CR-39 PNTDs are commonly used as the heavy ion detectors with the LET detection threshold of > ~5 keV/um in water. In the space utilization field, CR-39 PNTDs onboard the International Space Station (ISS) are used as the space radiation dosimeter to measure precisely LET distribution of cosmic rays and also CR-39 is a promising candidate detector for the precise observation of trans-iron nuclei in galactic cosmic rays (GCRs). However, due to the high sensitivity of CR-39 detector, a single track of ultra heavy trans-iron nuclei will not be discernible among the numerous background tracks produced by lighter nuclei such as CNO group and Fe in GCRs. Moreover, the detector response will be saturated in higher LET (i.e. trans-iron nuclei) regio...
We studied the track response of CR-39 plastic nuclear track detectors (PNTD) for low (100 MeV/n) en...
The occurrence of saturation in the CR-39 detector reduces and limits its detection dynamic range; n...
Observation of trans-iron nuclei in galactic cosmic rays (Z>30) requires a high performance cosmic r...
We verified that the two-step etching method of the combination of pre-etching with PEW (Potassium h...
It is necessary to develop a track detector with higher detection threshold and high charge resoluti...
The two-step etching method using PEW (Potassium hydroxide + Ethanol + Water) and NaOH solutions was...
The chemical compositions of ultra heavy (UH, Z ³ 30) nuclei in galactic cosmic rays (GCRs) cou...
Charge identification of trans-iron nuclei (nuclear charge: Z≥ 30) using CR-39 plastic nuclear track...
Charge identification of trans-iron nuclei (nuclear charge: Z>=30) using CR-39 plastic nuclear track...
none13Several improvements were made for Nuclear Track Detectors (NTDs) used for environmental studi...
In the Indian cosmic ray experiment (IONS) in Spacelab-3 the intention is to study nuclei up to iron...
We report here the first successful detection of highly relativistic cosmic ray iron group nuclei in...
Several improvements were made for Nuclear Track Detectors (NTDs) used for environmental studies and...
We have studied the performance of a newly-commercialized CR-39 plastic nuclear track detector (PNTD...
A time-efficient surface grinding and polishing procedure was developed to remove noise pitting asso...
We studied the track response of CR-39 plastic nuclear track detectors (PNTD) for low (100 MeV/n) en...
The occurrence of saturation in the CR-39 detector reduces and limits its detection dynamic range; n...
Observation of trans-iron nuclei in galactic cosmic rays (Z>30) requires a high performance cosmic r...
We verified that the two-step etching method of the combination of pre-etching with PEW (Potassium h...
It is necessary to develop a track detector with higher detection threshold and high charge resoluti...
The two-step etching method using PEW (Potassium hydroxide + Ethanol + Water) and NaOH solutions was...
The chemical compositions of ultra heavy (UH, Z ³ 30) nuclei in galactic cosmic rays (GCRs) cou...
Charge identification of trans-iron nuclei (nuclear charge: Z≥ 30) using CR-39 plastic nuclear track...
Charge identification of trans-iron nuclei (nuclear charge: Z>=30) using CR-39 plastic nuclear track...
none13Several improvements were made for Nuclear Track Detectors (NTDs) used for environmental studi...
In the Indian cosmic ray experiment (IONS) in Spacelab-3 the intention is to study nuclei up to iron...
We report here the first successful detection of highly relativistic cosmic ray iron group nuclei in...
Several improvements were made for Nuclear Track Detectors (NTDs) used for environmental studies and...
We have studied the performance of a newly-commercialized CR-39 plastic nuclear track detector (PNTD...
A time-efficient surface grinding and polishing procedure was developed to remove noise pitting asso...
We studied the track response of CR-39 plastic nuclear track detectors (PNTD) for low (100 MeV/n) en...
The occurrence of saturation in the CR-39 detector reduces and limits its detection dynamic range; n...
Observation of trans-iron nuclei in galactic cosmic rays (Z>30) requires a high performance cosmic r...