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Evolution of Periodic Orbits in the Sun-Saturn System
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作者 Niraj Pathak R. K. Sharma V. O. Thomas 《International Journal of Astronomy and Astrophysics》 2016年第2期175-197,共23页
We analyze the periodic orbits, quasi periodic orbits and chaotic orbits in the photo gravitational Sun-Saturn system incorporating actual oblateness of Saturn in the planar circular restricted three body problem. In ... We analyze the periodic orbits, quasi periodic orbits and chaotic orbits in the photo gravitational Sun-Saturn system incorporating actual oblateness of Saturn in the planar circular restricted three body problem. In this paper, we study the effect of solar radiation pressure on the location of Sun centered and Saturn centered orbits, its diameter, semi major axis and eccentricity by taking different values of solar radiation pressure q and different values of Jacobi constant “C”, and by considering actual oblateness of Saturn using Poincare surface of section (PSS) method. It is ob-served that by the introduction of perturbing force due to solar radiation pressure admissible range of Jacobi constant C decreases, it is also observed that as value of C decreases the number of islands decreases and as a result the number of periodic and quasi periodic orbits decreases.Fur-ther, the periodic orbits around Saturn and Sun moves towards Sun by decreasing perturbation due to solar radiation pressure q for a specific choice of Jacobi constant C. It is also observed that due to solar radiation pressure, semi major axis and eccentricity of Sun centered periodic orbit reduces, whereas, due to solar radiation pressure uniform change in semi major axis and eccen-tricity of Saturn centered periodic orbits is observed. 展开更多
关键词 Restricted Three Body Problem Sun-saturn system Periodic Orbits Quasi Periodic Orbits Chaotic Orbits Photo Gravitation OBLATENESS Poincare Surface Section
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Evolution of the “f” Family Orbits in the Photo Gravitational Sun-Saturn System with Oblateness
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作者 Niraj Pathak V. O. Thomas 《International Journal of Astronomy and Astrophysics》 2016年第3期254-271,共19页
We analyze the periodic orbits of “f” family (simply symmetric retrograde periodic orbits) and the regions of quasi-periodic motion around Saturn in the photo gravitational Sun-Saturn system in the framework of plan... We analyze the periodic orbits of “f” family (simply symmetric retrograde periodic orbits) and the regions of quasi-periodic motion around Saturn in the photo gravitational Sun-Saturn system in the framework of planar circular restricted three-body problem with oblateness. The location, nature and size of these orbits are studied using the numerical technique of Poincare surface of sections (PSS). In this paper we analyze these orbits for different solar radiation pressure (q) and actual oblateness coefficient of Sun Saturn system. It is observed that as Jacobi constant (C) increases, the number of islands in the PSS and consequently the number of periodic and quasi-periodic orbits increase. The periodic orbits around Saturn move towards the Sun with decrease in solar radiation pressure for given value of “C”. It is observed that as the perturbation due to solar radiation pressure decreases, the two separatrices come closer to each other and also come closer to Saturn. It is found that the eccentricity and semi major axis of periodic orbits at both separatrices are increased by perturbation due to solar radiation pressure. 展开更多
关键词 Restricted Three Body Problem Sun-saturn system “f” Family Periodic Orbits Region of Quasi Periodic Orbits Photo Gravitation OBLATENESS Poincare Surface of Section
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Quantum Locking and the Meissner Effect Lead to the Origin and Stability of the Saturn Rings System
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作者 Vladimir V. Tchernyi (Cherny) Andrew Yu. Pospelov 《International Journal of Astronomy and Astrophysics》 2018年第1期104-120,共17页
