SDO HMI 2014-06-05 12:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.11 | 0.00 | 10.78 | 4.71 | 266.07 | -32.21 | 80.95 | 0.5340 | -531.6 | -358.4 | |
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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 | 1.09 | 0.00 | 0.60 | 4.10 | 273.22 | -25.06 | 80.10 | 0.4307 | -744.0 | -616.0 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 3.86 | 273.03 | -25.25 | 80.72 | 0.4331 | -966.0 | -752.1 | |
| 0.00 | 1.63 | 0.00 | 0.90 | 6.15 | 272.90 | -25.38 | 75.61 | 0.4418 | -833.0 | -683.6 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 3.64 | 272.93 | -25.35 | 81.24 | 0.4341 | -969.0 | -786.0 | |
| 0.00 | 1.09 | 0.00 | 0.60 | 5.90 | 272.71 | -25.57 | 76.25 | 0.4439 | -816.0 | -652.6 | |
| 0.00 | 2.62 | 0.00 | 1.44 | 3.34 | 272.77 | -25.51 | 81.99 | 0.4360 | -907.0 | -782.2 | |
| 0.00 | 0.90 | 0.00 | 0.51 | 3.80 | 270.64 | -27.64 | 81.58 | 0.4698 | -619.0 | -482.3 | |
| 0.00 | 1.54 | 0.00 | 0.86 | 3.19 | 270.35 | -27.93 | 82.94 | 0.4732 | -932.0 | -774.5 | |
| 0.00 | 0.90 | 0.00 | 0.53 | 0.25 | 266.78 | -31.50 | 89.29 | 0.5246 | -669.0 | -544.9 | |
| 0.00 | 1.00 | 0.00 | 0.59 | 1.68 | 265.33 | -32.96 | 86.69 | 0.5468 | -554.0 | -527.3 | |
| 0.00 | 2.26 | 0.00 | 1.49 | 5.30 | 257.48 | -40.80 | 81.76 | 0.6597 | 264.0 | 330.0 | |
| 0.00 | 1.54 | 0.00 | 1.08 | 7.09 | 253.88 | -44.40 | 79.78 | 0.7078 | 426.0 | 420.2 | |
| 0.00 | 1.00 | 0.00 | 0.78 | 9.97 | 248.47 | -49.82 | 76.93 | 0.7747 | 408.0 | 367.5 | |
| 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. | |