Avalanches in gas-based detectors operating at atmospheric pressure and using Ar−CO(2) or Ne−CO(2) as drift medium produce in a first instance mainly Ar(+), Ne(+) and CO(2)(+) ions. The noble gas ions transfer their charge to CO(2) in a few ns. A few ns later, the CO(2)(+) ions have picked up CO(2) molecules, forming cluster ions, in particular CO(2)(+)·(CO(2))n. Since the cluster ions are slower than the initial ions, the signals induced by ion motion are altered. The effect is shown to be present in constant-field detectors and TPC readout chambers, and is expected to affect devices such as Micromegas and drift tubes
The formation of secondary particles in the atmosphere accounts for more than half of global cloud c...
We show that the cluster ion concentration (CIC) in the atmosphere is significantly suppressed durin...
We show that the cluster ion concentration (CIC) in the atmosphere is significantly suppressed durin...
Avalanches in gas-based detectors operating at atmospheric pressure and using Ar-CO2 or Ne-CO2 as dr...
Avalanches in gas-based detectors operating at atmospheric pressure and using Ar-CO2 or Ne-CO2 as dr...
Avalanches in gas-based detectors operating at atmospheric pressure and using Ar-CO2 or Ne-CO2 as dr...
Detektörlerin aktif gaz hacimlerinde, yüklü parcacıkların gaz moleküllerini iyonlaştırması ile ilk i...
One of the main drawbacks of the use of microgap structures when used at high pressure (6 bar) at hi...
One of the main drawbacks of the use of microgap structures when used at high pressure (6 bar) at hi...
Avalanche fluctuations set a limit to the energy and position resolutions that can be reached by gas...
We show that the cluster ion concentration (CIC) in the atmosphere is significantly suppressed durin...
International audienceTheRout, Prasant Kumar micropatternBhattacharya, Deb Sankar gaseousBhattachary...
The formation of secondary particles in the atmosphere accounts for more than half of global cloud c...
The formation of secondary particles in the atmosphere accounts for more than half of global cloud c...
International audienceAvalanche fluctuations set a limit to the energy and position resolutions that...
The formation of secondary particles in the atmosphere accounts for more than half of global cloud c...
We show that the cluster ion concentration (CIC) in the atmosphere is significantly suppressed durin...
We show that the cluster ion concentration (CIC) in the atmosphere is significantly suppressed durin...
Avalanches in gas-based detectors operating at atmospheric pressure and using Ar-CO2 or Ne-CO2 as dr...
Avalanches in gas-based detectors operating at atmospheric pressure and using Ar-CO2 or Ne-CO2 as dr...
Avalanches in gas-based detectors operating at atmospheric pressure and using Ar-CO2 or Ne-CO2 as dr...
Detektörlerin aktif gaz hacimlerinde, yüklü parcacıkların gaz moleküllerini iyonlaştırması ile ilk i...
One of the main drawbacks of the use of microgap structures when used at high pressure (6 bar) at hi...
One of the main drawbacks of the use of microgap structures when used at high pressure (6 bar) at hi...
Avalanche fluctuations set a limit to the energy and position resolutions that can be reached by gas...
We show that the cluster ion concentration (CIC) in the atmosphere is significantly suppressed durin...
International audienceTheRout, Prasant Kumar micropatternBhattacharya, Deb Sankar gaseousBhattachary...
The formation of secondary particles in the atmosphere accounts for more than half of global cloud c...
The formation of secondary particles in the atmosphere accounts for more than half of global cloud c...
International audienceAvalanche fluctuations set a limit to the energy and position resolutions that...
The formation of secondary particles in the atmosphere accounts for more than half of global cloud c...
We show that the cluster ion concentration (CIC) in the atmosphere is significantly suppressed durin...
We show that the cluster ion concentration (CIC) in the atmosphere is significantly suppressed durin...