AIM:To explore the clinical and pathological characteristics of thirteen patients with orbital liposarcoma.METHODS:The clinical history data of thirteen patients diagnosed as orbital liposarcoma at Beijing Tongren Hos...AIM:To explore the clinical and pathological characteristics of thirteen patients with orbital liposarcoma.METHODS:The clinical history data of thirteen patients diagnosed as orbital liposarcoma at Beijing Tongren Hospital,from 2006 to 2021 were collected and analyzed.The data includes age,gender,affected orbital side,course of disease,status of disease(primary or recurrent),clinical manifestations,preoperative visual acuity,operative treatment,the relations between liposarcoma and surrounding tissue,longest diameter of liposarcoma,histological subtype,immunohistochemical indicators,follow-up treatment and prognosis.RESULTS:The initial symptoms are diverse.Proptosis is the most frequent chief complaint and the others included vision loss,epiphora,diplopia,and eyelid palpable mass.Results of imaging examination[computed tomography(CT)or magnetic resonance imaging(MRI)]showed orbital mass.In terms of treatment,10 patients received tumor resection,and the mean longest diameter of the tumor was 3.39±1.36 cm.The other 3 patients had optic nerve invaded,so they received orbital exenteration.Pathological examination results confirmed the diagnose of liposarcoma for 13 patients.Six patients displayed as myxoid type,and three patients in each type of dedifferentiated and welldifferentiated type.One patient was verified as pleomorphic,which was a rare type of liposarcoma.All of the patients showed Vimentin positive,and most showed CD34 and S-100 positive.Besides,four patients showed smooth muscle actin positive.All thirteen patients were alive.CONCLUSION:Orbital liposarcoma is a rare disease and it has no specific clinical manifestation.The diagnosis of liposarcoma should be considered when proptosis and orbital mass occurred in orbit.It is recommended to perform pathological examination to achieve early detection and early treatment.展开更多
Recent measurements have shown that gravitational waves and thus the gravitational interaction propagate with the speed of light. The propagation delay of the gravitational interaction in orbiting systems couples the ...Recent measurements have shown that gravitational waves and thus the gravitational interaction propagate with the speed of light. The propagation delay of the gravitational interaction in orbiting systems couples the orbital and center of mass motions. This causes the orbits to spiral out and the center of mass to accelerate. It is one of a number of small effects modifying the Kepler orbits. The calculations show that the analytical describable expansion of the semimajor axis started at a time that is less than the age of the systems. This could be caused by a collision of a system component in the past. The effect of this propagation delay on the motion of the Earth Moon and the Brown Dwarf 569Bab binary star system is analyzed. These systems were chosen because a considerable amount of measured astronomical data is available. The calculated results are in excellent agreement with the measured data. In galaxies, too, the energy transfer from the orbit of the star cloud to the center of mass motion causes the galaxies to ac-celerate. If galaxies are considered to be molecules of the universe, then the acceleration of the galaxies will cause the molecular gas to heat and expand. Alternatively, the loss in orbital internal energy of the galaxies should be included in the mass and energy in the calculation of the expanding Universe.展开更多
Spacecrafts with the pure gravity environment are of great significance in precision navigation, gravity field measurement for celestial bodies, and basic physics ex- periments. The radiometer effect is one of the imp...Spacecrafts with the pure gravity environment are of great significance in precision navigation, gravity field measurement for celestial bodies, and basic physics ex- periments. The radiometer effect is one of the important interfering factors on the proof mass in a purely gravitational orbit. For the gravity field measurement system based on the inner-formation flying, the relationship between the radiometer effect on the inner- satellite and the system parameters is studied by analytical and numerical methods. An approximate function of the radiometer effect suitable for the engineering computation and the correction factor are obtained. The analytic results show that the radiometer effect on the inner-satellite is proportional to the average pressure while inversely pro- portional to the average temperature in the outer-satellite cavity. The radiometer effect increases with the temperature difference in the cavity, and its minimum exists when the cavity radius increases. When the minimum of the radiometer effect arrives, the ratio of the cavity radius to the inner-satellite radius is 1.189 4. This constant is determined by the spherical cavity configuration and independent of the temperature and pressure distributions. When the ratio of the cavity radius to the inner-satellite radius is more than 10, it is believed that the cavity is large enough, the radiometer effect is approxi- mately proportional to the square of the inner-satellite radius, and the influence of the outer-satellite cavity radius on the radiometer effect can be ignored.展开更多
