The nitrogen fluorescence induced in air is used to detect ultra-high energy cosmic rays and to measure their energy. The precise knowledge of the absolute fluorescence yield is the key quantity to improve the accuracy on the cosmic ray energy. The total yield has been measured in dry air using a 90Sr source and a [300-430 nm] filter. The fluorescence yield in air is 4.23 ± 0.20 photons per meter when normalized to 760 mmHg, 15°C and with an electron energy of 0.85 MeV. This result is consistent with previous experiments made at various energies, but with an accuracy improved by a factor of about 3. For the first time, the absolute continuous spectrum of nitrogen excited by 90Sr electrons has also been measured with a spectrometer. Details ...
A measurement of the absolute fluorescence yield of the 337 nm nitrogen band, relevant to ultra-high...
For the JEM-EUSO CollaborationThe fluorescence yield is a key ingredient in cosmic ray energy determ...
The fluorescence detection of ultra high energy (> 10^18 eV) cosmic rays requires a detailed knowled...
The nitrogen fluorescence induced in air is used to detect ultra-high energy cosmic rays and to meas...
Most of the Ultra High Energy Cosmic Ray (UHECR) experiments and projects (HiRes, AUGER, TA, EUSO, T...
The study of the energy spectrum of ultra-high energy cosmic rays (E > 1020 eV) requires to determin...
A precise measurement of the energy is essential for the study of ultra-high energy cosmic rays. Bas...
In order to detect ultrahigh-energy cosmic rays (UHECR), atmospheric fluorescence light from the tra...
International audienceDetecting UHECR showers using fluorescence to determine energy requires a prec...
A measurement of the absolute fluorescence yield of the 337 nm nitrogen band, relevant to ultra-high...
For the JEM-EUSO CollaborationThe fluorescence yield is a key ingredient in cosmic ray energy determ...
The fluorescence detection of ultra high energy (> 10^18 eV) cosmic rays requires a detailed knowled...
The nitrogen fluorescence induced in air is used to detect ultra-high energy cosmic rays and to meas...
Most of the Ultra High Energy Cosmic Ray (UHECR) experiments and projects (HiRes, AUGER, TA, EUSO, T...
The study of the energy spectrum of ultra-high energy cosmic rays (E > 1020 eV) requires to determin...
A precise measurement of the energy is essential for the study of ultra-high energy cosmic rays. Bas...
In order to detect ultrahigh-energy cosmic rays (UHECR), atmospheric fluorescence light from the tra...
International audienceDetecting UHECR showers using fluorescence to determine energy requires a prec...
A measurement of the absolute fluorescence yield of the 337 nm nitrogen band, relevant to ultra-high...
For the JEM-EUSO CollaborationThe fluorescence yield is a key ingredient in cosmic ray energy determ...
The fluorescence detection of ultra high energy (> 10^18 eV) cosmic rays requires a detailed knowled...