It is demonstrated how superconducting iced particles of the protoplanetary cloud of Saturn are coming to magnetic equator plane and create the stable enough rings disk. There are two steps. First, after appearance of... It is demonstrated how superconducting iced particles of the protoplanetary cloud of Saturn are coming to magnetic equator plane and create the stable enough rings disk. There are two steps. First, after appearance of the Saturn magnetic field due to Meissner phenomenon, all particles orbits are moving to the magnetic equator plane. Finally they become distributed as rings and gaps like iron particles around magnet on laboratory table. And they are separated from each other by the magnetic field expelled from them. It takes up to few tens of thousands years with ten meters rings disk thickness. Second, because of quantum locking all particles become to be locked within magnetic well at the magnetic equator plane due to Abrikosov vortex for superconductor. Finally each particle is locked within three-dimensional magnetic well. It works even when particles have small fraction of superconductor. During the rings evolution some contribution to the disk also could come from the collision-generated debris of the current moon, coming meteorites and from the geysers like it happened due to magnetic coupling of Saturn and Enceladus. The rings are relict of the early days of the magnetic field of Saturn system. 展开更多
关键词 ORIGIN of saturn RINGS Age of saturn RINGS SUPERCONDUCTIVITY of saturn RINGS QUANTUM LOCKING of saturn RINGS Space SUPERCONDUCTIVITY QUANTUM Phenomena in Space
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Astrometric Reduction of Saturnian Satellites with Cassini-ISS Images Degraded by Trailed Stars
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作者 Qing-Feng Zhang Meng-Qi Liu +4 位作者 Yan Li Lin-Peng Wu Zhi-Qiang Wang Li-Sha Zhu Zhan Li 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2023年第3期85-92,共8页
The Imaging Science Subsystem(ISS)mounted on the Cassini spacecraft has taken a lot of images,which provides an important source of high-precision astrometry of some planets and satellites.However,some of these images... The Imaging Science Subsystem(ISS)mounted on the Cassini spacecraft has taken a lot of images,which provides an important source of high-precision astrometry of some planets and satellites.However,some of these images are degraded by trailed stars.Previously,these degraded images cannot be used for astrometry.In this paper,a new method is proposed to detect and compute the centers of these trailed stars automatically.The method is then performed on the astrometry of ISS images with trailed stars.Finally,we provided 658 astrometric positions between 2004 and 2017 of several satellites that include Enceladus,Dione,Tethys,Mimas and Rhea.Compared with the JPL ephemeris SAT427,the mean residuals of these measurements are 0.11 km and 0.26 km in R.A.and decl.,respectively.Their standard deviations are 1.08 km and 1.37 km,respectively.The results show that the proposed method performs astrometric measurements of Cassini ISS images with trailed stars effectively. 展开更多
关键词 STARS TRAIL saturn
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SATURN软启动器在连铸机大包回转台电机控制中的应用
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作者 李祖林 《江苏电器》 2004年第1期25-26,共2页
介绍SATURN软启动器的结构和功能,阐述了软启动器在大包回转台控制中的应用和控制效果。
关键词 连铸机 大包回转台 电机控制 saturn 软启动器
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Preliminarily study of Saturn’s upper atmosphere density by observing Cassini plunging via China’s deep space station 被引量:1
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作者 Lue Chen Jin-Song Ping +10 位作者 Xiang Liu Na Wang Jian-Feng Cao Guang-Ming Chen Ming-Yuan Wang Wen-Xiao Li Jian-Hui Zhang Yong-Qiang Chen Shi-Lei Yue Song-Tao Han Jing Sun 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2020年第7期112-116,共5页
When the Cassini spacecraft finally plunged into the Saturnian atmosphere on 2017 September15,China’s deep space telescope pointed to Saturn to observe Cassini and study the Saturnian upper neutral atmosphere.In this... When the Cassini spacecraft finally plunged into the Saturnian atmosphere on 2017 September15,China’s deep space telescope pointed to Saturn to observe Cassini and study the Saturnian upper neutral atmosphere.In this first Chinese Saturnian radio science experiment,X band Doppler velocity radio science data between the deep space telescope and the Cassini spacecraft were obtained.After removing Saturnian and solar gravity effects,Earth rotation effect,the remaining Saturnian atmosphere drag information was retrieved in the Cassini final plunge progress.Saturn’s upper neutral atmosphere mass density profile is approximately estimated based on atmosphere mass density derived principally by real orbit measurement data.Saturn’s upper neutral atmosphere mass density from 76000 km to 1400 km is estimated from the orbit measurement data,the mass density results are about from 1.4×10^-15 kg cm^-3 to 2.5×10^-14 kg cm^-3. 展开更多
关键词 CASSINI saturn Doppler velocity neutral atmosphere mass density
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地层流体取样和压力测量Saturn 3D圆径探头 被引量:1
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作者 石钻 《石油钻探技术》 CAS CSCD 北大核心 2015年第1期26-26,共1页
