Submillimeter and millimeter observations of jupiter
References (40)
- et al.
The Queen Mary College/University of Oregon photometer for submillimeter continuum observations
Infrared Phys.
(1984) - et al.
On the detectability of H2S in Jupiter
Icarus
(1983) - et al.
The submillimeter spectra of the planets: Narrow-band photometry
Icarus
(1981) - et al.
Far infrared adsorption in normal H2 from 77 K to 298 K
J. Quant. Spectrosc. Radiat. Transfer
(1983) - et al.
Mars: Sub-surface properties from observed longitudinal variation of the 3.5 mm brightness temperature
Icarus
(1983) Modifications to Scott's method for direct integration of gaseous transmission to improve speed and accuracy
J. Quant. Spectroc. Radiat. Transfer
(1981)- et al.
Airborne spectroscopy of Jupiter in the 100- through 300-cm−1 region: Global properties of ammonia gas and ice haze
Icarus
(1982) - et al.
The effect of ammonia ice on the outgoing thermal radiance from the atmosphere of Jupiter
Icarus
(1982) - et al.
Observational constraints on the atmospheres of Uranus and Neptune from new measurements near 10 μm
Icarus
(1983) - et al.
Absolute measurements of the atmospheric transparency at short millimetre wavelengths
Infrared Phys.
(1979)
A direct method of computation of the transmission function of an inhomogeneous gaseous medium
J. Quant. Spectrosc. Radiat. Transfer
Mars: Far infrared spectra and thermal emission models
Icarus
One-millimeter brightness temperature of the planets
Icarus
Solar heating of the Martian dusty atmosphere
Icarus
Detection of carbon monoxide on Jupiter
Astrophys. J.
Earth based observations of Jupiter: Millimeter to meter wavelengths
Mars as an infrared calibration standard: Incorporation of Viking IRTM results
Bull. Amer. Astron. Soc.
Analysis of the far infrared H2-He spectrum
J. Chem. Phys.
Observations of giant planets at 1.4 mm and consequences on the effective temperatures
Astron. Astrophys.
The C/H ratio in Jupiter from the Voyager infrared investigation
Astrophys. J.
Cited by (100)
Ground-based measurements of the 1.3 to 0.3 mm spectrum of Jupiter and Saturn, and their detailed calibration
2017, IcarusCitation Excerpt :Several other observations have been carried out from space, with interesting results despite the small size of the telescope, such as the detection of 557 GHz water emission in the upper atmosphere (maximum pressures around 5 mbar) of both planets (Bergin et al., 2000). Disk-average brightness temperatures at 489 and 553 GHz resulted from these observations which are in disagreement with those of Goldin et al. (1997), thus illustrating how difficult it is to draw conclusions from data at a few frequencies provided by very different experiments (see also Hildebrand, 1985; Griffin et al., 1986. An additional problem for Saturn is the changing temperature due to the effect of the rings, which makes the different data sets incompatible with a single model.
Reconciling the centimeter- and millimeter-wavelength ammonia absorption spectra under jovian conditions: Extensive millimeter-wavelength measurements and a consistent model
2011, IcarusCitation Excerpt :Furthermore, at millimeter-wavelengths, the planets Uranus and Neptune with small apparent diameters and large flux densities are frequently used as primary calibrators of astronomical sources and telescope parameters (Ulich, 1981; Kramer et al., 2008). To date, ground-based millimeter-wavelength observations have yielded disk-averaged emission measurements of the jovian planets (Ulich, 1974; Griffin et al., 1986; Muhleman and Berge, 1991; Griffin and Orton, 1993; Kramer et al., 2008), interferometric mapping of Saturn (Dowling et al., 1987; van der Tak et al., 1999; Dunn et al., 2005), and interferometric observations of limb darkening of Jupiter (Valdes et al., 1982). Accurate interpretation and modeling of the emission spectra of the jovian planets depend on the knowledge of the atmospheric abundances of various constituents and the opacity of each constituent.
