SDO HMI 2014-07-04 22:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.42 | 0.00 | 8.81 | 5.03 | 261.63 | -7.26 | 175.73 | 0.1682 | 821.3 | 644.0 | |
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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 | 0.72 | 8.85 | 269.89 | 1.00 | 349.97 | 0.0993 | 997.0 | 830.6 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 8.15 | 268.29 | -0.60 | 6.98 | 0.0862 | 762.0 | 536.2 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 11.90 | 268.10 | -0.79 | 5.16 | 0.1513 | 810.0 | 683.1 | |
| 0.00 | 2.54 | 0.00 | 1.26 | 2.76 | 267.80 | -1.09 | 115.11 | 0.0211 | 1022.0 | 790.5 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 12.20 | 266.72 | -2.17 | 13.37 | 0.1604 | 914.0 | 747.6 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 9.46 | 262.16 | -6.73 | 46.92 | 0.1591 | 851.0 | 625.6 | |
| 0.00 | 1.91 | 0.00 | 0.96 | 1.57 | 260.36 | -8.53 | 101.06 | 0.1518 | 961.0 | 774.1 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 7.11 | 259.46 | -9.43 | 67.35 | 0.1769 | 816.0 | 663.5 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -2.86 | 257.12 | -11.77 | 117.38 | 0.2304 | 860.0 | 614.3 | |
| 0.00 | 1.45 | 0.00 | 0.74 | -2.61 | 256.69 | -12.20 | 115.61 | 0.2352 | 627.0 | 442.6 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 3.96 | 250.82 | -18.07 | 87.26 | 0.3111 | 468.0 | 329.1 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 5.84 | 250.39 | -18.50 | 81.39 | 0.3207 | 768.0 | 556.0 | |
| 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. | |