SDO HMI 2014-06-09 10:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.21 | 0.00 | 10.98 | 3.66 | 259.51 | 13.07 | 256.81 | 0.2542 | 222.0 | 237.3 | |
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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 | 1.81 | 0.00 | 1.02 | 5.47 | 274.15 | 27.70 | 281.04 | 0.4734 | -780.0 | -679.9 | |
| 0.00 | 1.00 | 0.00 | 0.55 | 4.81 | 272.43 | 25.99 | 280.20 | 0.4456 | -542.0 | -499.1 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 6.56 | 270.86 | 24.42 | 284.85 | 0.4267 | -801.0 | -662.5 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 3.84 | 270.68 | 24.24 | 278.56 | 0.4159 | -653.0 | -566.9 | |
| 0.00 | 1.00 | 0.00 | 0.54 | 1.04 | 270.05 | 23.61 | 271.83 | 0.4024 | -669.0 | -567.5 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 0.25 | 268.17 | 21.73 | 269.85 | 0.3717 | -834.0 | -707.7 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 6.34 | 260.42 | 13.98 | 293.59 | 0.2632 | 802.0 | 684.6 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 5.00 | 259.16 | 12.72 | 290.38 | 0.2351 | 911.0 | 717.5 | |
| 0.00 | 1.45 | 0.00 | 0.73 | -0.11 | 255.70 | 9.26 | 267.28 | 0.1618 | 815.0 | 613.4 | |
| 0.00 | 1.45 | 0.00 | 0.72 | -3.18 | 252.20 | 5.76 | 238.59 | 0.1180 | 832.0 | 615.3 | |
| 0.00 | 3.53 | 0.00 | 1.76 | 5.26 | 250.48 | 4.04 | 320.77 | 0.1114 | 1105.0 | 946.1 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 5.57 | 250.48 | 4.04 | 322.44 | 0.1156 | 916.0 | 763.9 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 6.58 | 244.64 | -1.80 | 16.01 | 0.1138 | 848.0 | 692.3 | |
| 0.00 | 1.54 | 0.00 | 0.76 | 1.13 | 243.06 | -3.38 | 76.77 | 0.0608 | 1158.0 | 979.1 | |
| 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. | |