The main activities of Chinese space solar physics in 2012–2014 include: to continue studying the mid and long-term(2016–2030) plan of Chinese space solar physics; to arrange a group of pre-study projects of space s...The main activities of Chinese space solar physics in 2012–2014 include: to continue studying the mid and long-term(2016–2030) plan of Chinese space solar physics; to arrange a group of pre-study projects of space solar physics; to initiate and continue a few solar mission-level projects.This paper summarizes all these activities briefly.展开更多
In the first part of this paper,we describe briefly the mid and long-term plan of Chinese space astronomy,its preliminary study program,the current status of satellite missions undertaken, and the current status of as...In the first part of this paper,we describe briefly the mid and long-term plan of Chinese space astronomy,its preliminary study program,the current status of satellite missions undertaken, and the current status of astronomy experiments in China's manned space flight program.In the second part,the recent research progress made in the fields of solar physics is summarized briefly, including solar vector magnetic field,solar flares,CME and filaments,solar radio and nonthermal processes,EUV waves,MHD waves and coronal waves,solar model and helioseismology,solar wind and behavior of solar cycle.展开更多
Magnetospheric physics has been one of the most active areas in Chinese space research in past two years. The major project "Energy Transport Processes in the Solar-Terrestrial System" (1993-1997) sponsored ...Magnetospheric physics has been one of the most active areas in Chinese space research in past two years. The major project "Energy Transport Processes in the Solar-Terrestrial System" (1993-1997) sponsored by the National Natural Science Foundation in China (NSFC) has been successfully completed. Prestudies relevant to the key scientific engineering program "Meridian Chain at One Hundred Twenty Degree East Multi-Station and Multi-Instrument Observatory System" have started. A new key project "Study of Auroral Magnetospheric and Ionospheric Physics" (1997-1999) sponsored by the NSFC has begun. The Space Active Experiment Program has been carrying on further.Collaborations between Chinese and international magnetospheric physicists have proceeded forward. More than 40 papers covering a variety of subjects in the magnetospheric physics were published in Chinese and international academic journals. Most of these works were supported by the NSFC. This report provides a brief summary of aforementioned advances made in China in the past two years.展开更多
This brief report presents the latest advances of the magnetospheric physics researches in China during the period of 2002-2004. The progress of the magnetospheric space mission DSP is given in another dedicated paper...This brief report presents the latest advances of the magnetospheric physics researches in China during the period of 2002-2004. The progress of the magnetospheric space mission DSP is given in another dedicated paper of this issue.展开更多
Their brief report presents the advances of the magnetospheric physics researches in China during the period of 2004-2006. During the past two years, China-ESA cooperation DSP (Double Star Program) satellites were suc...Their brief report presents the advances of the magnetospheric physics researches in China during the period of 2004-2006. During the past two years, China-ESA cooperation DSP (Double Star Program) satellites were successively launched. In addition, China also participated in the scientific research of ESA's Cluster mission. The DSP and Cluster missions provide Chinese space physicists high quality data to study multiscale physical process in the magnetosphere. The work made based on the data of DSP is presented in the paper of "Progress of Double Star Program" of this issue.展开更多
This brief report presents the latest advances of the magnetospheric physics researches in China during the period of 2000-2002, made independently by Chinese space physicists and through international cooperation. Th...This brief report presents the latest advances of the magnetospheric physics researches in China during the period of 2000-2002, made independently by Chinese space physicists and through international cooperation. The related areas cover almost every aspect of magnetospheric physics.展开更多
The activities of Chinese space solar physics in 2018–2020 are going on smoothly.Besides the missions of ASO-S and CHASE which are in the engineering phases,there are quite a number of projects which are in the pre-s...The activities of Chinese space solar physics in 2018–2020 are going on smoothly.Besides the missions of ASO-S and CHASE which are in the engineering phases,there are quite a number of projects which are in the pre-study stage(conception study)or have finished the pre-study stage,constituting a rich pond for the selection of next solar mission(s).This paper describes in brief the status of all these related projects.展开更多
