SDO HMI 2014-07-02 15:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.33 | 0.00 | 11.93 | 7.13 | 268.50 | -30.75 | 81.12 | 0.5088 | 143.6 | 59.9 | |
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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 | 2.72 | 0.00 | 1.44 | 4.73 | 279.41 | -19.83 | 84.42 | 0.3412 | -1115.0 | -824.7 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 4.48 | 279.26 | -19.99 | 85.17 | 0.3435 | -856.0 | -735.9 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 3.78 | 279.24 | -20.00 | 87.22 | 0.3432 | -823.0 | -646.0 | |
| 0.00 | 2.09 | 0.00 | 1.10 | 6.34 | 278.97 | -20.28 | 79.92 | 0.3514 | -812.0 | -630.2 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 5.43 | 275.90 | -23.35 | 83.29 | 0.3989 | -830.0 | -708.5 | |
| 0.00 | 1.27 | 0.00 | 0.73 | 9.00 | 268.66 | -30.59 | 77.50 | 0.5168 | 692.0 | 629.1 | |
| 0.00 | 1.00 | 0.00 | 0.58 | 8.02 | 268.53 | -30.72 | 79.42 | 0.5166 | 794.0 | 707.7 | |
| 0.00 | 0.54 | 0.00 | 0.32 | 9.08 | 268.40 | -30.85 | 77.41 | 0.5208 | 389.0 | 389.0 | |
| 0.00 | 1.09 | 0.00 | 0.65 | 10.70 | 266.70 | -32.55 | 74.98 | 0.5495 | 678.0 | 533.8 | |
| 0.00 | 0.64 | 0.00 | 0.38 | 10.97 | 266.48 | -32.77 | 74.57 | 0.5533 | 585.0 | 581.1 | |
| 0.00 | 1.00 | 0.00 | 0.60 | 11.51 | 265.78 | -33.47 | 73.88 | 0.5646 | 727.0 | 604.0 | |
| 0.00 | 1.63 | 0.00 | 0.99 | 9.06 | 264.16 | -35.08 | 78.57 | 0.5812 | 825.0 | 642.7 | |
| 0.00 | 0.91 | 0.00 | 0.58 | 9.35 | 260.41 | -38.84 | 78.87 | 0.6329 | 687.0 | 591.8 | |
| 0.00 | 1.36 | 0.00 | 0.87 | 8.24 | 260.43 | -38.82 | 80.61 | 0.6311 | 734.0 | 578.9 | |
| 0.00 | 2.18 | 0.00 | 1.61 | 5.07 | 251.12 | -48.12 | 85.89 | 0.7458 | 479.0 | 390.2 | |
| 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. | |