SDO HMI 2014-04-14 19:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.97 | 413.18 | 34.13 | 220.30 | 11.77 | 274.83 | 12.90 | 323.72 | 0.3712 | -917.6 | -356.9 | |
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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 | 0.53 | 0.00 | 0.28 | 8.76 | 279.31 | 17.38 | 309.62 | 0.3849 | -363.0 | -591.0 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 11.82 | 278.11 | 16.18 | 317.38 | 0.4045 | -835.0 | -706.6 | |
| 63.97 | 386.23 | 34.13 | 206.05 | 11.68 | 275.18 | 13.25 | 322.77 | 0.3726 | -1486.9 | -431.4 | |
| 0.00 | 1.59 | 0.00 | 0.84 | 10.02 | 273.57 | 11.64 | 323.46 | 0.3352 | -980.0 | -804.7 | |
| 0.00 | 2.12 | 0.00 | 1.12 | 12.99 | 270.57 | 8.64 | 335.33 | 0.3521 | 729.0 | 681.8 | |
| 0.00 | 5.66 | 0.00 | 2.99 | 13.05 | 270.10 | 8.17 | 336.58 | 0.3498 | 754.0 | 753.0 | |
| 0.00 | 2.03 | 0.00 | 1.08 | 13.49 | 269.59 | 7.66 | 338.39 | 0.3532 | 801.0 | 614.3 | |
| 0.00 | 3.89 | 0.00 | 2.05 | 13.20 | 269.55 | 7.61 | 338.18 | 0.3486 | 864.0 | 814.8 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 12.81 | 268.38 | 6.45 | 340.87 | 0.3359 | 715.0 | 587.4 | |
| 0.00 | 1.94 | 0.00 | 1.03 | 14.49 | 268.09 | 6.16 | 343.19 | 0.3607 | 885.0 | 785.5 | |
| 0.00 | 0.97 | 0.00 | 0.52 | 14.75 | 268.07 | 6.13 | 343.46 | 0.3646 | 682.0 | 563.3 | |
| 0.00 | 1.41 | 0.00 | 0.76 | 17.17 | 267.92 | 5.99 | 345.56 | 0.4017 | 688.0 | 550.2 | |
| 0.00 | 1.24 | 0.00 | 0.65 | 11.72 | 267.61 | 5.68 | 341.98 | 0.3149 | 791.0 | 572.8 | |
| 0.00 | 1.33 | 0.00 | 0.70 | 13.59 | 267.63 | 5.70 | 343.66 | 0.3445 | 782.0 | 713.4 | |
| 0.00 | 2.21 | 0.00 | 1.15 | 11.74 | 266.01 | 4.08 | 346.87 | 0.3081 | 1068.0 | 869.4 | |
| 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. | |