SDO HMI 2014-07-05 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 | 20.26 | 0.00 | 10.60 | -13.54 | 256.13 | -7.26 | 157.63 | 0.3190 | 604.1 | 421.7 | |
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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 | 1.18 | 0.00 | 0.61 | -12.88 | 260.99 | -2.40 | 171.68 | 0.2833 | 815.0 | 514.8 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -12.72 | 259.77 | -3.62 | 167.44 | 0.2844 | 862.0 | 694.3 | |
| 0.00 | 1.18 | 0.00 | 0.61 | -12.72 | 259.30 | -4.09 | 165.87 | 0.2862 | 868.0 | 687.8 | |
| 0.00 | 1.09 | 0.00 | 0.57 | -13.77 | 259.19 | -4.20 | 166.39 | 0.3037 | 747.0 | 620.6 | |
| 0.00 | 1.09 | 0.00 | 0.57 | -12.73 | 257.58 | -5.81 | 160.32 | 0.2947 | 862.0 | 677.5 | |
| 0.00 | 4.00 | 0.00 | 2.09 | -14.19 | 257.51 | -5.88 | 161.72 | 0.3182 | 818.0 | 638.7 | |
| 0.00 | 1.64 | 0.00 | 0.85 | -12.76 | 257.36 | -6.03 | 159.68 | 0.2965 | 882.0 | 720.4 | |
| 0.00 | 0.91 | 0.00 | 0.47 | -13.34 | 256.78 | -6.62 | 158.62 | 0.3089 | 762.0 | 570.3 | |
| 0.00 | 0.82 | 0.00 | 0.42 | -11.74 | 254.46 | -8.93 | 149.62 | 0.3018 | 801.0 | 630.2 | |
| 0.00 | 1.09 | 0.00 | 0.57 | -11.90 | 253.73 | -9.66 | 147.91 | 0.3105 | 805.0 | 554.8 | |
| 0.00 | 1.36 | 0.00 | 0.72 | -13.85 | 252.95 | -10.44 | 149.13 | 0.3444 | 831.0 | 555.5 | |
| 0.00 | 1.00 | 0.00 | 0.53 | -14.65 | 252.82 | -10.58 | 150.00 | 0.3567 | 900.0 | 653.8 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -14.49 | 252.02 | -11.37 | 147.96 | 0.3613 | -585.0 | -396.4 | |
| 0.00 | 2.45 | 0.00 | 1.31 | -14.72 | 251.72 | -11.67 | 147.63 | 0.3670 | -911.0 | -616.3 | |
| 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. | |