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2020
This chapter presents a description of the detected radio emission from Solar System objects such as the Sun, the terrestrial planets (in which the Moon may be included, given its general similar radio properties), the giant planets, and the minor planets.
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This chapter presents a description of the detected radio emission from Solar System objects such as the Sun, the terrestrial planets (in which the Moon may be included, given its general similar radio properties), the giant planets, and the minor planets.
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Classical Astronomy. The Solar System
1991We shall begin our treatment of astronomy with a historical overview of classical astronomy (Sect. 2.1) from ancient times up through the introduction of the heliocentric system by Nicholas Copernicus, Tycho Brahe, Johannes Kepler, Galileo Galilei and their contemporaries, and the founding of celestial mechanics by Isaac Newton at the close of the 17th
Albrecht Unsöld, Bodo Baschek
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Overview on wavefront corrector technologies for astronomy and solar adaptive optics systems
Adaptive Optics Systems VII, 2020By now Adaptive optics systems are used at nearly all large telescopes. Over the past years not only the number of applications increased but as well the correction order and specialization have evolved. One key element following and sometimes driving the development of adaptive optics is the wavefront corrector. The construction and development of the
Stefan Stroebele +2 more
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X-ray Astronomy from the Solar System to the High Redshift Universe
Astronomische Nachrichten, 2003F01 XMM-Newton: Mission Status and Science Archive F02 Introduction to the Chandra X-ray Observatory F03 Discovery of X-rays from Mars with Chandra F04 Investigation of Stellar Coronae with Chandra and XMM-Newton F05 High-resolution X-ray Spectra of Young Stars F06 Chandra Spectroscopy of an Extremely Hot Bare Stellar
Stefanie Komossa +3 more
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Solar system, low frequency radio astronomy from the moon
Advances in Space Research, 1994Radio astronomy, particularly radio astronomy at low frequencies (< 100 MHz) is becoming more and more difficult to operate from Earth-based observatories because of the proliferation of manmade interferences. At frequencies lower than 10 MHz, observations are rarely possible,or impossible, because of the opacity of the terrestial ionosphere.
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Astronomische Nachrichten, 2005
AbstractP01 Calibrations on DSS‐II PlatesP02 High‐Resolution Near‐Infrared Speckle Interferometry and Radiative Transfer Modeling of the OH/IR star OH 26.5 + 0.6P03 Mid‐infrared long‐baseline interferometry of the symbiotic Mira star RX Pup with the VLTI/MIDI instrumentP04 N2D+ abundance in high mass star forming regionsP05Causal Viscosity in Accretion
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AbstractP01 Calibrations on DSS‐II PlatesP02 High‐Resolution Near‐Infrared Speckle Interferometry and Radiative Transfer Modeling of the OH/IR star OH 26.5 + 0.6P03 Mid‐infrared long‐baseline interferometry of the symbiotic Mira star RX Pup with the VLTI/MIDI instrumentP04 N2D+ abundance in high mass star forming regionsP05Causal Viscosity in Accretion
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The Solar System and Video Astronomy
2016The solar system is of interest to many video astronomers. Video astronomy and its adaptabilities for solar, lunar, and planetary viewing, photography, and other scientific activities are explored. Each activity is discussed separately and in detail from the perspective of the characteristics of a video telescope. For solar observers attention is given
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IAF Symposium on Ongoing and Near Future Space Astronomy and Solar-System Science Missions
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The Beginning of the New Age of Astronomy: Beyond the Solar System
1995In 1757 a 19-year-old musician from Hannover, Germany, settled in England as a music teacher and organist. Coming from a highly cultured and gifted German-Jewish family of musicians—his father was a kappellmeister—and having won a prestigious prize for his organ playing, William Herschel, at the age of 36, became the music master at Bath and a popular ...
Lloyd Motz, Jefferson Hane Weaver
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Impact to the radio astronomy by the interference caused by the solar power satellite systems
2011 XXXth URSI General Assembly and Scientific Symposium, 2011We have conducted a preliminary study to assess interference caused by a SPS to radio astronomy observations, and show that the SPS that is currently planned is highly unlikely to coexist with radio astronomy observations.
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