| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 215 | 1016 | 129 | 606 | 18.58 | 32.22 | -30.53 | 60.68 | 0.5537 | 308.8 | -3.9 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-07-05 19:11:31 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | 18.06 | 36.84 | -25.91 | 58.18 | 0.4908 | -650.0 | -494.6 | |
| 0 | 3 | 0 | 2 | 17.00 | 36.91 | -25.84 | 60.09 | 0.4828 | 455.0 | 417.9 | |
| 44 | 425 | 25 | 246 | 19.30 | 35.32 | -27.43 | 57.29 | 0.5187 | 1630.8 | 443.2 | |
| -3 | -3 | -3 | -3 | 18.92 | 35.06 | -27.69 | 58.16 | 0.5195 | 999999 | 999999 | |
| 12 | -3 | 7 | -3 | 18.09 | 34.87 | -27.88 | 59.75 | 0.5165 | 1531.2 | 999999 | |
| 8 | 98 | 5 | 58 | 20.13 | 34.11 | -28.64 | 56.87 | 0.5395 | 1355.2 | 570.5 | |
| 17 | -3 | 10 | -3 | 18.00 | 34.46 | -28.29 | 60.23 | 0.5212 | 1189.9 | 999999 | |
| 4 | -3 | 2 | -3 | 19.26 | 33.99 | -28.76 | 58.42 | 0.5352 | 865.8 | 999999 | |
| 5 | -3 | 3 | -3 | 17.67 | 34.24 | -28.51 | 60.99 | 0.5221 | 618.0 | 999999 | |
| 15 | -6 | 9 | -6 | 20.41 | 33.67 | -29.08 | 56.76 | 0.5468 | 1216.3 | 999999 | |
| 6 | -3 | 4 | -3 | 18.15 | 34.01 | -28.74 | 60.31 | 0.5280 | 259.9 | 999999 | |
| 0 | 3 | 0 | 2 | 19.91 | 33.38 | -29.37 | 57.81 | 0.5470 | 298.0 | 213.6 | |
| 0 | 3 | 0 | 2 | 19.98 | 33.03 | -29.72 | 57.95 | 0.5518 | 303.0 | 297.5 | |
| 0 | 2 | 0 | 1 | 17.91 | 32.90 | -29.84 | 61.50 | 0.5409 | -131.0 | -107.6 | |
| 9 | 27 | 5 | 16 | 19.51 | 32.54 | -30.21 | 59.08 | 0.5549 | -1095.6 | -763.0 | |
| 0 | 6 | 0 | 4 | 20.66 | 32.29 | -30.45 | 57.39 | 0.5652 | 429.0 | 215.2 | |
| 0 | 4 | 0 | 3 | 21.19 | 31.68 | -31.07 | 57.00 | 0.5759 | -776.0 | -562.0 | |
| 8 | 20 | 5 | 12 | 19.78 | 31.75 | -31.00 | 59.20 | 0.5664 | 956.7 | 560.8 | |
| 0 | 5 | 0 | 3 | 20.76 | 31.23 | -31.51 | 57.99 | 0.5786 | 582.0 | 447.1 | |
| 9 | 35 | 5 | 20 | 16.78 | 32.00 | -30.74 | 64.03 | 0.5465 | -1342.5 | -871.0 | |
| 0 | 3 | 0 | 2 | 20.50 | 31.04 | -31.70 | 58.52 | 0.5793 | 690.0 | 641.4 | |
| 3 | 39 | 2 | 23 | 16.93 | 31.30 | -31.45 | 64.21 | 0.5565 | -1379.8 | -974.5 | |
| 0 | 11 | 0 | 7 | 17.94 | 30.91 | -31.84 | 62.75 | 0.5667 | -542.0 | -255.4 | |
| 5 | -22 | 3 | -22 | 16.92 | 31.01 | -31.74 | 64.39 | 0.5602 | -1269.6 | 999999 | |
| 0 | 3 | 0 | 2 | 20.02 | 30.31 | -32.44 | 59.76 | 0.5856 | -442.0 | -340.9 | |
| 5 | 15 | 3 | 9 | 20.08 | 29.54 | -33.21 | 60.15 | 0.5953 | 194.3 | -53.0 | |
| 0 | 8 | 0 | 5 | 16.73 | 30.26 | -32.48 | 65.13 | 0.5691 | -817.0 | -702.4 | |
| 19 | 40 | 12 | 24 | 17.29 | 30.00 | -32.74 | 64.34 | 0.5751 | -1199.6 | -834.9 | |
| 0 | 11 | 0 | 7 | 19.49 | 29.23 | -33.52 | 61.26 | 0.5960 | -640.0 | -581.4 | |
| 0 | 3 | 0 | 2 | 20.68 | 28.73 | -34.02 | 59.72 | 0.6083 | 504.0 | 478.8 | |
| 0 | 8 | 0 | 5 | 19.69 | 28.93 | -33.82 | 61.13 | 0.6007 | -667.0 | -526.4 | |
| 0 | 3 | 0 | 2 | 16.49 | 29.22 | -33.52 | 66.07 | 0.5816 | -825.0 | -739.5 | |
| 31 | 227 | 19 | 140 | 17.92 | 28.93 | -33.82 | 63.92 | 0.5918 | -1386.8 | -466.2 | |
| -33 | -33 | -33 | -33 | 18.40 | 28.62 | -34.13 | 63.32 | 0.5980 | 999999 | 999999 | |
| -33 | -33 | -33 | -33 | 17.98 | 28.46 | -34.29 | 64.06 | 0.5981 | 999999 | 999999 | |
| 15 | -33 | 10 | -33 | 18.34 | 27.97 | -34.77 | 63.76 | 0.6058 | 1000.3 | 999999 | |
| 0 | 9 | 0 | 6 | 16.88 | 27.49 | -35.26 | 66.29 | 0.6056 | -437.0 | -377.5 | |
| 0 | 2 | 0 | 1 | 16.33 | 25.61 | -37.14 | 67.98 | 0.6273 | -594.0 | -461.0 | |
| 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. | |