Add to ORKGCommunications Research Laboratory and National Space Development Agency of Japan are collaborating to develop a submillimeter-wave limb-emission sounder (SMILES) to be installed on the Japanese Experiment Module (JEM) of the International Space Station. The JEM/SMILES is a submillimeter-wave limb-sounding radiometer operating in the 640-GHz band for observing stratospheric minor constituents such as O3, ClO, HCl, HO2, BrO, etc., which play important roles in the depletion of the stratospheric ozone layer. This paper describes the objectives of the JEM/SMILES mission and the outline of the design of the SMILES system currently being developed
A new state-of-the-art balloon borne three channel (500, 625, 1800 GHz) cryogenic heterodyne spectro...
The Submillimeter Wave Astronomy Satellite (SWAS), launched in 1998 December, is a NASA mission dedi...
The simulated retrieval performance of a submillimeter wave limb sounder was compared with that of a...
A new generation of sub-millimeter-wave receivers employing sensitive SIS (Superconductor-Insulator-...
successfully launched and attached to the Japanese Experiment Module (JEM) on the International Spac...
The submillimeter-wave limb-emission sounder called SMILES is currently being developed for the Japa...
We observed ozone (O3) in the vertical region between 250 and 0.0005 hPa (~12-96 km) using the Super...
The isotopic ratio of molecules often provides valuable information about past or presently occurrin...
Recent progress in sub-millimeter wave receiver technology gives the possibility to drastically impr...
SMILES is a heterodyne sub-millimeter receiver which will be installed on the ELM-ES platform of th...
Abstract. Chlorine monoxide (ClO) is the key species for anthropogenic ozone losses in the middle at...
Technology is now becoming available to develop submilli-meter wavelength heterodyne radiometric exp...
The Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) onboard the International Spac...
Trace gases such as ClO, HO_2,etc. in the upper atmosphere play important roles in the chemistry of ...
Chlorine monoxide (ClO) is the key species for anthropogenic ozone losses in the middle atmosphere. ...
A new state-of-the-art balloon borne three channel (500, 625, 1800 GHz) cryogenic heterodyne spectro...
The Submillimeter Wave Astronomy Satellite (SWAS), launched in 1998 December, is a NASA mission dedi...
The simulated retrieval performance of a submillimeter wave limb sounder was compared with that of a...
A new generation of sub-millimeter-wave receivers employing sensitive SIS (Superconductor-Insulator-...
successfully launched and attached to the Japanese Experiment Module (JEM) on the International Spac...
The submillimeter-wave limb-emission sounder called SMILES is currently being developed for the Japa...
We observed ozone (O3) in the vertical region between 250 and 0.0005 hPa (~12-96 km) using the Super...
The isotopic ratio of molecules often provides valuable information about past or presently occurrin...
Recent progress in sub-millimeter wave receiver technology gives the possibility to drastically impr...
SMILES is a heterodyne sub-millimeter receiver which will be installed on the ELM-ES platform of th...
Abstract. Chlorine monoxide (ClO) is the key species for anthropogenic ozone losses in the middle at...
Technology is now becoming available to develop submilli-meter wavelength heterodyne radiometric exp...
The Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) onboard the International Spac...
Trace gases such as ClO, HO_2,etc. in the upper atmosphere play important roles in the chemistry of ...
Chlorine monoxide (ClO) is the key species for anthropogenic ozone losses in the middle atmosphere. ...
A new state-of-the-art balloon borne three channel (500, 625, 1800 GHz) cryogenic heterodyne spectro...
The Submillimeter Wave Astronomy Satellite (SWAS), launched in 1998 December, is a NASA mission dedi...
The simulated retrieval performance of a submillimeter wave limb sounder was compared with that of a...