SOHO MDI 2000-09-04 06:23:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 173 | 959 | 90 | 494 | 13.36 | 357.57 | 14.82 | 295.38 | 0.2748 | 725.3 | 268.1 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-09-04 06:23:31 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 2 | 11.61 | 2.68 | 19.93 | 284.05 | 0.3456 | 823.0 | 646.1 | |
| 15 | 81 | 8 | 43 | 12.88 | 2.48 | 19.73 | 287.77 | 0.3471 | 1426.5 | 748.7 | |
| 0 | 6 | 0 | 3 | 13.95 | 2.44 | 19.69 | 290.76 | 0.3512 | 791.0 | 654.1 | |
| 6 | -2 | 3 | -2 | 12.94 | 2.14 | 19.39 | 288.16 | 0.3420 | 1635.9 | 999999 | |
| 0 | 6 | 0 | 3 | 11.64 | 2.04 | 19.29 | 284.48 | 0.3357 | 777.0 | 514.7 | |
| 0 | 14 | 0 | 7 | 13.71 | 1.57 | 18.81 | 290.82 | 0.3367 | 884.0 | 835.4 | |
| 0 | 5 | 0 | 2 | 15.91 | 1.08 | 18.32 | 297.41 | 0.3421 | 759.0 | 541.4 | |
| 48 | 556 | 25 | 288 | 13.69 | 0.08 | 17.33 | 292.15 | 0.3138 | 1985.5 | 669.6 | |
| 9 | -8 | 4 | -8 | 13.22 | 359.96 | 17.21 | 290.83 | 0.3095 | 1285.8 | 999999 | |
| 7 | -8 | 4 | -8 | 12.71 | 359.88 | 17.13 | 289.31 | 0.3058 | 821.9 | 999999 | |
| -8 | -8 | -8 | -8 | 14.01 | 359.89 | 17.14 | 293.32 | 0.3127 | 999999 | 999999 | |
| 5 | -8 | 3 | -8 | 12.68 | 359.58 | 16.83 | 289.49 | 0.3010 | 516.8 | 999999 | |
| -8 | -8 | -8 | -8 | 13.71 | 359.53 | 16.78 | 292.78 | 0.3055 | 999999 | 999999 | |
| 13 | -8 | 7 | -8 | 12.88 | 358.38 | 15.63 | 291.36 | 0.2833 | 1350.2 | 999999 | |
| 0 | 8 | 0 | 4 | 13.96 | 357.95 | 15.20 | 295.47 | 0.2831 | 727.0 | 582.6 | |
| 0 | 8 | 0 | 4 | 12.15 | 357.84 | 15.08 | 289.42 | 0.2710 | 885.0 | 715.5 | |
| 14 | -8 | 7 | -8 | 13.41 | 357.83 | 15.08 | 293.80 | 0.2778 | 1525.4 | 999999 | |
| 9 | -8 | 5 | -8 | 13.06 | 357.77 | 15.01 | 292.68 | 0.2747 | 1753.3 | 999999 | |
| 0 | 9 | 0 | 4 | 12.07 | 356.67 | 13.92 | 290.43 | 0.2522 | -650.0 | -472.9 | |
| 0 | 6 | 0 | 3 | 14.90 | 356.84 | 14.09 | 300.20 | 0.2734 | -571.0 | -423.1 | |
| 0 | 5 | 0 | 2 | 13.98 | 354.46 | 11.71 | 301.32 | 0.2315 | -470.0 | -357.2 | |
| 0 | 5 | 0 | 3 | 12.96 | 354.33 | 11.58 | 297.55 | 0.2216 | -675.0 | -542.1 | |
| 0 | 6 | 0 | 3 | 12.65 | 353.90 | 11.15 | 297.09 | 0.2129 | -792.0 | -652.6 | |
| 13 | 45 | 6 | 23 | 13.53 | 353.33 | 10.58 | 302.02 | 0.2114 | -1389.5 | -714.1 | |
| 0 | 3 | 0 | 2 | 12.91 | 353.06 | 10.30 | 300.00 | 0.2022 | -456.0 | -368.9 | |
| 0 | 7 | 0 | 4 | 13.04 | 352.61 | 9.86 | 301.62 | 0.1968 | -1134.0 | -923.2 | |
| 0 | 29 | 0 | 15 | 13.75 | 352.56 | 9.81 | 304.81 | 0.2024 | -736.0 | -730.1 | |
| 4 | 103 | 2 | 52 | 12.85 | 352.03 | 9.28 | 302.27 | 0.1868 | -1211.7 | -941.7 | |
| 0 | 9 | 0 | 4 | 14.23 | 351.97 | 9.21 | 308.45 | 0.1991 | -909.0 | -899.6 | |
| 0 | 9 | 0 | 5 | 13.65 | 351.78 | 9.02 | 306.54 | 0.1906 | -971.0 | -846.0 | |
| 0 | 15 | 0 | 7 | 14.36 | 351.60 | 8.85 | 310.05 | 0.1956 | -1082.0 | -835.3 | |
| 5 | -28 | 3 | -28 | 13.06 | 351.51 | 8.76 | 304.70 | 0.1812 | -1352.5 | 999999 | |
| 17 | -28 | 9 | -28 | 13.26 | 351.07 | 8.32 | 307.00 | 0.1771 | -1619.5 | 999999 | |
| -33 | -28 | -33 | -28 | 13.23 | 350.74 | 7.99 | 307.92 | 0.1723 | 999999 | 999999 | |
| 8 | -28 | 4 | -28 | 13.12 | 350.50 | 7.74 | 308.23 | 0.1678 | -1457.5 | 999999 | |
| 0 | 5 | 0 | 3 | 15.29 | 350.24 | 7.49 | 318.28 | 0.1898 | -700.0 | -601.3 | |
| 0 | 4 | 0 | 2 | 14.63 | 349.85 | 7.10 | 317.25 | 0.1770 | -569.0 | -648.3 | |
| 0 | 5 | 0 | 3 | 14.24 | 349.43 | 6.68 | 317.39 | 0.1673 | -869.0 | -801.8 | |
| 0 | 5 | 0 | 3 | 13.41 | 349.17 | 6.41 | 314.88 | 0.1540 | -771.0 | -693.1 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |