Accurate and consistent microwave observations of venus and their implications

Icarus

Volumn 154, Issue 2, 2001, Pages 226-238

  Butler, Bryan J ^a   Steffes, Paul G ^b   Suleiman, Shady H ^b   Kolodner, Marc A ^c   Jenkins, Jon M ^d  

^a NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^b GEORGIA INSTITUTE OF TECHNOLOGY   (United States)

^c JOHNS HOPKINS UNIVERSITY   (United States)

^d NASA AMES RESEARCH CENTER   (United States)

Author keywords

Radiative transfer; Radio observations; Venus

Indexed keywords

EID: 0035735791     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1006/icar.2001.6710     Document Type: Article

References (63)

1. Cloud structure on the dark side of Venus
2. The absolute spectrum of Cas A. An accurate flux density scale and a set of secondary calibrators
3. Microwave absorption and emission in the atmosphere of Venus
4. Radio observations of Venus and the interpretations
5. High-resolution interferometry of Venus at 3.12-cm wavelength
6. High-resolution interferometric observations of Venus at three radio wavelengths
7. The abundance of sulfur dioxide below the clouds of Venus
8. Balloons on Planet Venus-Final results
9. Solar System objects
10. Electrical properties of rocks and their significance for lunar radar observations
11. The measurement of the polarization and brightness distribution of Venus at 10.6-cm wavelength
12. Some decimeter observations of Venus during the 1962
13. The brightness temperature of Venus at 70 centimeters
14. Self-calibration
15. The dark side of Venus: Near infrared images and spectra from the Anglo-Australian observatory
16. Sulfur dioxide at the Venus cloud tops, 1978-1986
17. 2) under simulated conditions for the Venus atmosphere
18. Analysis of the panoramas of the Venera 13 and Venera 14 landing sites
19. Venus topography and kilometer-scale slopes
20. How to measure surface and atmospheric conditions on Venus by microwave interferometry
21. Observations of the CO bulge on Venus and implications for mesospheric winds
22. Essential ray tracing algorithms
23. High-resolution radio observations of the planet Venus at a wavelength of 6 cm
24. Atmospheric ray path modeling for radiative transfer algorithms
25. Writing a ray tracer
26. Laboratory measurement of microwave absorption in models of the atmosphere of Venus
27. Constraints on the composition of the Venus atmosphere from microwave measurements near 1.35-cm wavelength
28. 4 abundance profiles from the Season 10 (1986) Pioneer Venus Orbiter Radio Occultation Experiment
29. Radio occultation studies of the Venus atmosphere with the Magellan Spacecraft 2: Results from the October 1991 experiments
30. Retrievals of sulfur-bearing gas abundances from microwave emission maps of Venus obtained at the VLA
31. The microwave absorption and abundance of sulfuric acid vapor in the Venus atmosphere based on new laboratory measurements
32. Revised lunar heat-flow values
33. Detection of the surface of Venus at 1.0 μm from ground-based observations
34. Estimates of elastic lithosphere thickness and heat flux beneath large volcanoes on Venus
35. Microwave imaging of Mercury's thermal emission at wavelengths from 0.3 to 20.5 cm
36. Lunar Remote Sensing and Measurements
37. The brightness temperature of Venus and the absolute flux-density scale at 608 MHz
38. A model of the Venus atmosphere from radio, radar, and occultation observations
39. 2 and SO
40. Sulfur dioxide in the atmosphere of Venus II. Modeling results
41. The primary antenna elements
42. VLA Primary Beam Parameters
43. Pioneer Venus gas chromotography of the lower atmosphere of Venus
44. Venus: Surface electromagnetic properties
45. Magellan: Radar performance and data products
46. Venus surface radiothermal emission as observed by Magellan
47. The Non-SAR Experiments
48. Magellan mission summary
49. Lunar heat flow and regolith structure inferred from interferometric observations at a wavelength of 49.3 cm
50. Atmospheres of Earth, Mars, and Venus, as defined by entry probe experiments
51. Precision interferometric observations of Venus at 11.1-centimeter wavelength
52. Observations of the microwave emission of Venus from 1.3 to 3.6 cm
53. Radio occultation studies of the Venus atmosphere with the Magellan spacecraft 1. Experimental description and performance
54. 2) microwave absorption with application to the Venus atmosphere
55. Interferometry and Synthesis in Radio Astronomy
56. Effect of heat from within the Moon on its radio emission for the case of lunar properties which vary with depth
57. Calibration radio sources for radio astronomy: Precision flux density measurements at 8420 MHz
58. Scattering properties of the venusian surface: Preliminary results from Magellan
59. Absolute brightness temperature measurements at 3.5-mm wavelength
60. First panoramic pictures of Venus: Preliminary image analysis
61. Venus: Measurements of brightness temperatures in the 7-15-cm wavelength range and theoretical radio and radar spectra for a two-layer subsurface model
62. Seismic investigation of the lunar regolith
63. 2 in the middle atmosphere of Venus: IR measurements from Venera-15 and comparison to UV data