SDO HMI 2014-04-16 06:00:34 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 107.92 | 607.87 | 54.45 | 306.67 | 4.33 | 246.43 | 3.76 | 340.14 | 0.1897 | -438.3 | -217.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-04-16 06:00:34 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 | 1.06 | 0.00 | 0.54 | 5.50 | 250.94 | 8.27 | 323.03 | 0.2392 | -941.0 | -733.5 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 1.07 | 249.35 | 6.68 | 314.46 | 0.1637 | -902.0 | -693.7 | |
| 48.24 | 450.93 | 24.39 | 227.80 | 4.61 | 248.13 | 5.46 | 331.62 | 0.2005 | -1511.4 | -403.1 | |
| 3.28 | -3.00 | 1.65 | -3.00 | 4.00 | 248.03 | 5.37 | 330.53 | 0.1905 | -1305.4 | 999999 | |
| 31.96 | -3.00 | 16.13 | -3.00 | 4.30 | 247.58 | 4.91 | 333.37 | 0.1914 | -1581.7 | 999999 | |
| 0.89 | -3.00 | 0.45 | -3.00 | 4.98 | 247.58 | 4.92 | 334.84 | 0.2019 | -862.0 | 999999 | |
| 0.00 | 3.63 | 0.00 | 1.82 | 2.86 | 245.73 | 3.06 | 339.89 | 0.1559 | -773.0 | -819.7 | |
| 6.46 | 17.97 | 3.25 | 9.03 | 3.99 | 245.49 | 2.83 | 343.41 | 0.1731 | -1101.2 | -964.8 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 4.90 | 245.47 | 2.80 | 344.94 | 0.1882 | 587.0 | 457.1 | |
| 0.00 | 1.33 | 0.00 | 0.67 | 3.56 | 245.40 | 2.73 | 343.21 | 0.1656 | -1201.0 | -1028.6 | |
| 0.00 | 1.50 | 0.00 | 0.75 | 2.25 | 245.00 | 2.34 | 343.23 | 0.1419 | -861.0 | -604.4 | |
| 0.00 | 3.36 | 0.00 | 1.69 | 4.11 | 245.01 | 2.34 | 346.29 | 0.1729 | -860.0 | -780.1 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 3.35 | 244.70 | 2.04 | 347.02 | 0.1589 | -766.0 | -566.0 | |
| 0.00 | 5.13 | 0.00 | 2.58 | 3.68 | 244.68 | 2.01 | 347.65 | 0.1644 | -760.0 | -785.5 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 3.50 | 244.52 | 1.86 | 348.33 | 0.1608 | -767.0 | -506.8 | |
| 0.00 | 2.57 | 0.00 | 1.29 | 4.47 | 244.38 | 1.71 | 350.26 | 0.1769 | -955.0 | -819.3 | |
| 0.00 | 1.86 | 0.00 | 0.93 | 4.26 | 244.29 | 1.62 | 350.58 | 0.1730 | -865.0 | -692.6 | |
| 0.00 | 1.95 | 0.00 | 0.98 | 3.47 | 243.59 | 0.92 | 354.11 | 0.1578 | 902.0 | 693.9 | |
| 0.00 | 1.50 | 0.00 | 0.75 | 2.92 | 243.59 | 0.92 | 353.74 | 0.1484 | -911.0 | -692.3 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 3.19 | 243.47 | 0.80 | 354.72 | 0.1529 | 709.0 | 515.6 | |
| 0.00 | 1.95 | 0.00 | 0.98 | 4.04 | 243.29 | 0.62 | 356.26 | 0.1674 | 886.0 | 612.5 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 3.98 | 242.57 | -0.10 | 0.60 | 0.1660 | 763.0 | 634.9 | |
| 0.00 | 1.42 | 0.00 | 0.71 | 4.35 | 242.57 | -0.10 | 0.57 | 0.1723 | 702.0 | 445.2 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 3.25 | 242.41 | -0.25 | 1.64 | 0.1534 | -777.0 | -579.9 | |
| 0.00 | 1.33 | 0.00 | 0.67 | 3.95 | 242.32 | -0.34 | 2.06 | 0.1655 | 838.0 | 654.8 | |