In the past two years, many progresses have been made in magnetospheric physics by using the data of Double Star Program, Cluster, THEMIS and RBSP missions, or by computer simulations. This paper briefly reviews these...In the past two years, many progresses have been made in magnetospheric physics by using the data of Double Star Program, Cluster, THEMIS and RBSP missions, or by computer simulations. This paper briefly reviews these works based on papers selected from the 126 publications from March 2012 to March 2014. The subjects cover various sub-branches of magnetospheric physics,including geomagnetic storm, magnetospheric substorm and magnetic reconnection.展开更多
MEASURING WORKLOAD WITH PAIRED DETECTORS Robert Corns1,Charles Schroeder2,Gurpreet Sandhu3,Keith Henderson4,Ian Mc Kay4(1.East Carolina University,Brody School of Medicine,Department of Radiation Oncology,Greenville,N...MEASURING WORKLOAD WITH PAIRED DETECTORS Robert Corns1,Charles Schroeder2,Gurpreet Sandhu3,Keith Henderson4,Ian Mc Kay4(1.East Carolina University,Brody School of Medicine,Department of Radiation Oncology,Greenville,NC;2. Medical Physics,Cancer Care Manitoba,Winnipeg,Manitoba,Canada;3. Department of Medical Physics,British Columbia Cancer—Surrey,British Columbia,Canada;4. National Dosimetry Services,Health Canada,Ottawa,Ontario,Canada)展开更多
In the past two years,many progresses are made in magnetospheric physics by using either the data of Double Star Program,Cluster and THEMIS missions,or by computer simulations. This paper briefly reviews these works b...In the past two years,many progresses are made in magnetospheric physics by using either the data of Double Star Program,Cluster and THEMIS missions,or by computer simulations. This paper briefly reviews these works based on papers selected from the 80 publications from April 2010 to April 2011.The subjects covered various sub-branches of magnetospheric physics,including geomagnetic storm,magnetospheric substorm,etc.展开更多
THE INFLUENCE OF MAGNETIC FIELDS (0. 05 T≤B≤7 T) ON THE RESPONSE OF PERSONAL THERMOLUMINESCENT DOSIMETERS TO IONIZING RADIATION Atallah Copty1,Günter Rabineg1,Andreas Berg2,3(1. Radiation Protection Laboratory,...THE INFLUENCE OF MAGNETIC FIELDS (0. 05 T≤B≤7 T) ON THE RESPONSE OF PERSONAL THERMOLUMINESCENT DOSIMETERS TO IONIZING RADIATION Atallah Copty1,Günter Rabineg1,Andreas Berg2,3(1. Radiation Protection Laboratory,Vienna City Administration,Vienna,Austria;2. Center for Medical Physics and Biomedical Engineering,Medical University of Vienna,Vienna,Austria;3. High-field MR Centre,Medical University of Vienna/AKH,Vienna,Austria)展开更多
The progress on Chinese Space Solar Telescope (SST) in 2002-2004 is introduced. The documentations on plans and outlines based on the standards of Chinese aerospace industry for SST mission has been fulfilled. The key...The progress on Chinese Space Solar Telescope (SST) in 2002-2004 is introduced. The documentations on plans and outlines based on the standards of Chinese aerospace industry for SST mission has been fulfilled. The key technical problems of SST satellite platform and payloads are tackled during pre-study stage of the mission. The laboratory assembly and calibration of the main optical telescope of 1.2 m spherical mirror and 1 m plain mirror have been carried out with the accuracy of λ/40 and λ/30, respectively. The prototype at 17.1 nm for extreme ultraviolet telescope is under development and manufacture with a diameter of 13 cm. Its primary and secondary mirrors have a manufacturing error of 5 nm with a roughness degree of less than 0.5 nm and a multiplayer reflection factor of better than 20%. The on-board scientific data processing unit has been developed. Prototypes for other payloads such as H. and white light telescope, wide band spectroscopy in high energy and solar and interplanetary radio spectrometer have been developed accordingly.展开更多
In the past two years,many progresses were made in Magnetospheric Physics by using the data of SuperMAG,Double Star Program,Cluster,THEMIS,RBSP,DMSP,DEMETER,NOAA,Van Allen probe,Swarm,MMS,ARTEMIS,MESSENGER,Fengyun,Bei...In the past two years,many progresses were made in Magnetospheric Physics by using the data of SuperMAG,Double Star Program,Cluster,THEMIS,RBSP,DMSP,DEMETER,NOAA,Van Allen probe,Swarm,MMS,ARTEMIS,MESSENGER,Fengyun,BeiDa etc.,or by computer simulations.This paper briefly reviews these works based on papers selected from the 248 publications from January 2018 to December 2019.The subjects covered various sub-branches of Magnetospheric Physics,including geomagnetic storm,magnetospheric substorm,magnetic reconnection,solar wind-magnetosphere-ionosphere interaction,radiation belt,ring current,whistler waves,plasmasphere,outer magnetosphere,magnetotail,planetary magnetosphere,and technique.展开更多
