Observation of the March Maximum in the Daemon Flux from Neos in the Year 2005: New Efforts and New Effects

Details Observation of the March Maximum in the Daemon Flux from Neos in the Year 2005: New Efforts and New Effects Observation of the March Maximum in the Daemon Flux from Neos in the Year 2005: New Efforts and New Effects

2006-05-12

arxiv.org/abs/astro-ph/0605314v1

Astron.Astrophys.Trans.25:43-55,2006

Astronomy and Astrophysics

Astrophysics

14 pages

Scientific paper

10.1080/10556790600682473

The experiments of 2005 aimed at detection of low-velocity (~10-15 km s-1) daemons falling on to the Earth's surface from Near-Earth, Almost Circular Heliocentric Orbits (NEACHOs) have corroborated once more the existence of the March maximum in their flux by raising its confidence level to 99.99%. In addition, these experiments permitted us to identify several FEU-167-1-type PM tubes, with a few times thicker inner Al coating, which appear to be capable to detect, without any scintillator, the crossing of negatively charged daemons. As a result, detection efficiency increases tens of times, thus raising the measured level of the March daemon flux to f > 0.5E-7 cm-2s-1.

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