地层流体取样和压力测量Saturn 3D圆径探头由Schlumberger公司研发,该探头设有4个自密封吸入口,每个吸入口的过流面积为128.1cm2,与常规探头相比,过流面积增大了500倍以上。4个吸入口间隔90°安装在探头上,从地层吸取流体。吸入口... 地层流体取样和压力测量Saturn 3D圆径探头由Schlumberger公司研发,该探头设有4个自密封吸入口,每个吸入口的过流面积为128.1cm2,与常规探头相比,过流面积增大了500倍以上。4个吸入口间隔90°安装在探头上,从地层吸取流体。吸入口装有过滤装置,当其靠在井壁上吸取地层流体时,可有效避免堵塞,使流体持续流动。该探头可实时监测滤液的清除情况,提取未污染的地层流体。该探头集成了地层动态测试器(MDT),一次起下作业即可完成大范围的产能测试、渗透试验及地层流体取样,从而建立储层预测模型,确定流体的组分和储层的连通性。 展开更多
关键词 地层流体 saturn 3D 吸入口 过流面积 测试器 压力测量 Schlumberger 过滤装置 储层预测 渗透试验
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A prediction method for ground-based stellar occultations by ellipsoidal solar system bodies and its application 被引量:3
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作者 Ye Yuan Yan-Ning Fu Zhuo Cheng 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2017年第5期65-78,共14页
A new programmable prediction method is developed to refine the occultation band by taking into consideration the triaxiality of an occulting body, as well as two more factors, namely, the barycenter offset of an occu... A new programmable prediction method is developed to refine the occultation band by taking into consideration the triaxiality of an occulting body, as well as two more factors, namely, the barycenter offset of an occulting planet from the relevant planetary satellite system and the gravitational deflection of light rays due to an occulting planet. Although these factors can be neglected in most cases, it is shown that there are cases when these factors can cause a variation ranging from several tens to thousands of kilometers in the boundaries of occultation bands. Knowledge of analytic geometry simplifies the process of derivation and computation. This method is applied to long-term predictions of Jovian and Saturnian events. 展开更多
关键词 shadow stellar saturn Jupiter uncertainty programmable planet offset derivation refine
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Saturne43型直线加速器光敏接收管受到辐射污染一例
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作者 李刚 周宇峰 李玉权 《医疗装备》 2001年第2期24-24,共1页
关键词 saturnE43型直线加速器 光敏接收管 辐射污染
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GE SATURNE 41医用直线加速器偏转系统工作原理及典型故障分析
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作者 陈利 《医疗装备》 2011年第11期69-69,共1页
本文介绍了GE SATURNE 41型医用直线加速器偏转系统的构成和工作原理,同时分析了典型故障的排除方法。
关键词 GE saturnE 41型医用直线加速器 偏转系统 故障分析
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新一代预调和测量设备:ZOLLER smile/saturn set
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《工具技术》 北大核心 2007年第3期93-93,共1页
关键词 saturn SMILE 测量设备 调和 小批量生产 机械系统 标准模式
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A model of Saturn inferred from its measured gravitational field
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作者 Dali Kong Keke Zhang +1 位作者 Gerald Schubert John D.Anderson 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2018年第4期7-14,共8页
We present an interior model of Saturn with an ice-rock core,a metallic region,an outer molecular envelope and a thin transition layer between the metallic and molecular regions.The shape of Saturn’s 1 bar surface is... We present an interior model of Saturn with an ice-rock core,a metallic region,an outer molecular envelope and a thin transition layer between the metallic and molecular regions.The shape of Saturn’s 1 bar surface is irregular and determined fully self-consistently by the required equilibrium condition.While the ice-rock core is assumed to have a uniform density,three different equations of state are adopted for the metallic,molecular and transition regions.The Saturnian model is constrained by its known mass,its known equatorial and polar radii,and its known zonal gravitational coefficients,J_(2n),n=1,2,3.The model produces an ice-rock core with equatorial radius 0.203 R_S,where R_S is the equatorial radius of Saturn at the 1-bar pressure surface;the core densityρ_c=10388.1 kgm^(3)corresponding to 13.06 Earth masses;and an analytical expression describing the Saturnian irregular shape of the 1-bar pressure level.The model also predicts the values of the higher-order gravitational coefficients,J_8,J_10 and J_12,for the hydrostatic Saturn and suggests that Saturn’s convective dynamo operates in the metallic region approximately defined by 0.2 R_S 展开更多
关键词 gravitation planets and satellites individual(saturn planets and satellites INTERIORS
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Saturn's gravitational field induced by its equatorially antisymmetric zonal winds
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作者 Dali Kong Keke Zhang +1 位作者 Gerald Schubert John D.Anderson 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2018年第5期29-36,共8页
