1954
DOI: 10.1103/physrev.96.643
|View full text |Cite
|
Sign up to set email alerts
|

Ionization Produced by 5-Mev Alpha Particles in Argon Mixtures

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

0
13
0
1

Year Published

1960
1960
2001
2001

Publication Types

Select...
6
2
1

Relationship

0
9

Authors

Journals

citations
Cited by 78 publications
(14 citation statements)
references
References 6 publications
0
13
0
1
Order By: Relevance
“…This is the case for the Penning ionization ͑PI͒ and hetero-nuclear associative ionization ͑AI͒ mechanisms involving the Ne 1s and dimer states. [26][27][28][29][30][31][32][33][34][35][36][37][38][39][40][41] Table I is a list of the PI and AI mechanisms and related processes affecting the population of the relevant excited species, together with the rate coefficients used in the simulation. In addition to the listed mechanisms, the simulation includes collisional mixing between Ne 1s or higher excited states and radiative cascading, as well as the imprisonment of resonance radiation, or photon trapping effect, i.e., the repeated absorption and reemission of the Ne( 1 P 1 , 3 P 1 ) spontaneous emissions by neighboring ground-state Ne atoms.…”
Section: A Descriptionmentioning
confidence: 99%
“…This is the case for the Penning ionization ͑PI͒ and hetero-nuclear associative ionization ͑AI͒ mechanisms involving the Ne 1s and dimer states. [26][27][28][29][30][31][32][33][34][35][36][37][38][39][40][41] Table I is a list of the PI and AI mechanisms and related processes affecting the population of the relevant excited species, together with the rate coefficients used in the simulation. In addition to the listed mechanisms, the simulation includes collisional mixing between Ne 1s or higher excited states and radiative cascading, as well as the imprisonment of resonance radiation, or photon trapping effect, i.e., the repeated absorption and reemission of the Ne( 1 P 1 , 3 P 1 ) spontaneous emissions by neighboring ground-state Ne atoms.…”
Section: A Descriptionmentioning
confidence: 99%
“…The role of impurities in our system can be of great importance in these measurements on account of Penning e!ects [20], which increase the ionization yield, therefore reducing the =-value measured. This was tested by switching o!…”
Section: Impuritiesmentioning
confidence: 99%
“…L'énergie moyenne nécessaire pour former une paire d'ions est fonction essentiellement du gaz ou du mélange gazeux, et la présence d'impu retés, même en faible quantité, peut entraîner de grandes variations de valeur, en particulier pour les gaz nobles (tableau 2) [53]. Pour un mélange gazeux, Hurst propose la formule [54] : où w, w1, w2 sont les énergies moyennes nécessaires pour former une paire d'ions respectivement dans le mélange gazeux et dans chacun des gaz constitutifs, p1 et p2 les pressions partielles de remplissage, et« a » une constante caractéristique du mélange gazeux déterminé empiriquement. Le tableau ci-dessous donne dif férentes valeurs de « a » : mélange : N2-H2 N2-Ar N2-O2 He-Ar He-H2 «a» : 0,28 0,53 1,06 0,75 3,55 mélange : He-N2…”
Section: Réalisation Des Compteurs : A) Technologie Généraleunclassified