Found 49 datasets matching "radio astronomy".
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VG1-J-PRA-3-RDR-6SEC-V1.0
Search relevance: 105.35 | Views last month: 0 -
VG2-J-PRA-3-RDR-6SEC-V1.0
Search relevance: 105.35 | Views last month: 0 -
VG2-J-PRA-3-RDR-6SEC-V1.0
Search relevance: 103.24 | Views last month: 0 -
VG1-J-PRA-3-RDR-6SEC-V1.0
Search relevance: 102.62 | Views last month: 0 -
C USER'S GUIDE TO RAR 144 SECOND AVERAGED DATA FILES ---------------- This document describes the contents and format of the RAR 144 second averaged data files.
Search relevance: 90.16 | Views last month: 0 -
C USER'S GUIDE TO RAR 144 SECOND AVERAGED DATA FILES ------------------ This document describes the contents and format of the RAR 144 second averaged data files.
Search relevance: 89.60 | Views last month: 0 -
A. UDS data files -------------------- Eight files are provided that conform to the UDS conventions regarding the naming of files and the format of the data. The eight files are divided into 4...
Search relevance: 89.60 | Views last month: 0 -
A. UDS data files -------------------- Eight files are provided that conform to the UDS conventions regarding the naming of files and the format of the data. The eight files are divided into 4...
Search relevance: 88.38 | Views last month: 0 -
A. UDS data files --------------------- Eight files are provided that conform to the UDS conventions regarding the naming of files and the format of the data. The eight files are divided into 4...
Search relevance: 87.84 | Views last month: 0 -
C USER'S GUIDE TO RAR 144 SECOND AVERAGED DATA FILES ---------------------------------------------------- This document describes the contents and format of the RAR 144 second averaged data files.
Search relevance: 87.84 | Views last month: 0 -
Wind Waves RAD2, RAD1, and TNR data in CDF format. RAD1 RAD1 is the low frequency radio astronomy receiver. It sweeps over the range of 20 to 1040 kHz with as many as 256 channels. However, some...
Search relevance: 58.12 | Views last month: 6 -
This database contains critically evaluated transition frequencies for the molecular transitions detected in interstellar and circumstellar clouds reported in the literature through mid-2008. The...
Search relevance: 57.61 | Views last month: 1 -
Very Long Baseline Interferometry (VLBI) is a geometric technique: it measures the time difference between the arrival at two Earth-based antennas of a radio wavefront emitted by a distant quasar....
Search relevance: 55.03 | Views last month: 0 -
Very Long Baseline Interferometry (VLBI) is a geometric technique: it measures the time difference between the arrival at two Earth-based antennas of a radio wavefront emitted by a distant quasar....
Search relevance: 54.86 | Views last month: 0 -
This dataset consists of edited browse data derived from an original dataset obtained from the Voyager 2 Planetary Radio Astronomy (PRA) instrument in the vicinity of Neptune. Data are provided...
Search relevance: 53.82 | Views last month: 0 -
This data set consists of edited browse data derived from an original data set obtained from the Voyager 1 Planetary Radio Astronomy (PRA) instrument in the vicinity of Jupiter. Data are provided...
Search relevance: 53.04 | Views last month: 0 -
This data set consists of edited browse data derived from an original data set obtained from the Voyager 2 Planetary Radio Astronomy (PRA) instrument in the vicinity of Jupiter. Data are provided...
Search relevance: 52.95 | Views last month: 0 -
This dataset consists of edited browse data derived from an original dataset obtained from the Voyager 2 Planetary Radio Astronomy (PRA) instrument in the vicinity of Uranus. Data are provided for...
Search relevance: 52.31 | Views last month: 0 -
This data set (VG2-U-PRA-2-RDR-HIGHRATE-60MS-V1.0) contains data acquired by the Voyager-2 Planetary Radio Astronomy (PRA) instrument during the Uranus encounter. Since the PRA instrument is able...
Search relevance: 52.07 | Views last month: 0 -
This data set contains data acquired by the Voyager-1 Planetary Radio Astronomy (PRA) instrument during the Saturn encounter. Since the PRA instrument is able to observe planetary phenomenon at...
Search relevance: 51.86 | Views last month: 0
