SDO HMI 2014-07-07 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 | 15.62 | 0.00 | 8.44 | 6.43 | 261.14 | 22.57 | 277.75 | 0.3865 | 727.2 | 611.6 | |
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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 | 2.18 | 0.00 | 1.26 | 9.13 | 268.91 | 30.34 | 282.00 | 0.5119 | 599.0 | 415.8 | |
| 0.00 | 0.82 | 0.00 | 0.45 | 6.35 | 263.52 | 24.96 | 277.47 | 0.4247 | 692.0 | 562.3 | |
| 0.00 | 1.00 | 0.00 | 0.55 | 9.58 | 263.16 | 24.59 | 285.12 | 0.4269 | 612.0 | 495.9 | |
| 0.00 | 1.64 | 0.00 | 0.89 | 6.47 | 262.58 | 24.02 | 277.97 | 0.4101 | 828.0 | 699.3 | |
| 0.00 | 2.54 | 0.00 | 1.36 | 6.36 | 260.71 | 22.14 | 278.20 | 0.3801 | 823.0 | 745.8 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 5.61 | 260.54 | 21.98 | 276.23 | 0.3763 | 743.0 | 624.2 | |
| 0.00 | 0.45 | 0.00 | 0.24 | 1.13 | 260.40 | 21.83 | 264.24 | 0.3753 | 521.0 | 449.2 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 5.76 | 260.42 | 21.85 | 276.68 | 0.3745 | 785.0 | 684.7 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 5.49 | 260.24 | 21.68 | 275.99 | 0.3713 | 781.0 | 590.6 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 8.14 | 259.25 | 20.68 | 283.56 | 0.3612 | 809.0 | 699.1 | |
| 0.00 | 0.64 | 0.00 | 0.33 | 4.26 | 253.53 | 14.96 | 273.28 | 0.2591 | 753.0 | 560.0 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 3.74 | 251.57 | 13.00 | 271.33 | 0.2256 | 781.0 | 670.0 | |
| 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. | |