Device physics research for submicron and deep submicron space microelectronics devices and integrated circuits will be described in three topics.1.Thin film submicron and deep submicron SOS / CMOS devices and integra...Device physics research for submicron and deep submicron space microelectronics devices and integrated circuits will be described in three topics.1.Thin film submicron and deep submicron SOS / CMOS devices and integrated circuits.2.Deep submicron LDD CMOS devices and integrated circuits.3.C band and Ku band microwave GaAs MESFET and III-V compound hetrojunction HEM T and HBT devices and integrated circuits.展开更多
The solar physics studies in China during 2004-2006 from solar interior to solar atmospheres and solar-interplanetary space are summarized. These researches are arranged under the topics of solar interior, photosphere...The solar physics studies in China during 2004-2006 from solar interior to solar atmospheres and solar-interplanetary space are summarized. These researches are arranged under the topics of solar interior, photosphere, chromosphere and transition region, corona, flares and CMEs (and the associated radio bursts, X-ray/γ-ray bursts and particle acceleration), solar wind, solar cycle, and ground-based instrumentation.展开更多
To follow up the last report two years ago,what happened from 2020 to 2022 deserves specially mentioning:CHASE was successfully launched on 14 October 2021;ASO-S will finish soon its Phase-D study and is scheduled for...To follow up the last report two years ago,what happened from 2020 to 2022 deserves specially mentioning:CHASE was successfully launched on 14 October 2021;ASO-S will finish soon its Phase-D study and is scheduled for launch in October 2022;four solar mission candidates are being undertaken the engineering project evaluations;three solar mission proposals are being undertaken the background project evaluations;there are also quite a number of pre-study space solar physics projects getting either newly supported or finished.This paper describes in brief the status of all these related projects.展开更多
In this paper,a scheme of commonly-resonated extended interaction circuit system based on high order TMn,mode is proposed to lock the phases of two extended interaction oscillators(EIOs)for generating high power at G-...In this paper,a scheme of commonly-resonated extended interaction circuit system based on high order TMn,mode is proposed to lock the phases of two extended interaction oscillators(EIOs)for generating high power at G-band.Two separate EIOs are coupled through a specific single-gap coupling field supported by a designed gap waveguide with length Lg,which form the phase-locked EIOs based on the commonly-resonated system.As a whole system,the system has been focused on with mode analysis based on different single-gap coupling fields,mode hopping,which present the variation of phase difference between the two-beam-wave interactions when changing Lg.To demonstrate the effectiveness of the proposed circuit system in producing the phase locking,we conducted particle-in-cell(PIC)simulations to show that the interesting mode hopping occurs with the phase difference of O and r between the output signals from two output ports,corresponding to the excitation of the TMn mode with different n.Simulation results show that 1)the oscillator can deliver two times of the output power obtained from one single oscillator at 220 GHz,2)the two EIOs can still deliver output signals with phase difference of O and when the currents of the two beams are different or the fabrication errors of the two EIO cavities are taken into account.The proposed scheme is promising in extending to phase locking between multiple EIOs,and generating higher power at millimeter-wave and higher frequencies.展开更多
文摘The main activities of Chinese space solar physics in 2012–2014 include: to continue studying the mid and long-term(2016–2030) plan of Chinese space solar physics; to arrange a group of pre-study projects of space solar physics; to initiate and continue a few solar mission-level projects.This paper summarizes all these activities briefly.
文摘In the first part of this paper,we describe briefly the mid and long-term plan of Chinese space astronomy,its preliminary study program,the current status of satellite missions undertaken, and the current status of astronomy experiments in China's manned space flight program.In the second part,the recent research progress made in the fields of solar physics is summarized briefly, including solar vector magnetic field,solar flares,CME and filaments,solar radio and nonthermal processes,EUV waves,MHD waves and coronal waves,solar model and helioseismology,solar wind and behavior of solar cycle.