Potential for stratospheric Doppler windspeed measurements of Jupiter by sub-millimetre spectroscopy
2010, Planetary and Space ScienceCitation Excerpt :However, sub-millimetre technology has not been utilised to any great extent in planetary observations from spacecraft, as past sub-millimetre instruments have been physically large and heavy, with high power-requirements. In the past, sub-millimetre observations of Jupiter have been done using ground-based telescopes such as the James Clerk Maxwell Telescope (e.g., Davis et al., 1997), the Caltech Submillimeter Observatory (e.g., Weisstein and Serabyn, 1994), the United Kingdom Infrared Telescope (UKIRT) (e.g., Griffin et al., 1986), the NASA Infrared Telescope Facility (IRTF) (e.g., Griffin et al., 1986) and the Nationary Radio Astronomy Observatory (NRAO) (e.g., Griffin et al., 1986; Courtin et al., 1977; Ulich, 1981). The sub-millimetre component of ORTIS is proposed to measure between 73.16 and 73.30 cm−1 (approximately 2.2 THz), in which spectral range there exists strong water vapour H2O and methane CH4 emission lines (Irwin et al., 2008), at a spectral resolution varying between 300 kHz (10−5 cm−1) and 30 kHz (10−6 cm−1).
AMiBA: CLUSTER SUNYAEV-ZEL'DOVICH EFFECT OBSERVATIONS with the EXPANDED 13-ELEMENT ARRAY
2016, Astrophysical JournalA CubeSat for Calibrating Ground-Based and Sub-Orbital Millimeter-Wave Polarimeters (CalSat)
2015, Journal of Astronomical Instrumentation
- 1
Visiting astronomer, United Kingdom Infrared Telescope (UKIRT), Mauna Kea, Hawaii, which is operated by the Royal Observatory Edinburgh, under contract ot the U.k. Science and Engineering Research Council.
- 2
Visisting astronomer, National Radio Astronomy Observatory (NRAO), Kitt Peak, Arizona, which is operated by Associated Universities Inc., under contract to the National Science Foundation.
- 1
Visiting astronomer, United Kingdom Infrared Telescope (UKIRT), Mauna Kea, Hawaii, which is operated by the Royal Observatory Edinburgh, under contract ot the U.k. Science and Engineering Research Council.
- 2
Visisting astronomer, National Radio Astronomy Observatory (NRAO), Kitt Peak, Arizona, which is operated by Associated Universities Inc., under contract to the National Science Foundation.
- 3
Visiting astronomer, Infrared Telescope Facility (IRTF), Mauna Kea, Hawaii, which is operated by the University of Hawaii, under contract to the National Aeronautics and Space Administration.
- 1
Visiting astronomer, United Kingdom Infrared Telescope (UKIRT), Mauna Kea, Hawaii, which is operated by the Royal Observatory Edinburgh, under contract ot the U.k. Science and Engineering Research Council.
- 3
Visiting astronomer, Infrared Telescope Facility (IRTF), Mauna Kea, Hawaii, which is operated by the University of Hawaii, under contract to the National Aeronautics and Space Administration.
- 1
Visiting astronomer, United Kingdom Infrared Telescope (UKIRT), Mauna Kea, Hawaii, which is operated by the Royal Observatory Edinburgh, under contract ot the U.k. Science and Engineering Research Council.
- 2
Visisting astronomer, National Radio Astronomy Observatory (NRAO), Kitt Peak, Arizona, which is operated by Associated Universities Inc., under contract to the National Science Foundation.
- 1
Visiting astronomer, United Kingdom Infrared Telescope (UKIRT), Mauna Kea, Hawaii, which is operated by the Royal Observatory Edinburgh, under contract ot the U.k. Science and Engineering Research Council.
- 2
Visisting astronomer, National Radio Astronomy Observatory (NRAO), Kitt Peak, Arizona, which is operated by Associated Universities Inc., under contract to the National Science Foundation.
- 3
Visiting astronomer, Infrared Telescope Facility (IRTF), Mauna Kea, Hawaii, which is operated by the University of Hawaii, under contract to the National Aeronautics and Space Administration.
- 1
Visiting astronomer, United Kingdom Infrared Telescope (UKIRT), Mauna Kea, Hawaii, which is operated by the Royal Observatory Edinburgh, under contract ot the U.k. Science and Engineering Research Council.
- 2
Visisting astronomer, National Radio Astronomy Observatory (NRAO), Kitt Peak, Arizona, which is operated by Associated Universities Inc., under contract to the National Science Foundation.
- 3
Visiting astronomer, Infrared Telescope Facility (IRTF), Mauna Kea, Hawaii, which is operated by the University of Hawaii, under contract to the National Aeronautics and Space Administration.