SDO HMI 2014-06-29 03:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.78 | 248.41 | 80.74 | 601.69 | -10.81 | 268.16 | -77.39 | 101.63 | 0.9790 | 245.6 | 143.2 | |
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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 | 1.78 | -11.54 | 272.61 | -72.94 | 102.82 | 0.9618 | -135.0 | -124.1 | |
| 0.00 | 0.64 | 0.00 | 1.89 | -16.87 | 266.39 | -79.16 | 107.60 | 0.9868 | 79.0 | 98.4 | |
| 0.00 | 1.63 | 0.00 | 3.40 | -11.84 | 270.18 | -75.37 | 102.87 | 0.9724 | 312.0 | 282.8 | |
| 0.00 | 3.72 | 0.00 | 8.39 | -12.39 | 269.18 | -76.37 | 103.33 | 0.9765 | -125.0 | -123.2 | |
| 1.54 | 136.15 | 3.12 | 288.03 | -10.57 | 270.53 | -75.01 | 101.61 | 0.9705 | 854.1 | 218.3 | |
| 4.63 | -5.00 | 9.32 | -5.00 | -10.22 | 270.66 | -74.89 | 101.26 | 0.9698 | 909.2 | 999999 | |
| 18.53 | -5.00 | 39.40 | -5.00 | -10.23 | 269.78 | -75.77 | 101.19 | 0.9734 | 324.0 | 999999 | |
| 0.00 | 3.00 | 0.00 | 7.37 | -11.66 | 268.04 | -77.51 | 102.48 | 0.9802 | 80.0 | 36.2 | |
| 0.00 | 1.63 | 0.00 | 3.69 | -10.06 | 268.85 | -76.70 | 100.92 | 0.9769 | -247.0 | -261.7 | |
| 9.26 | 81.29 | 26.69 | 233.23 | -11.74 | 266.20 | -79.35 | 102.40 | 0.9860 | -90.8 | 83.9 | |
| 0.00 | 2.36 | 0.00 | 6.47 | -9.44 | 266.65 | -78.89 | 100.11 | 0.9841 | 81.0 | 56.0 | |
| 0.82 | 16.08 | 2.21 | 44.41 | -9.10 | 266.62 | -78.93 | 99.77 | 0.9841 | 230.3 | 162.6 | |
| 0.00 | 0.91 | 0.00 | 3.03 | -9.56 | 264.73 | -80.81 | 100.09 | 0.9894 | -238.0 | -234.4 | |
| 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. | |