Not exact matches
But instead of a momentum distribution of N +
ions, the scientists studied an interference pattern of
photoelectrons that had tunneled from the outer shell of the atom.
The time in which the
photoelectrons are able to fly «back and forth» in a laser field and return for rescattering on the parent
ion is comparable with the length of the optical cycle of the laser (a few femtoseconds).
Ionospheric
photoelectrons can be used as an important diagnostic tool for the topology of the solar wind interaction with both magnetized and unmagnetized objects (Coates et al. 2011), possibly playing a role also in enhancing the
ion escape.
Coates et al. (2015) suggested that the presence of
photoelectrons in the tail, together with low - energy
ions, is possible evidence for a polar wind style escape at Venus, along the draped magnetic field around the planet.
Ionospheres are formed when external radiation, or energetic particles, ionize a neutral molecule, knocking off an orbital electron (which is then called a
photoelectron or a secondary electron) and creating a positive
ion.
As neutrals from the planetary atmospheres are ionized,
ions and
photoelectrons are being generated.
The team used temperature - controlled
photoelectron spectroscopy in EMSL, the DOE's Environmental Molecular Sciences Laboratory on the PNNL campus, to determine how tightly one cyanide
ion and one to three water molecules interact at the very low temperature of -438 °F (12 Kelvin) and again at ambient temperature of 80 °F (equivalent to 300 Kelvin).