SDO HMI 2014-08-02 08:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.49 | 0.00 | 10.85 | 12.55 | 254.79 | 1.87 | 299.49 | 0.1688 | 818.5 | 619.1 | |
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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 | 1.00 | 0.00 | 0.50 | 9.42 | 259.25 | 6.32 | 299.93 | 0.1260 | 880.0 | 703.4 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 10.15 | 258.99 | 6.06 | 305.94 | 0.1289 | 1001.0 | 817.1 | |
| 0.00 | 2.54 | 0.00 | 1.28 | 16.48 | 258.93 | 6.01 | 331.49 | 0.2111 | 745.0 | 572.6 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 9.88 | 258.76 | 5.84 | 305.15 | 0.1231 | 968.0 | 691.5 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 15.71 | 258.37 | 5.44 | 331.97 | 0.1951 | 740.0 | 571.5 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 9.46 | 258.17 | 5.24 | 305.02 | 0.1105 | 892.0 | 708.1 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 8.13 | 257.59 | 4.66 | 296.29 | 0.0902 | 744.0 | 521.4 | |
| 0.00 | 1.81 | 0.00 | 0.92 | 17.99 | 257.38 | 4.45 | 340.65 | 0.2238 | 472.0 | 429.4 | |
| 0.00 | 2.08 | 0.00 | 1.04 | 3.36 | 256.93 | 4.01 | 238.02 | 0.0826 | 976.0 | 704.7 | |
| 0.00 | 1.45 | 0.00 | 0.72 | 4.00 | 255.69 | 2.76 | 236.00 | 0.0582 | 928.0 | 762.2 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 5.38 | 254.59 | 1.67 | 253.67 | 0.0303 | 918.0 | 657.1 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 20.19 | 249.00 | -3.92 | 14.54 | 0.2569 | 786.0 | 570.0 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 23.14 | 243.96 | -8.96 | 25.67 | 0.3322 | 793.0 | 597.6 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 17.22 | 243.07 | -9.86 | 39.51 | 0.2582 | 744.0 | 507.6 | |
| 0.00 | 0.91 | 0.00 | 0.49 | 22.35 | 236.18 | -16.75 | 42.81 | 0.3938 | 690.0 | 482.6 | |
| 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. | |