SDO HMI 2014-06-06 09:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.11 | 0.00 | 10.60 | 4.88 | 262.39 | -24.31 | 77.11 | 0.4155 | -160.2 | -81.8 | |
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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 | 2.26 | 0.00 | 1.16 | 4.95 | 273.52 | -13.18 | 69.09 | 0.2442 | -901.0 | -648.7 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 5.22 | 273.39 | -13.31 | 68.23 | 0.2479 | -957.0 | -819.1 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 3.73 | 272.38 | -14.32 | 75.12 | 0.2565 | -765.0 | -618.6 | |
| 0.00 | 2.17 | 0.00 | 1.12 | 3.67 | 271.65 | -15.04 | 76.01 | 0.2681 | -725.0 | -639.1 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 5.19 | 271.27 | -15.42 | 71.02 | 0.2813 | -856.0 | -630.8 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 2.97 | 270.30 | -16.39 | 79.48 | 0.2879 | -884.0 | -698.8 | |
| 0.00 | 2.08 | 0.00 | 1.08 | 2.39 | 270.09 | -16.61 | 81.58 | 0.2900 | -877.0 | -656.3 | |
| 0.00 | 1.54 | 0.00 | 0.89 | 5.89 | 256.26 | -30.44 | 78.44 | 0.5164 | 656.0 | 517.0 | |
| 0.00 | 1.27 | 0.00 | 0.74 | 1.04 | 254.68 | -32.02 | 87.98 | 0.5325 | 624.0 | 484.4 | |
| 0.00 | 0.81 | 0.00 | 0.48 | 7.39 | 254.32 | -32.38 | 76.33 | 0.5486 | 681.0 | 595.9 | |
| 0.00 | 1.90 | 0.00 | 1.15 | 7.95 | 252.24 | -34.45 | 76.09 | 0.5794 | 693.0 | 616.7 | |
| 0.00 | 1.90 | 0.00 | 1.18 | 4.28 | 249.80 | -36.90 | 82.85 | 0.6056 | 634.0 | 499.6 | |
| 0.00 | 1.09 | 0.00 | 0.70 | 9.53 | 248.27 | -38.43 | 74.85 | 0.6373 | 595.0 | 497.0 | |
| 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. | |