SDO HMI 2014-06-10 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.50 | 0.00 | 10.96 | 3.79 | 255.50 | 19.55 | 281.16 | 0.3384 | 519.0 | 432.4 | |
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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 | 1.45 | 0.00 | 0.90 | 5.30 | 272.68 | 36.73 | 278.25 | 0.6040 | -578.0 | -465.0 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -0.80 | 268.06 | 32.11 | 267.81 | 0.5340 | -665.0 | -529.4 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 2.32 | 263.82 | 27.88 | 274.15 | 0.4703 | 751.0 | 624.6 | |
| 0.00 | 0.91 | 0.00 | 0.51 | 2.05 | 263.82 | 27.87 | 273.57 | 0.4700 | 576.0 | 463.5 | |
| 0.00 | 1.18 | 0.00 | 0.66 | 2.44 | 263.62 | 27.67 | 274.44 | 0.4673 | 680.0 | 599.8 | |
| 0.00 | 1.00 | 0.00 | 0.55 | 6.42 | 261.32 | 25.37 | 283.87 | 0.4404 | 816.0 | 614.4 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 6.39 | 261.08 | 25.13 | 283.92 | 0.4367 | 636.0 | 460.7 | |
| 0.00 | 0.91 | 0.00 | 0.49 | 8.95 | 258.95 | 23.00 | 291.07 | 0.4154 | 639.0 | 413.9 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 8.20 | 253.71 | 17.77 | 294.17 | 0.3325 | 738.0 | 523.1 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 8.69 | 253.60 | 17.66 | 295.66 | 0.3342 | 657.0 | 581.6 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 5.05 | 250.88 | 14.94 | 287.49 | 0.2704 | 783.0 | 570.8 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 1.14 | 246.42 | 10.48 | 273.92 | 0.1830 | 695.0 | 519.3 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 4.34 | 243.70 | 7.76 | 296.90 | 0.1516 | 736.0 | 489.3 | |
| 0.00 | 5.07 | 0.00 | 2.53 | 1.39 | 243.22 | 7.27 | 277.56 | 0.1283 | 802.0 | 729.4 | |
| 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. | |