The cloud-level zonal winds of Saturn are marked by a substantial equatorially antisymmetric component with a speed of about 50 m s^-1 which, if they are sufficiently deep, can produce measurable odd zonal gravitation... The cloud-level zonal winds of Saturn are marked by a substantial equatorially antisymmetric component with a speed of about 50 m s^-1 which, if they are sufficiently deep, can produce measurable odd zonal gravitational coefficients △J2 k+1, k = 1, 2, 3, 4. This study, based on solutions of the thermal-gravitational wind equation, provides a theoretical basis for interpreting the odd gravitational coefficients of Saturn in terms of its equatorially antisymmetric zonal flow. We adopt a Saturnian model comprising an ice-rock core, a metallic dynamo region and an outer molecular envelope. We use an equatorially antisymmetric zonal flow that is parameterized, confined in the molecular envelope and satisfies the solvability condition required for the thermal-gravitational wind equation. The structure and amplitude of the zonal flow at the cloud level are chosen to be consistent with observations of Saturn.We calculate the odd zonal gravitational coefficients △J2k+1, k = 1, 2, 3, 4 by regarding the depth of the equatorially antisymmetric winds as a parameter. It is found that △J3 is-4.197 × 10^-8 if the zonal winds extend about 13 000 km downward from the cloud tops while it is-0.765 × 10^-8 if the depth is about 4000 km. The depth/profile of the equatorially antisymmetric zonal winds can eventually be estimated when the high-precision measurements of the Cassini Grand Finale become available. 展开更多
关键词 gravitation - planets and satellites individual saturn - planets and satellites INTERIORS
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The effect of the equatorially symmetric zonal winds of Saturn on its gravitational field
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作者 Dali Kong Keke Zhang +1 位作者 Gerald Schubert John D.Anderson 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2018年第4期15-22,共8页
The penetration depth of Saturn’s cloud-level winds into its interior is unknown.A possible way of estimating the depth is through measurement of the effect of the winds on the planet’s gravitational field.We use a ... The penetration depth of Saturn’s cloud-level winds into its interior is unknown.A possible way of estimating the depth is through measurement of the effect of the winds on the planet’s gravitational field.We use a self-consistent perturbation approach to study how the equatorially symmetric zonal winds of Saturn contribute to its gravitational field.An important advantage of this approach is that the variation of its gravitational field solely caused by the winds can be isolated and identified because the leading-order problem accounts exactly for rotational distortion,thereby determining the irregular shape and internal structure of the hydrostatic Saturn.We assume that(i)the zonal winds are maintained by thermal convection in the form of non-axisymmetric columnar rolls and(ii)the internal structure of the winds,because of the Taylor-Proundman theorem,can be uniquely determined by the observed cloud-level winds.We calculate both the variation △J_n,n=2,4,6...of the axisymmetric gravitational coefficients J_n caused by the zonal winds and the non-axisymmetric gravitational coefficients △J_(nm) produced by the columnar rolls,where m is the azimuthal wavenumber of the rolls.We consider three different cases characterized by the penetration depth 0.36 R_S,0.2 R_S and 0.1 R_S,where R_S is the equatorial radius of Saturn at the 1-bar pressure level.We find that the high-degree gravitational coefficient ( J_(12)+△J_(12)) is dominated,in all the three cases,by the effect of the zonal flow with |△J_(12)/J_(12)|〉100%and that the size of the non-axisymmetric coefficientsdirectly reflects the depth and scale of the flow taking place in the Saturnian interior. 展开更多
关键词 gravitation planets and satellites individual(saturn planets and satellites INTERIORS
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Observations of loading-unloading process at Saturn's distant magnetotail
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作者 ZhongHua Yao 《Earth and Planetary Physics》 2017年第1期53-57,共5页
Using in-situ measurements from the Cassini spacecraft in 2013, we report an Earth substorm-like loading-unloading process at Saturn's distant magnetotail. We found that the loading process is featured with two di... Using in-situ measurements from the Cassini spacecraft in 2013, we report an Earth substorm-like loading-unloading process at Saturn's distant magnetotail. We found that the loading process is featured with two distinct processes: a rapid loading process that was likely driven by an internal source and a slow loading process that was likely driven by solar wind. Each of the two loading processes could also individually lead to an unloading process. The rapid internal loading process lasts for ~ 1-2 hours; the solar wind driven loading process lasts for ~ 3-18 hours and the following unloading process lasts for ~1-3 hours. In this letter, we suggest three possible loadingunloading circulations, which are fundamental in understanding the role of solar wind in driving giant planetary magnetospheric dynamics. 展开更多