文摘Magnetospheric physics has been one of the most active areas in Chinese space research in past two years. The major project "Energy Transport Processes in the Solar-Terrestrial System" (1993-1997) sponsored by the National Natural Science Foundation in China (NSFC) has been successfully completed. Prestudies relevant to the key scientific engineering program "Meridian Chain at One Hundred Twenty Degree East Multi-Station and Multi-Instrument Observatory System" have started. A new key project "Study of Auroral Magnetospheric and Ionospheric Physics" (1997-1999) sponsored by the NSFC has begun. The Space Active Experiment Program has been carrying on further.Collaborations between Chinese and international magnetospheric physicists have proceeded forward. More than 40 papers covering a variety of subjects in the magnetospheric physics were published in Chinese and international academic journals. Most of these works were supported by the NSFC. This report provides a brief summary of aforementioned advances made in China in the past two years.
文摘This brief report presents the latest advances of the magnetospheric physics researches in China during the period of 2002-2004. The progress of the magnetospheric space mission DSP is given in another dedicated paper of this issue.
基金Supported by the National Natural Science Foundation of China (40523006, 40390153, 40474062), International Collaboration Research Team Program and Bairen Plan of Chinese Academy of Sciences
文摘Their brief report presents the advances of the magnetospheric physics researches in China during the period of 2004-2006. During the past two years, China-ESA cooperation DSP (Double Star Program) satellites were successively launched. In addition, China also participated in the scientific research of ESA's Cluster mission. The DSP and Cluster missions provide Chinese space physicists high quality data to study multiscale physical process in the magnetosphere. The work made based on the data of DSP is presented in the paper of "Progress of Double Star Program" of this issue.
基金Supported by the National Natural Science Foundation of China through grant No.40025413
文摘This brief report presents the latest advances of the magnetospheric physics researches in China during the period of 2000-2002, made independently by Chinese space physicists and through international cooperation. The related areas cover almost every aspect of magnetospheric physics.
基金Supported by Chinese Academy of Sciences(XDA15052200)by National Natural Science Foundation of China(U1731241,11921003 and U1931138)。
文摘The activities of Chinese space solar physics in 2018–2020 are going on smoothly.Besides the missions of ASO-S and CHASE which are in the engineering phases,there are quite a number of projects which are in the pre-study stage(conception study)or have finished the pre-study stage,constituting a rich pond for the selection of next solar mission(s).This paper describes in brief the status of all these related projects.
文摘In the past two years, many progresses have been made in magnetospheric physics by using the data of Double Star Program, Cluster, THEMIS and RBSP missions, or by computer simulations. This paper briefly reviews these works based on papers selected from the 126 publications from March 2012 to March 2014. The subjects cover various sub-branches of magnetospheric physics,including geomagnetic storm, magnetospheric substorm and magnetic reconnection.
文摘MEASURING WORKLOAD WITH PAIRED DETECTORS Robert Corns1,Charles Schroeder2,Gurpreet Sandhu3,Keith Henderson4,Ian Mc Kay4(1.East Carolina University,Brody School of Medicine,Department of Radiation Oncology,Greenville,NC;2. Medical Physics,Cancer Care Manitoba,Winnipeg,Manitoba,Canada;3. Department of Medical Physics,British Columbia Cancer—Surrey,British Columbia,Canada;4. National Dosimetry Services,Health Canada,Ottawa,Ontario,Canada)
文摘In the past two years,many progresses are made in magnetospheric physics by using either the data of Double Star Program,Cluster and THEMIS missions,or by computer simulations. This paper briefly reviews these works based on papers selected from the 80 publications from April 2010 to April 2011.The subjects covered various sub-branches of magnetospheric physics,including geomagnetic storm,magnetospheric substorm,etc.
文摘THE INFLUENCE OF MAGNETIC FIELDS (0. 05 T≤B≤7 T) ON THE RESPONSE OF PERSONAL THERMOLUMINESCENT DOSIMETERS TO IONIZING RADIATION Atallah Copty1,Günter Rabineg1,Andreas Berg2,3(1. Radiation Protection Laboratory,Vienna City Administration,Vienna,Austria;2. Center for Medical Physics and Biomedical Engineering,Medical University of Vienna,Vienna,Austria;3. High-field MR Centre,Medical University of Vienna/AKH,Vienna,Austria)
文摘The progress on Chinese Space Solar Telescope (SST) in 2002-2004 is introduced. The documentations on plans and outlines based on the standards of Chinese aerospace industry for SST mission has been fulfilled. The key technical problems of SST satellite platform and payloads are tackled during pre-study stage of the mission. The laboratory assembly and calibration of the main optical telescope of 1.2 m spherical mirror and 1 m plain mirror have been carried out with the accuracy of λ/40 and λ/30, respectively. The prototype at 17.1 nm for extreme ultraviolet telescope is under development and manufacture with a diameter of 13 cm. Its primary and secondary mirrors have a manufacturing error of 5 nm with a roughness degree of less than 0.5 nm and a multiplayer reflection factor of better than 20%. The on-board scientific data processing unit has been developed. Prototypes for other payloads such as H. and white light telescope, wide band spectroscopy in high energy and solar and interplanetary radio spectrometer have been developed accordingly.
