$^{*}$ Now at The Martin Company, Orlando, Florida.Author Institution: Radiation Laboratory, The Johns Hopkins UniversityThe advantages of extending gas maser techniques to millimeter wavelengths are presented. Following a review of the requirements for maser action, several molecules are examined for those features satisfying such requirements Data include rotational energy level schemes and their populations along with the Stark focusing efficiencies for several heavy symmetrical and anti-symmetrical top molecules. Among the gases studied thus far which have transitions in the one to two millimeter wavelength region, methyl fluoride shows some promise of satisfying the conditions for maser action. Consequently, a maser has been designed f...
We studied class I methanol masers in the transition 7_0-6_1 A+ at the frequency 44 GHz with the VLA...
The mm-wave (10-110 GHz) frequency band contains the fundamental rotational resonance frequencies of...
We have used the Australia Telescope National Facility Mopra 22-m antenna to search for 37.7-GHz (7₋...
The theory of the molecular transitions which are induced by the microwave field in a maser and the ...
Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness tempe...
$^{1}$ J.P. Gordon, H.J. Zeiger and C.H. Townes, Phys. Rev. 99, 1264 (1955). $^{2}$ P. Thaddeus, L.C...
The fundamental theoretical limitations of the maser, systematic processes that cause instability, a...
Since the 1950's, many devices have been discovered which produce co-herent, monochromatic, ele...
This work is supported by the National Science Foundation, Grant No. GP-34590.Author Institution: De...
An amnonia beam maser with a single resonant cavity and with two cascaded cavities is investigated. ...
We report the detection of a new class I methanol maser candidate from the 52-41 E transition (266.8...
Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness tempe...
Author Institution: Martin Marietta CorporationA description is given of experiments performed or co...
Massive newly formed stars are obscured by dust, and their clearest signature is often at radio freq...
$^{*}$Supported to part by Space System Division, Air Force systems command, Los Angeles, California...
We studied class I methanol masers in the transition 7_0-6_1 A+ at the frequency 44 GHz with the VLA...
The mm-wave (10-110 GHz) frequency band contains the fundamental rotational resonance frequencies of...
We have used the Australia Telescope National Facility Mopra 22-m antenna to search for 37.7-GHz (7₋...
The theory of the molecular transitions which are induced by the microwave field in a maser and the ...
Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness tempe...
$^{1}$ J.P. Gordon, H.J. Zeiger and C.H. Townes, Phys. Rev. 99, 1264 (1955). $^{2}$ P. Thaddeus, L.C...
The fundamental theoretical limitations of the maser, systematic processes that cause instability, a...
Since the 1950's, many devices have been discovered which produce co-herent, monochromatic, ele...
This work is supported by the National Science Foundation, Grant No. GP-34590.Author Institution: De...
An amnonia beam maser with a single resonant cavity and with two cascaded cavities is investigated. ...
We report the detection of a new class I methanol maser candidate from the 52-41 E transition (266.8...
Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness tempe...
Author Institution: Martin Marietta CorporationA description is given of experiments performed or co...
Massive newly formed stars are obscured by dust, and their clearest signature is often at radio freq...
$^{*}$Supported to part by Space System Division, Air Force systems command, Los Angeles, California...
We studied class I methanol masers in the transition 7_0-6_1 A+ at the frequency 44 GHz with the VLA...
The mm-wave (10-110 GHz) frequency band contains the fundamental rotational resonance frequencies of...
We have used the Australia Telescope National Facility Mopra 22-m antenna to search for 37.7-GHz (7₋...