SDO HMI 2014-06-06 18:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.25 | 0.00 | 13.26 | 4.97 | 264.98 | -16.75 | 69.98 | 0.3023 | -30.4 | -97.8 | |
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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 | 1.54 | 0.00 | 0.77 | 6.09 | 273.95 | -7.78 | 51.71 | 0.1722 | -964.0 | -733.3 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 4.99 | 273.66 | -8.07 | 58.08 | 0.1656 | -892.0 | -664.6 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 5.23 | 273.53 | -8.20 | 57.24 | 0.1697 | -1021.0 | -763.0 | |
| 0.00 | 5.52 | 0.00 | 2.78 | 5.42 | 273.41 | -8.32 | 56.73 | 0.1732 | -663.0 | -555.9 | |
| 0.00 | 0.54 | 0.00 | 0.27 | 4.96 | 271.09 | -10.64 | 64.77 | 0.2043 | -668.0 | -464.3 | |
| 0.00 | 2.80 | 0.00 | 1.42 | 2.22 | 270.07 | -11.67 | 79.09 | 0.2067 | -831.0 | -700.0 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 1.28 | 267.86 | -13.88 | 84.63 | 0.2419 | -880.0 | -701.8 | |
| 0.00 | 1.99 | 0.00 | 1.05 | 1.14 | 261.68 | -20.05 | 86.66 | 0.3448 | 443.0 | 376.7 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 8.13 | 260.26 | -21.47 | 68.65 | 0.3906 | 778.0 | 610.5 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 5.74 | 259.49 | -22.25 | 75.10 | 0.3914 | 674.0 | 492.8 | |
| 0.00 | 1.99 | 0.00 | 1.07 | 3.64 | 258.99 | -22.74 | 80.64 | 0.3926 | 645.0 | 445.3 | |
| 0.00 | 1.27 | 0.00 | 0.71 | 9.40 | 255.63 | -26.10 | 69.36 | 0.4657 | 683.0 | 510.2 | |
| 0.00 | 2.08 | 0.00 | 1.17 | 4.25 | 253.98 | -27.75 | 80.91 | 0.4722 | 818.0 | 611.5 | |
| 0.00 | 0.63 | 0.00 | 0.37 | 8.57 | 251.93 | -29.80 | 73.11 | 0.5156 | 659.0 | 483.7 | |
| 0.00 | 1.18 | 0.00 | 0.70 | 9.41 | 248.85 | -32.88 | 73.01 | 0.5621 | 763.0 | 601.7 | |
| 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. | |