SDO HMI 2011-12-04 20:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.90 | 153.81 | 40.44 | 145.99 | 18.91 | 171.75 | 56.60 | 292.12 | 0.8528 | -134.9 | -0.3 | |
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back to the solar disc SDO HMI 2011-12-04 20:58:56 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 | 1.79 | 0.00 | 1.85 | 17.03 | 175.23 | 60.08 | 289.23 | 0.8797 | 435.0 | 327.0 | |
| 11.77 | 59.97 | 12.37 | 63.22 | 18.89 | 175.48 | 60.33 | 291.27 | 0.8841 | -563.3 | -102.1 | |
| 1.36 | -2.00 | 1.43 | -2.00 | 19.18 | 175.27 | 60.12 | 291.63 | 0.8829 | -610.1 | 999999 | |
| 9.21 | 18.00 | 8.93 | 17.41 | 19.03 | 172.63 | 57.48 | 292.00 | 0.8618 | -658.5 | -498.0 | |
| 4.01 | 7.08 | 3.61 | 6.38 | 18.05 | 169.99 | 54.84 | 291.45 | 0.8374 | -601.2 | -390.6 | |
| 0.00 | 1.28 | 0.00 | 1.15 | 18.33 | 169.91 | 54.76 | 291.80 | 0.8372 | -95.0 | -81.1 | |
| 0.00 | 0.94 | 0.00 | 0.83 | 17.68 | 169.23 | 54.08 | 291.20 | 0.8298 | -579.0 | -555.2 | |
| 0.68 | 1.28 | 0.61 | 1.14 | 18.55 | 169.36 | 54.21 | 292.19 | 0.8328 | 230.9 | 64.7 | |
| 0.00 | 0.94 | 0.00 | 0.81 | 18.53 | 167.93 | 52.78 | 292.53 | 0.8196 | 283.0 | 233.6 | |
| 3.07 | 58.52 | 2.64 | 49.87 | 18.94 | 167.80 | 52.65 | 293.04 | 0.8194 | 403.8 | 244.7 | |
| 8.36 | -10.00 | 7.11 | -10.00 | 19.00 | 167.37 | 52.22 | 293.24 | 0.8155 | 732.3 | 999999 | |
| 2.05 | -10.00 | 1.73 | -10.00 | 19.16 | 166.93 | 51.78 | 293.55 | 0.8118 | 769.2 | 999999 | |
| 2.39 | 2.73 | 2.01 | 2.29 | 19.54 | 166.69 | 51.54 | 294.07 | 0.8105 | 703.8 | 651.5 | |
| 0.00 | 1.28 | 0.00 | 1.04 | 20.39 | 164.93 | 49.78 | 295.64 | 0.7962 | 557.0 | 439.5 | |
| 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. | |