关键词 saturn magnetosphere loading-unloading process magnetic reconnection DIPOLARIZATION
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About Role of Electromagnetism to the Saturn Rings Origin<br/>—To the Unified Theory of the Planetary Rings Origin
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作者 Vladimir V. Tchernyi 《International Journal of Astronomy and Astrophysics》 2013年第4期412-420,共9页
Experimental data observation of the Saturn rings points to the conjecture that the particles constituting the rings may be superconductive. The main argument for this based on the fact that Saturn has a magnetic fiel... Experimental data observation of the Saturn rings points to the conjecture that the particles constituting the rings may be superconductive. The main argument for this based on the fact that Saturn has a magnetic field and the temperature in its vicinity is low enough. Electromagnetic modeling shows the rings system emerges some time after appearance of the planetary magnetic field. Rings can be a result of the interaction of the superconducting carbon doped ice particles of the protoplanetary cloud with the nonuniform magnetic field. At the beginning all Keplerian orbits of the particles are located within protoplanetary cloud. After appearance of the magnetic field of Saturn, all iced particles demonstrate superconductivity and their orbits start to move to the magnetic equator plane where there is a minimum of magnetic energy. And then particles redistributed like iron particles nearby magnet on laboratory table forming system of rings and gaps. But rings particles are not stuck together because of Meissner phenomenon. The gravitational resonances and other interactions also play an important role and they help bring the order to the system of rings and gaps. It becomes to be clear why the rings appear only for the planets with magnetic field outside the asteroid belt such as Jupiter, Saturn, Uranus and Neptune. Inside the asteroid belt Sun’s heat is destroying superconductivity. Scenario of the rings creation for all planets could be the same. So we are coming to the unified theory of the rings origin. The presented model allows enriching the well-known theories that treat gravitational, mechanical, gas-plasma, dusty plasma and magnetohydrodynamic interactions in a consistent way. 展开更多
关键词 saturn system saturn RINGS ORIGIN saturn RINGS Electromagnetism saturn RINGS SUPERCONDUCTIVITY ORIGIN of PLANETARY RINGS SPACE Electromagnetism SPACE SUPERCONDUCTIVITY
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Space Magnetism and Superconductivity: Diamagnetic Expulsion, Meissner Effect, Magnetic Pressure and Quantum Trapping Lead to the Origin and Stability of the Saturn Rings
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作者 Vladimir V. Tchernyi (Cherny) Andrey Yu. Pospelov Sergey V. Kapranov 《Journal of Applied Mathematics and Physics》 2019年第8期1625-1636,共12页
Existence of the magnetic field of Saturn and the temperature around 70 - 100 K nearby of it bring us to the idea of diamagnetism and superconductivity of the rings particles. The rings could emerge from the icy parti... Existence of the magnetic field of Saturn and the temperature around 70 - 100 K nearby of it bring us to the idea of diamagnetism and superconductivity of the rings particles. The rings could emerge from the icy particles moving on chaotic orbits around Saturn within protoplanetary cloud. After appearance of the magnetic field of Saturn all chaotic orbits of icy particles start to shift to the magnetic equator plane, where there is a minimum of the particles magnetic energy, due to diamagnetic force of expulsion like Meissner phenomenon. Each particle comes to the stable position preventing its own horizontal and vertical shift. Particles are locked within three-dimensional magnetic well due to Abrikosov quantum vortex phenomenon for superconductor. This mechanism is valid and it works even particles have a small fraction of superconductor. Final picture is similar to the picture of iron particles forms the same shape around a magnet on laboratory table. Any other phenomena like gravity resonances, dusty plasma and others may bring some peculiarities to the final picture of the rings. It follows that magnetic field of Saturn and low temperature around of it are the main reason for the rings origin and the rings is product of the early time of the magnetic field of Saturn appearance. Additional matter to the rings also may come from the frozen water particles generated from the Saturn sputniks geysers due to magnetic coupling between planet and satellites. The data of Cassini mission to Saturn rings are conforming suggested theory of their origin and existence. 展开更多
