SDO HMI 2014-10-02 01:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.44 | 15.66 | 0.26 | 9.34 | -4.71 | 139.38 | -31.60 | 109.05 | 0.5548 | -778.5 | -656.5 | |
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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 |
| 0.44 | 2.20 | 0.26 | 1.30 | -4.39 | 140.14 | -30.84 | 108.97 | 0.5426 | -914.2 | -766.9 | |
| 0.00 | 1.23 | 0.00 | 0.73 | -3.92 | 139.84 | -31.14 | 107.97 | 0.5444 | -782.0 | -656.5 | |
| 0.00 | 1.14 | 0.00 | 0.68 | -4.93 | 139.79 | -31.18 | 109.69 | 0.5501 | -721.0 | -602.1 | |
| 0.00 | 1.67 | 0.00 | 0.99 | -4.11 | 139.73 | -31.25 | 108.24 | 0.5469 | -888.0 | -658.9 | |
| 0.00 | 1.06 | 0.00 | 0.63 | -4.33 | 139.61 | -31.37 | 108.55 | 0.5496 | -776.0 | -677.3 | |
| 0.00 | 1.06 | 0.00 | 0.63 | -6.38 | 139.17 | -31.81 | 111.73 | 0.5660 | -950.0 | -832.6 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -3.99 | 139.13 | -31.85 | 107.69 | 0.5546 | -810.0 | -523.0 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -5.93 | 138.92 | -32.06 | 110.83 | 0.5671 | -828.0 | -697.9 | |
| 0.00 | 1.06 | 0.00 | 0.64 | -6.58 | 138.87 | -32.11 | 111.86 | 0.5711 | -732.0 | -609.5 | |
| 0.00 | 1.32 | 0.00 | 0.79 | -4.12 | 138.99 | -31.99 | 107.83 | 0.5573 | -775.0 | -614.5 | |
| 0.00 | 1.23 | 0.00 | 0.74 | -5.48 | 138.84 | -32.14 | 110.03 | 0.5658 | -765.0 | -675.0 | |
| 0.00 | 1.23 | 0.00 | 0.73 | -3.39 | 138.91 | -32.07 | 106.54 | 0.5550 | -604.0 | -547.7 | |
| 0.00 | 0.35 | 0.00 | 0.21 | -4.14 | 138.70 | -32.28 | 107.70 | 0.5613 | -540.0 | -525.5 | |
| 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. | |