scholarly journals Lunar Occultation

Lunar Science ◽  
2019 ◽  
Author(s):  
Abdulrahman Malawi
Keyword(s):  
Lunar Occultation

scholarly journals Lunar occultation of the diffuse radio sky: LOFAR measurements between 35 and 80 MHz

2015 ◽  
Vol 450 (3) ◽  
pp. 2291-2305 ◽  
Author(s):  
H. K. Vedantham ◽  
L. V. E. Koopmans ◽  
A. G. de Bruyn ◽  
S. J. Wijnholds ◽  
M. Brentjens ◽  
...  
Keyword(s):  
Lunar Occultation

scholarly journals Lunar Occultation of the Radio Source CTA 21

Nature ◽  
1965 ◽  
Vol 207 (4996) ◽  
pp. 511-511 ◽  
Author(s):  
R. W. CLARKE ◽  
R. A. BATCHELOR
Keyword(s):  
Radio Source ◽  
Lunar Occultation

Stratospheric Aerosol and Gas Experiment III on the International Space Station (SAGE III/ISS) Newly Released V5.2 Validation of Ozone and Water Vapor Data

2021 ◽  
Author(s):  
Susan Kizer ◽  
David Flittner ◽  
Marilee Roell ◽  
Robert Damadeo ◽  
Carrie Roller ◽  
...  
Keyword(s):  
Water Vapor ◽  
International Space Station ◽  
Space Station ◽  
Stratospheric Aerosol ◽  
Vertical Profiles ◽  
Science Data ◽  
International Space ◽  
Lunar Occultation ◽  
Data Continuity

<p>The Stratospheric Aerosol and Gas Experiment III (SAGE III) instrument installed on the International Space Station (ISS) has completed over three and a half years of data collection and production of science data products. The SAGE III/ISS is a solar and lunar occultation instrument that scans the light from the Sun and Moon through the limb of the Earth’s atmosphere to produce vertical profiles of aerosol, ozone, water vapor, and other trace gases. It continues the legacy of previous SAGE instruments dating back to the 1970s to provide data continuity of stratospheric constituents critical for assessing trends in the ozone layer. This presentation shows the validation results of comparing SAGE III/ISS ozone and water vapor vertical profiles from the newly released v5.2 science product with those of in situ and satellite data .</p>

Analysis of Lunar Occultation Data

1971 ◽  
pp. 668-674 ◽  
Author(s):  
M. M. McCants ◽  
R. Edward Nather
Keyword(s):  
Lunar Occultation ◽  
Occultation Data

scholarly journals FIRST LUNAR OCCULTATION RESULTS FROM THE 2.4 m THAI NATIONAL TELESCOPE EQUIPPED WITH ULTRASPEC

2014 ◽  
Vol 148 (5) ◽  
pp. 100 ◽  
Author(s):  
A. Richichi ◽  
P. Irawati ◽  
B. Soonthornthum ◽  
V. S. Dhillon ◽  
T. R. Marsh
Keyword(s):  
Lunar Occultation

78. The lunar occultation of a radio star and the derivation of an upper limit for the density of the lunar atmosphere

1957 ◽  
Vol 4 ◽  
pp. 403-405 ◽  
Author(s):  
B. Elsmore
Keyword(s):  
Radio Source ◽  
Large Diameter ◽  
Circular Region ◽  
Radio Brightness ◽  
Interferometric Method ◽  
Filamentary Structure ◽  
Lunar Occultation ◽  
Upper Limit

Observations were made at Cambridge on 26 April 1955 of the lunar occultation of the large-diameter radio source in the constellation of Gemini. This radio source, having r.a. 06h 13m 37s and dec. 22° 38′ (1950·0), has been identified by Baldwin and Dewhirst (1954) [1] as the galactic nebulosity IC443, which consists of a filamentary structure contained within a circular region of 24′·5 radius. Baldwin and Dewhirst also succeeded in measuring the distribution of radio ‘brightness’ across the source using an interferometric method; their measurements indicate that the diameter of the radio source is approximately the same as that of the visible nebulosity.

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