | 0.1359 | 944.0 | 667.0 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 5.38 | 203.04 | -8.57 | 94.23 | 0.1495 | 855.0 | 581.6 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 4.46 | 201.19 | -10.42 | 98.31 | 0.1830 | 748.0 | 521.2 | |
| 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. | |