Not exact matches
When comets approach the Sun, these
ices heat up, eventually turning to gases that jet out into space together with dusty material to form a head or coma around the cometary
nucleus.
Circling the South Pole, ANITA's antennas will scan a million cubic kilometers of
ice at a time, looking for the telltale radio waves emitted
when an ultrahigh - energy neutrino hits a
nucleus in
ice.
Researchers from the IceCube project will place a string of Digital Optical Modules into this hole, which can detect the faint signal produced on the rare occasion
when a neutrino collides directly with the
nucleus of an atom in a molecule of
ice.
When a neutrino collides with an atomic
nucleus, a new particle called a muon is produced, which emits a faint blue glow in the transparent
ice that the DOMs can detect.
ANITA will exploit a phenomenon known as the Askaryan effect, whereby high - energy neutrinos streaming through
ice, salt or sand produce a cone of radio waves
when they collide with a
nucleus in the material.
When comets venture into the more intense sunlight of the inner solar system, the
ices on the comet
nucleus begin to melt and fall away.
Usually
when comets approach the sun, their
ices erupt from the
nucleus, creating a gaseous coma and tails.
Including aggregation, in addition to quadrupled
ice nucleus concentrations aloft or an
ice nucleus reservoir below, allowed the simulations to roughly match the in situ properties
when assuming the presence of low - density dendrites and their aggregates (Fig. 2).
When endothermic reacting (toxic)
ice nucleating materials are utilized on a massive scale for climate intervention / modification programs, convection is greatly impacted, too many condensation
nuclei are present, and precipitation is generally greatly reduced (from what it would have otherwise been) in the core of the engineered chemical cool - down zones.