Selection | Block A | Block B | Both Blocks | ||||
Criteria | No. pixels | % of total | No. pixels | % of total | No. pixels | % of A | % of B |
1700Å | |||||||
LLO | 64 | 1 | 103 | 2 | 0 | - | - |
2-3 cycles | 4857 | 81 | 4611 | 77 | 3754 | 77 | 81 |
230-280 s & 2-3 cycles | 2090 | 35 | 2215 | 37 | 818 | 39 | 37 |
230-280 s | 3868 | 64 | 4138 | 69 | 2709 | 65 | 70 |
1600Å | |||||||
LLO | 142 | 2 | 93 | 2 | 2 | 1 | 2 |
2-3 cycles | 4637 | 77 | 4913 | 82 | 3812 | 82 | 78 |
230-280 s& 2-3 cycles | 2430 | 41 | 2337 | 39 | 961 | 40 | 41 |
230-280 s | 4587 | 76 | 4465 | 74 | 3429 | 75 | 77 |
1216Å | |||||||
LLO | 134 | 2 | 123 | 2 | 4 | 3 | 3 |
2-3 cycles | 5173 | 86 | 5126 | 85 | 4370 | 85 | 84 |
230-280 s& 2-3 cycles | 2537 | 42 | 2440 | 41 | 1024 | 40 | 41 |
230-280 s | 4727 | 79 | 4515 | 75 | 3584 | 76 | 79 |
1550Å | |||||||
LLO | 131 | 2 | 50 | 1 | 0 | - | - |
2-3 cycles | 4704 | 78 | 3516 | 59 | 2085 | 44 | 59 |
230-280 s& 2-3 cycles | 2470 | 41 | 1591 | 27 | 679 | 27 | 43 |
230-280 s | 4560 | 76 | 3051 | 51 | 2324 | 51 | 76 |
By comparing how many pixels in block A of each wavelength display a similar behaviour in block B, it is possible to study whether oscillations of specific period and lifetime occur repeatedly (Table 6.2). At each wavelength all network pixels displaying periodicity between 230-280 s in block A were selected and compared to network pixels containing periodicity in the same range in block B. This showed a recurrence rate of ~65-75% in all four UV passbands. This was also carried out for all network pixels displaying oscillations lasting 2-3 cycles at all periods (where the corresponding value was ~75-85%). A study of all network pixels lasting 2-3 cycles and in the range 230-280 s (i.e., at the peak value in the lifetime-period plots), showed ~40% common pixels. As these oscillations are the most frequent, a 40% chance of a recurrence at the same position represents a good candidate for repeated heating of the surrounding plasma.
Selection | Block A | Block B | Both Blocks | ||||
Criteria | No. pixels | % of total | No. pixels | % of total | No. pixels | % of A | % of B |
1700Å | |||||||
LLO | 642 | 2 | 613 | 2 | 15 | 1 | 1 |
2-3 cycles | 24370 | 85 | 26427 | 92 | 22420 | 85 | 92 |
230-280 s & 2-3 cycles | 13709 | 48 | 14518 | 51 | 6990 | 51 | 48 |
230-280 s | 23871 | 83 | 25084 | 87 | 20866 | 87 | 83 |
1600Å | |||||||
LLO | 618 | 2 | 716 | 2 | 18 | 1 | 1 |
2-3 cycles | 24078 | 83 | 26220 | 91 | 21994 | 91 | 84 |
230-280 s & 2-3 cycles | 13240 | 46 | 13826 | 48 | 6337 | 48 | 46 |
230-280 s | 23380 | 81 | 24640 | 86 | 20059 | 86 | 81 |
1216Å | |||||||
LLO | 777 | 3 | 836 | 3 | 19 | 1 | 1 |
2-3 cycles | 26421 | 92 | 26334 | 92 | 24248 | 92 | 92 |
230-280 s & 2-3 cycles | 14499 | 50 | 14594 | 51 | 7418 | 51 | 51 |
230-280 s | 25355 | 88 | 25318 | 88 | 22364 | 88 | 88 |
1550Å | |||||||
LLO | 462 | 2 | 161 | 1 | 2 | 1 | 1 |
2-3 cycles | 23675 | 82 | 15763 | 55 | 12985 | 55 | 82 |
230-280 s & 2-3 cycles | 12592 | 44 | 8128 | 28 | 3564 | 28 | 44 |
230-280 s | 22245 | 77 | 14764 | 51 | 11457 | 52 | 78 |
In the internetwork, the fraction of pixels showing oscillations recurring in the same location was generally 5-10% higher than in the network (Table 6.3). The internetwork oscillations lasting 2-3 cycles and in the range 230-280 s (with a ~50% recurrence rate) may be the persistent flashers first identified by Brandt et al. (1992). However their studies suggest grains which are persistent flashers should be 5-10 times less likely to occur than normal K2V grains, which in turn suggests a recurrence rate of ~10-17%. The higher value of 50% obtained in these data could be due to the internetwork mask preferentially containing persistent flashers rather than normal internetwork grains.