scholarly journals Venus: The Atmosphere, Climate, Surface, Interior and Near-Space Environment of an Earth-Like Planet

2018 ◽  
Vol 214 (1) ◽  
Author(s):  
Fredric W. Taylor ◽  
Håkan Svedhem ◽  
James W. Head
Keyword(s):  
2017 ◽  
pp. 805-816
Author(s):  
Victor Pankratius ◽  
Anthea Coster ◽  
Juha Vierinen ◽  
Philip Erickson ◽  
Bill Rideout

2010 ◽  
Vol 31 (1) ◽  
pp. 70-82
Author(s):  
Kang Cao ◽  
John Baker

Author(s):  
David Murphy ◽  
Joseph Mangan ◽  
Alexei Ulyanov ◽  
Sarah Walsh ◽  
Rachel Dunwoody ◽  
...  

AbstractRecent advances in silicon photomultiplier (SiPM) technology and new scintillator materials allow for the creation of compact high-performance gamma-ray detectors which can be deployed on small low-cost satellites. A small number of such satellites can provide full sky coverage and complement, or in some cases replace the existing gamma-ray missions in detection of transient gamma-ray events. The aim of this study is to test gamma-ray detection using a novel commercially available CeBr3 scintillator combined with SiPM readout in a near-space environment and inform further technology development for a future space mission. A prototype gamma-ray detector was built using a CeBr3 scintillator and an array of 16 J-Series SiPMs by ON Semiconductor. SiPM readout was performed using SIPHRA, a radiation-tolerant low-power integrated circuit developed by IDEAS. The detector was flown as a piggyback payload on the Advanced Scintillator Compton Telescope balloon flight from Columbia Scientific Balloon Facility. The payload included the detector, a Raspberry Pi on-board computer, a custom power supply board, temperature and pressure sensors, a Global Navigation Satellite System receiver and a satellite modem. The balloon delivered the detector to 37 km altitude where its detection capabilities and readout were tested in the radiation-intense near-space environment. The detector demonstrated continuous operation during the 8-hour flight and after the landing. It performed spectral measurements in an energy range of 100 keV to 8 MeV and observed the 511 keV gamma-ray line arising from positron annihilation in the atmosphere with full width half maximum of 6.8%. During ascent and descent, the detector count rate peaked at an altitude of 16 km corresponding to the point of maximum radiation intensity in the atmosphere. Despite several engineering issues discovered after the flight test, the results of this study confirm the feasibility of using CeBr3 scintillator, SiPMs, and SIPHRA in future space missions.


2021 ◽  
Vol 29 ◽  
pp. 22-29
Author(s):  
Bo Wang ◽  
Tong Ye ◽  
Xiaoyan Li ◽  
Po Bian ◽  
Yongding Liu ◽  
...  

Author(s):  
Q. Meng ◽  
F. He ◽  
W. Zhao ◽  
K. Wang ◽  
L. Yang ◽  
...  

<p><strong>Abstract.</strong> To investigate mass transport and energy dissipation in space environments for solar system planet, a balloon-borne planetary atmospheric spectral telescope (PAST) is designed with 0.8-m aperture in spectral range from 280&amp;thinsp;nm to 680&amp;thinsp;nm will be floated at 35&amp;ndash;40&amp;thinsp;km altitude to observe and investigate the global space environment of Mercury, Venus, Mars, and Jupiter. The telescope is designed by Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences (CIOMP, CAS), and supported by the Strategic Priority Research Program of Chinese Academy of Sciences, that is the Scientific Experimental system in Near-SpacE (SENSE). The telescope is mainly supported by a Ritchey-Chrétien optical system which can achieve 0.5" angular resolution observation, and the optical system has the function of focusing and stabilizing. The telescope is combined with a two-dimension rotate platform to achieve planetary atmospheric imaging in long exposure time. This paper mainly introduces the PAST scheme briefly.</p>


2020 ◽  
Vol 5 (1) ◽  
pp. 52-73 ◽  
Author(s):  
David J. Smith ◽  
Marianne B. Sowa

AbstractDespite centuries of scientific balloon flights, only a handful of experiments have produced biologically relevant results. Yet unlike orbital spaceflight, it is much faster and cheaper to conduct biology research with balloons, sending specimens to the near space environment of Earth's stratosphere. Samples can be loaded the morning of a launch and sometimes returned to the laboratory within one day after flying. The National Aeronautics and Space Administration (NASA) flies large unmanned scientific balloons from all over the globe, with missions ranging from hours to weeks in duration. A payload in the middle portion of the stratosphere (~35 km above sea level) will be exposed to an environment similar to the surface of Mars—temperatures generally around −36°C, atmospheric pressure at a thin 1 kPa, relative humidity levels <1%, and harsh illumination of ultraviolet (UV) and cosmic radiation levels (about 100 W/m2 and 0.1 mGy/d, respectively)—that can be obtained nowhere else on the surface of the Earth, including environmental chambers and particle accelerator facilities attempting to simulate space radiation effects. Considering the operational advantages of ballooning and the fidelity of space-like stressors in the stratosphere, researchers in aerobiology, astrobiology, and space biology can benefit from balloon flight experiments as an intermediary step on the extraterrestrial continuum (i.e., ground, low Earth orbit, and deep space studies). Our review targets biologists with no background or experience in scientific ballooning. We will provide an overview of large balloon operations, biology topics that can be uniquely addressed in the stratosphere, and a roadmap for developing payloads to fly with NASA.


Eos ◽  
2017 ◽  
Author(s):  
Leah Crane

Modeling Earth’s near-space environment and its electrical currents is challenging. A new study compares how four different models stack up against observations.


Radio Science ◽  
1997 ◽  
Vol 32 (5) ◽  
pp. 1953-1963 ◽  
Author(s):  
V. E. Kunitsyn ◽  
E. S. Andreeva ◽  
O. G. Razinkov

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