关键词 saturn Rings ORIGIN SPACE MAGNETISM SPACE DIAMAGNETISM SPACE SUPERCONDUCTIVITY SPACE Ice
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Energy Gap in Saturn’s Rings
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作者 Andrey Yu Pospelov Vladimir V. Tchernyi 《Journal of Modern Physics》 2019年第4期477-485,共9页
In this article, we consider, based on the super-diamagnetic model, the new problems of Saturn’s rings discovered by Cassini, such as: 1) anomalous purity of water ice;2) Saturn’s magnetic field alignment with the p... In this article, we consider, based on the super-diamagnetic model, the new problems of Saturn’s rings discovered by Cassini, such as: 1) anomalous purity of water ice;2) Saturn’s magnetic field alignment with the planet’s rotation axis;3) “ring rain” of the submicron particles;4) the deviation in the qualitative composition of the “rain” from the composition of the rings;5) “dirt” concentrated in the ring gaps;6) “plateaus” in Saturn’s C ring;7) age of the rings;8) roll-off in the spectrum of Saturn’s rings, and 9) “propellers” in Saturn’s A ring. Interpretation of Cassini’s observations of spectral roll-off in Saturn’s rings in the wavelength range from 100 micrometers to 0.5 mm is given. It was concluded that the substance of the rings could be in the superconducting state. An explanation of the Cassini spectral data is given using the hypothesis of the existence of a superconducting energy gap in the substance of rings. 展开更多
关键词 saturn RINGS CASSINI CIRS Interpretation Super-Diamagnetic Model Superconducting Energy Gap Ring RAIN PLATEAUS and PROPELLERS in saturn’s RINGS
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Could Superconductivity Contribute to the Saturn Rings Origin?
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作者 Vladimir V. Tchernyi (Cherny) 《Journal of Modern Physics》 2013年第6期17-23,共7页
The article shows how the phenomenon of superconductivity can contribute to the origin of Saturn rings. The main argument for this coming from the general physics consideration and based on the fact that Saturn has a ... The article shows how the phenomenon of superconductivity can contribute to the origin of Saturn rings. The main argument for this coming from the general physics consideration and based on the fact that Saturn has a magnetic field, and the temperature of the environment in its vicinity is low enough to think about superconductivity. 展开更多
关键词 ORIGIN of saturn RINGS ORIGIN of PLANETARY RINGS SUPERCONDUCTIVITY of the PLANETARY RINGS
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Superconductivity of Saturn Rings: Quantum Locking, Rings Disc Thickness and Its Time Creation
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作者 Vladimir V. Tchernyi Andrew Yu Pospelov 《Journal of Modern Physics》 2018年第3期419-432,共14页
The article demonstrates how rings disc of Saturn was created after appearance of the planetary magnetic field from superconducting iced particles of the protoplanetary cloud moving around planet by chaotic orbits. It... The article demonstrates how rings disc of Saturn was created after appearance of the planetary magnetic field from superconducting iced particles of the protoplanetary cloud moving around planet by chaotic orbits. It is based on the fact that Saturn has magnetic field and the temperature of its vicinity is low enough to have superconductivity. Electromagnetic simulation estimates time of rings disc formation with the thickness about few meters from a few thousand years up to few tens of thousands of years. A rings disk has a stable structure located within magnetic equator of Saturn due to quantum locking of the particles by planetary magnetic field. Also may happened contribution to the rings disc from the debris of the moons migrated inward towards Saturn and particles of the frozen water coming from the geyser of the geologically active satellite (as Enceladus contributed to the E-ring). Suggested mechanism of the rings formation works even in case where only a small fraction of the particles poses superconductivity. Presented electromagnetic modeling of the role of superconducting iced particles of the rings disc origin, dynamics and evolution allow us to enrich the classical theories based on gravitational, mechanical, magnetohydrodynamic and plasma interactions. 展开更多
关键词 ORIGIN of saturn RINGS ORIGIN of PLANETARY RINGS SUPERCONDUCTIVITY of the PLANETARY RINGS
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