has made the first continuous global measurements of HCN in the middle atmosphere. The measurements are in broad agreement with most earlier measurements, showing HCN to be a long-lived tracer with sources in the troposphere and sinks in the middle atmosphere. There is no evidence in the data for a proposed mesospheric source of HCN
peer reviewedVertical mixing ratio profiles of four relatively long-lives gases, HCN, C2H2, CO, and ...
Abstract. Gas phase HCl was measured from the marine boundary layer (MBL) to the lower stratosphere ...
HCN J = 1-0 emission from the long-period comet C/2013 R1 (Lovejoy) was observed from the Onsala Spa...
It is known from ground-based measurements made during the 1982–1983 and 1997–1998 El Niño events t...
The potential to detect hydrogen cyanide (HCN) spectral signatures and retrieve HCN volume mixing ra...
It is known from ground-based measurements made during the 1982-1983 and 1997-1998 El Niño events th...
To identify the effect of meteor showers on the molecular content of the upper atmosphere of the Ear...
To identify the effect of meteor showers on the molecular content of the upper atmosphere of the Ear...
CH3CN in the stratosphere has been measured by the Microwave Limb Sounder (MLS) on the Upper Atmosph...
We report the first in situ measurements of hydrogen cyanide (HCN) and methyl cyanide (CH3CN, aceton...
International audienceObservations of Jupiter by Cassini/CIRS, acquired during the December 2000 fly...
Abstract. We present global upper tropospheric HCN and C2H6 amounts derived from MIPAS/ENVISAT limb ...
(EOS) Aura satellite. The HIRDLS instrument obtains between 5000 and 7000 HNO3 profiles per day. HIR...
International audience Aims: The aim of this study is to measure the vertical distribution of HCN on...
HCN J = 1–0 emission from the long-period comet C/2013 R1 (Lovejoy) was observed from the Onsala Spa...
peer reviewedVertical mixing ratio profiles of four relatively long-lives gases, HCN, C2H2, CO, and ...
Abstract. Gas phase HCl was measured from the marine boundary layer (MBL) to the lower stratosphere ...
HCN J = 1-0 emission from the long-period comet C/2013 R1 (Lovejoy) was observed from the Onsala Spa...
It is known from ground-based measurements made during the 1982–1983 and 1997–1998 El Niño events t...
The potential to detect hydrogen cyanide (HCN) spectral signatures and retrieve HCN volume mixing ra...
It is known from ground-based measurements made during the 1982-1983 and 1997-1998 El Niño events th...
To identify the effect of meteor showers on the molecular content of the upper atmosphere of the Ear...
To identify the effect of meteor showers on the molecular content of the upper atmosphere of the Ear...
CH3CN in the stratosphere has been measured by the Microwave Limb Sounder (MLS) on the Upper Atmosph...
We report the first in situ measurements of hydrogen cyanide (HCN) and methyl cyanide (CH3CN, aceton...
International audienceObservations of Jupiter by Cassini/CIRS, acquired during the December 2000 fly...
Abstract. We present global upper tropospheric HCN and C2H6 amounts derived from MIPAS/ENVISAT limb ...
(EOS) Aura satellite. The HIRDLS instrument obtains between 5000 and 7000 HNO3 profiles per day. HIR...
International audience Aims: The aim of this study is to measure the vertical distribution of HCN on...
HCN J = 1–0 emission from the long-period comet C/2013 R1 (Lovejoy) was observed from the Onsala Spa...
peer reviewedVertical mixing ratio profiles of four relatively long-lives gases, HCN, C2H2, CO, and ...
Abstract. Gas phase HCl was measured from the marine boundary layer (MBL) to the lower stratosphere ...
HCN J = 1-0 emission from the long-period comet C/2013 R1 (Lovejoy) was observed from the Onsala Spa...