| 0.44 | 1.33 | 0.22 | 0.67 | 3.10 | 242.02 | -0.64 | 4.27 | 0.1511 | 1060.8 | 943.3 | |
| 3.54 | 13.81 | 1.78 | 6.95 | 4.41 | 241.99 | -0.67 | 3.88 | 0.1738 | 1016.7 | 735.8 | |
| 0.00 | 1.42 | 0.00 | 0.71 | 3.32 | 241.96 | -0.70 | 4.55 | 0.1549 | 284.0 | 316.4 | |
| 0.80 | 3.45 | 0.40 | 1.73 | 3.65 | 241.84 | -0.82 | 5.14 | 0.1608 | 619.9 | 320.7 | |
| 0.00 | 2.74 | 0.00 | 1.37 | 2.52 | 241.84 | -0.82 | 5.85 | 0.1414 | 878.0 | 620.3 | |
| 0.00 | 2.21 | 0.00 | 1.11 | 3.41 | 241.69 | -0.97 | 6.24 | 0.1569 | 953.0 | 796.2 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 2.53 | 241.54 | -1.12 | 7.97 | 0.1420 | 902.0 | 746.2 | |
| 1.15 | 5.05 | 0.58 | 2.53 | 3.50 | 241.39 | -1.28 | 8.06 | 0.1591 | 1207.0 | 834.8 | |
| 8.59 | 30.01 | 4.31 | 15.08 | 4.05 | 241.27 | -1.40 | 8.31 | 0.1688 | 1269.7 | 764.1 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 5.33 | 241.15 | -1.52 | 7.97 | 0.1910 | 713.0 | 549.7 | |
| 0.80 | 2.12 | 0.40 | 1.07 | 3.71 | 241.06 | -1.61 | 9.89 | 0.1637 | 1173.7 | 986.8 | |
| 0.00 | 1.59 | 0.00 | 0.80 | 3.04 | 240.94 | -1.73 | 11.42 | 0.1527 | 1006.0 | 874.7 | |
| 1.24 | -34.00 | 0.62 | -34.00 | 4.17 | 240.88 | -1.79 | 10.47 | 0.1720 | 1107.8 | 999999 | |
| 0.00 | 5.31 | 0.00 | 2.67 | 4.45 | 240.79 | -1.88 | 10.69 | 0.1770 | 464.0 | 663.3 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 2.56 | 240.79 | -1.88 | 13.11 | 0.1450 | 690.0 | 524.4 | |
| 0.00 | 4.69 | 0.00 | 2.35 | 2.16 | 240.73 | -1.94 | 14.18 | 0.1386 | 742.0 | 767.6 | |
| 0.00 | 2.04 | 0.00 | 1.02 | 4.11 | 240.58 | -2.09 | 12.26 | 0.1720 | 833.0 | 709.2 | |
| 0.00 | 1.95 | 0.00 | 0.97 | 2.01 | 240.58 | -2.09 | 15.52 | 0.1367 | 1013.0 | 777.0 | |
| 0.00 | 1.50 | 0.00 | 0.75 | 1.89 | 240.09 | -2.57 | 19.15 | 0.1372 | 732.0 | 574.9 | |
| 0.00 | 1.33 | 0.00 | 0.67 | 5.19 | 239.64 | -3.03 | 15.82 | 0.1939 | 790.0 | 621.0 | |
| 0.00 | 2.83 | 0.00 | 1.43 | 4.27 | 239.28 | -3.39 | 19.12 | 0.1808 | 1184.0 | 976.3 | |
| 0.00 | 1.59 | 0.00 | 0.80 | 4.12 | 238.76 | -3.90 | 22.07 | 0.1814 | 935.0 | 779.8 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 5.29 | 238.76 | -3.91 | 19.91 | 0.2002 | 688.0 | 580.7 | |
| 0.53 | 5.05 | 0.27 | 2.54 | 4.10 | 238.55 | -4.11 | 23.21 | 0.1824 | 1217.7 | 950.0 | |
| 0.00 | 3.01 | 0.00 | 1.52 | 4.01 | 238.34 | -4.32 | 24.47 | 0.1824 | 1110.0 | 964.6 | |
| 0.00 | 1.42 | 0.00 | 0.72 | 6.52 | 237.87 | -4.79 | 21.73 | 0.2253 | 762.0 | 531.9 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 6.40 | 237.87 | -4.79 | 21.93 | 0.2234 | 838.0 | 591.5 | |
| 0.00 | 2.39 | 0.00 | 1.22 | 6.55 | 237.63 | -5.04 | 22.67 | 0.2274 | 811.0 | 664.1 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 3.56 | 237.59 | -5.08 | 29.30 | 0.1814 | 931.0 | 713.6 | |
| 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. | |