SDO HMI 2011-02-15 11:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.40 | 74.59 | 25.33 | 63.67 | 19.77 | 64.54 | 48.28 | 300.37 | 0.8154 | 191.9 | 245.2 | |
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back to the solar disc SDO HMI 2011-02-15 11:58:57 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 | 0.86 | 0.00 | 0.79 | 17.81 | 68.63 | 52.37 | 296.30 | 0.8433 | 410.0 | 318.6 | |
| 9.86 | 18.34 | 9.19 | 17.17 | 19.02 | 68.85 | 52.59 | 297.56 | 0.8492 | -645.2 | 37.1 | |
| 0.00 | 0.86 | 0.00 | 0.76 | 18.52 | 67.06 | 50.80 | 297.75 | 0.8325 | -685.0 | -517.1 | |
| 0.00 | 1.89 | 0.00 | 1.69 | 19.13 | 67.27 | 51.01 | 298.34 | 0.8365 | -523.0 | -396.1 | |
| 0.00 | 0.86 | 0.00 | 0.74 | 18.97 | 65.29 | 49.03 | 299.04 | 0.8189 | 333.0 | 289.0 | |
| 3.00 | 5.57 | 2.50 | 4.65 | 20.00 | 63.39 | 47.12 | 301.11 | 0.8066 | 523.8 | 458.9 | |
| 7.71 | 39.00 | 6.33 | 32.02 | 19.87 | 62.69 | 46.43 | 301.31 | 0.7998 | 822.8 | 343.6 | |
| 1.97 | 2.23 | 1.68 | 1.90 | 21.89 | 63.47 | 47.21 | 303.17 | 0.8157 | -440.4 | -390.5 | |
| 6.86 | -7.00 | 5.63 | -7.00 | 20.25 | 62.56 | 46.30 | 301.81 | 0.8004 | 767.5 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.70 | 19.94 | 62.03 | 45.77 | 301.73 | 0.7943 | 350.0 | 297.1 | |
| 0.00 | 0.86 | 0.00 | 0.69 | 21.10 | 60.98 | 44.72 | 303.60 | 0.7905 | 505.0 | 445.7 | |
| 0.00 | 0.86 | 0.00 | 0.68 | 20.58 | 60.39 | 44.13 | 303.35 | 0.7826 | 652.0 | 582.3 | |
| 0.00 | 1.03 | 0.00 | 0.81 | 20.62 | 60.05 | 43.79 | 303.58 | 0.7797 | 677.0 | 542.3 | |
| 0.00 | 1.37 | 0.00 | 1.07 | 20.75 | 59.66 | 43.40 | 303.95 | 0.7768 | 700.0 | 525.0 | |
| 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. | |