SDO HMI 2011-06-19 07:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.79 | 48.72 | 13.44 | 59.71 | -14.78 | 245.86 | 64.79 | 253.07 | 0.9150 | -66.2 | 152.4 | |
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back to the solar disc SDO HMI 2011-06-19 07:59:11 UT
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 | 0.91 | 0.00 | 1.55 | -14.22 | 253.31 | 72.24 | 254.66 | 0.9585 | 43.0 | 31.0 | |
| 2.36 | 3.27 | 3.93 | 5.45 | -14.84 | 252.68 | 71.61 | 253.95 | 0.9558 | 294.6 | 76.7 | |
| 0.00 | 1.36 | 0.00 | 1.84 | -14.63 | 248.35 | 67.27 | 253.62 | 0.9318 | 181.0 | 132.5 | |
| 0.00 | 1.27 | 0.00 | 1.69 | -14.62 | 248.01 | 66.94 | 253.59 | 0.9297 | 497.0 | 402.9 | |
| 0.00 | 0.36 | 0.00 | 0.48 | -14.30 | 247.82 | 66.75 | 253.90 | 0.9282 | 531.0 | 557.8 | |
| 0.00 | 6.26 | 0.00 | 7.75 | -14.26 | 246.23 | 65.16 | 253.72 | 0.9180 | 751.0 | 624.6 | |
| 0.00 | 2.90 | 0.00 | 3.61 | -14.61 | 246.36 | 65.28 | 253.36 | 0.9191 | 519.0 | 418.7 | |
| 1.81 | 3.63 | 2.15 | 4.32 | -13.86 | 245.20 | 64.13 | 254.00 | 0.9105 | -135.0 | 116.6 | |
| 0.00 | 11.52 | 0.00 | 13.67 | -14.36 | 245.10 | 64.03 | 253.44 | 0.9104 | 345.0 | 284.6 | |
| 0.00 | 1.91 | 0.00 | 2.24 | -13.91 | 244.87 | 63.80 | 253.89 | 0.9083 | -468.0 | -386.3 | |
| 0.00 | 1.45 | 0.00 | 1.68 | -14.19 | 244.44 | 63.37 | 253.52 | 0.9055 | -348.0 | -231.6 | |
| 0.00 | 1.36 | 0.00 | 1.55 | -13.96 | 244.04 | 62.97 | 253.71 | 0.9024 | -425.0 | -331.7 | |
| 0.00 | 1.27 | 0.00 | 1.39 | -15.31 | 242.54 | 61.47 | 251.96 | 0.8930 | -419.0 | -353.9 | |
| 6.62 | 11.25 | 7.36 | 12.49 | -16.31 | 242.86 | 61.79 | 250.92 | 0.8968 | -501.7 | -495.4 | |
| 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. | |