| | Solar Activity and Hessdalen phenomenon (Site not responding. Last check: 2007-11-05) |
 | | In the first case, it must be reminded that a spike-like morphology in general is commonly detected during solar radio bursts: anyway, in this case spikes are usually observed in a very clustered form (20,21) but not exactly in the form of equidistant spikes all over the frequency band. |
 | | Unfortunately, in both cases, the absence of any recorded radiometric plot at Hessdalen in the 1984 campaign renders very difficult any precise comparison with typical solar radio spikes observed during radio bursts. |
 | | On the contrary, the evidence of further 8 data points (radio spikes of both types) which are not at all coincident with sunspot maximum, suggests that, as in the case of the magnetic phenomenon, some component of the radio phenomenon can be due to the luminous phenomenon. |
| www.ufodatanet.org /report/Hess09_e.htm (1637 words) |