基金Supported by National Natural Science Foundation of China Grants(41821003,41941001)。
文摘In the past two years,many progresses were made in Magnetospheric Physics by using the data of SuperMAG,Double Star Program,Cluster,THEMIS,RBSP,DMSP,DEMETER,NOAA,Van Allen probe,Swarm,MMS,ARTEMIS,MESSENGER,Fengyun,BeiDa etc.,or by computer simulations.This paper briefly reviews these works based on papers selected from the 248 publications from January 2018 to December 2019.The subjects covered various sub-branches of Magnetospheric Physics,including geomagnetic storm,magnetospheric substorm,magnetic reconnection,solar wind-magnetosphere-ionosphere interaction,radiation belt,ring current,whistler waves,plasmasphere,outer magnetosphere,magnetotail,planetary magnetosphere,and technique.
文摘Device physics research for submicron and deep submicron space microelectronics devices and integrated circuits will be described in three topics.1.Thin film submicron and deep submicron SOS / CMOS devices and integrated circuits.2.Deep submicron LDD CMOS devices and integrated circuits.3.C band and Ku band microwave GaAs MESFET and III-V compound hetrojunction HEM T and HBT devices and integrated circuits.
基金Supported by MOST (G20000784, Natinal Natural Science Foundation of China (10225313, 10333030) and the Chinese Academy of Sciences
文摘The solar physics studies in China during 2004-2006 from solar interior to solar atmospheres and solar-interplanetary space are summarized. These researches are arranged under the topics of solar interior, photosphere, chromosphere and transition region, corona, flares and CMEs (and the associated radio bursts, X-ray/γ-ray bursts and particle acceleration), solar wind, solar cycle, and ground-based instrumentation.
基金Supported by Strategic Priority Research Program of the Chinese Academy of Sciences(XDA15052200)National Natural Science Foundation of China(11921003,U1931138)。
文摘To follow up the last report two years ago,what happened from 2020 to 2022 deserves specially mentioning:CHASE was successfully launched on 14 October 2021;ASO-S will finish soon its Phase-D study and is scheduled for launch in October 2022;four solar mission candidates are being undertaken the engineering project evaluations;three solar mission proposals are being undertaken the background project evaluations;there are also quite a number of pre-study space solar physics projects getting either newly supported or finished.This paper describes in brief the status of all these related projects.
基金Supported in part by the National Natural Science Foundation of China(62401125)the Natural Science Foundation of Sichuan Province(2023NSFSC1376)the Fundamental Research Funds for the Central Universities(ZYGX2024J008)。
文摘In this paper,a scheme of commonly-resonated extended interaction circuit system based on high order TMn,mode is proposed to lock the phases of two extended interaction oscillators(EIOs)for generating high power at G-band.Two separate EIOs are coupled through a specific single-gap coupling field supported by a designed gap waveguide with length Lg,which form the phase-locked EIOs based on the commonly-resonated system.As a whole system,the system has been focused on with mode analysis based on different single-gap coupling fields,mode hopping,which present the variation of phase difference between the two-beam-wave interactions when changing Lg.To demonstrate the effectiveness of the proposed circuit system in producing the phase locking,we conducted particle-in-cell(PIC)simulations to show that the interesting mode hopping occurs with the phase difference of O and r between the output signals from two output ports,corresponding to the excitation of the TMn mode with different n.Simulation results show that 1)the oscillator can deliver two times of the output power obtained from one single oscillator at 220 GHz,2)the two EIOs can still deliver output signals with phase difference of O and when the currents of the two beams are different or the fabrication errors of the two EIO cavities are taken into account.The proposed scheme is promising in extending to phase locking between multiple EIOs,and generating higher power at millimeter-wave and higher frequencies.