AIM:To characterize spectral-domain optical coherence tomography(SD-OCT)features of chorioretinal folds in orbital mass imaged using enhanced depth imaging(EDI).METHODS:Prospective observational case-control study was...AIM:To characterize spectral-domain optical coherence tomography(SD-OCT)features of chorioretinal folds in orbital mass imaged using enhanced depth imaging(EDI).METHODS:Prospective observational case-control study was conducted in 20 eyes of 20 patients,the uninvolved eye served as a control.All the patients underwent clinical fundus photography,computed tomography,EDI SDOCT imaging before and after surgery.Two patients with cavernous hemangiomas underwent intratumoral injection of bleomycin A5;the remaining patients underwent tumor excision.Patients were followed 1 to 14mo following surgery(average follow up,5.8mo).RESULTS:Visual acuity prior to surgery ranged from 20/20 to 20/200.Following surgery,5 patients’visual acuity remained unchanged while the remaining 15 patients had a mean letter improvement of 10(range 4 to 26 letters).Photoreceptor inner/outer segment defects were found in 10 of 15 patients prior to surgery.Following surgical excision,photoreceptor inner/outer segment defects fully resolved in 8 of these 10 patients.CONCLUSION:Persistence of photoreceptor inner/outer segment defects caused by compression of the globe by an orbital mass can be associated with reduced visual prognosis.Our findings suggest that photoreceptor inner/outer segment defects on EDI SD-OCT could be an indicator for immediate surgical excision of an orbital mass causing choroidal compression.展开更多
目的研究清瘟护肺颗粒的化学成分。方法查阅中国知网、PubMed、Web of Science等数据库,检索该制剂组方药材化学成分的相关文献,结合文献报道和ChemicalBook数据库信息,建立化学成分数据库。采用超高效液相色谱-四极杆/静电场轨道阱高...目的研究清瘟护肺颗粒的化学成分。方法查阅中国知网、PubMed、Web of Science等数据库,检索该制剂组方药材化学成分的相关文献,结合文献报道和ChemicalBook数据库信息,建立化学成分数据库。采用超高效液相色谱-四极杆/静电场轨道阱高分辨质谱(UHPLC-Q Exactive Focus MS/MS)法分析制剂的图谱数据,并以Xcalibur 4.0软件拟合分子式,与自建数据库信息进行匹配,初步推测分子式信息,与ChemicalBook或ChemSpider数据库比对,推测化学成分结构。结果共鉴定出158个化学成分,包括苷类36个,黄酮类29个,苯丙素类28个,有机酸类18个,萜类17个,色原酮类8个,其他类22个。结论所建立的方法可系统、准确、快速地定性分析清瘟护肺颗粒中的化学成分。展开更多
目的建立基于Turboflow在线净化结合超高效液相色谱-静电场轨道阱高分辨质谱法(ultra performance liquid chromatography-electrostatic field orbital high resolution mass spectrometry,UPLC-Q Exactive MS)测定水产品中4种地西泮...目的建立基于Turboflow在线净化结合超高效液相色谱-静电场轨道阱高分辨质谱法(ultra performance liquid chromatography-electrostatic field orbital high resolution mass spectrometry,UPLC-Q Exactive MS)测定水产品中4种地西泮及代谢物和6种丁香酚类化合物的方法。方法采用Turboflow在线净化,Accucore^(TM) aQ C_(18)柱(100 mm×2.1 mm,2.6μm)分离,以水-乙腈为流动相梯度洗脱,全扫描+自动触发二级质谱的正离子扫描监测模式,外标法定量。结果地西泮及代谢物和丁香酚类化合物在1.0~100.0μg/L范围内线性良好,化合物的相关系数(r^(2))均大于0.995;在水产品中的定量限分别为0.5μg/kg、2.0μg/kg;加标回收率为75.3%~110.0%,相对标准偏差小于10%。结论该方法操作简便、灵敏度高、检出限低,适用于水产品中地西泮及丁香酚类化合物的测定。通过调查发现,运输环节中水产品中检出地西泮和丁香酚类化合物,亟需对水产品中镇静剂或麻醉剂残留情况开展风险监测,加强监管以保障水产品质量安全。展开更多
The aim of this paper is to understand the common characteristics of the generalized flyby trajectory around natural elongated bodies. Such flyby trajectories provide a short-term mechanism to clear away vicinal objec...The aim of this paper is to understand the common characteristics of the generalized flyby trajectory around natural elongated bodies. Such flyby trajectories provide a short-term mechanism to clear away vicinal objects or temporally capture ejecta into circling orbits. The gravitational potential of elongated bodies is described by a unified approximate model, i.e., the rotating mass dipole which is two point masses connected with a constant massless rod The energy power is used to illustrate the flyby effect in terms of the instantaneous orbital energy. The essential of the single flyby trajectory is studied analytically, and the relationship between the flyby trajectory and its Jacobi integral is also illustrated. Sample trajectories are given to show the variational trend of the energy increment with respect to differen orbital periapsides. The distribution of natural ejecting orbits is presented by varying the parameters of the approximate model.展开更多
Stars in the Pulkovo Observatory program are observed with a 65-cm refractor during many years to study their positions and movements. We present examples of two visual binary stars, for which orbits and masses of com...Stars in the Pulkovo Observatory program are observed with a 65-cm refractor during many years to study their positions and movements. We present examples of two visual binary stars, for which orbits and masses of components were determined, and two astrometric stars, for which masses of their unseen companions were estimated. The first two stars are ADS 14636 (61 Cygni) and ADS 7251, and the others are Gliese 623 and ADS 8035 (Alpha UMa). Direct astrometric methods are used for estimation of mass-ratio and masses.展开更多
1 Introduction The end-Triassic mass extinction event is one of the five global mass extinctions,and destroyed both the marine and terrestrial biological worlds.Though years the marine endTriassic mass extinction(ETE)...1 Introduction The end-Triassic mass extinction event is one of the five global mass extinctions,and destroyed both the marine and terrestrial biological worlds.Though years the marine endTriassic mass extinction(ETE)event has been widely studied and discussed,and the standard marine Triassic/Jurassic boundary(TJB)(base-Jurassic)has also been determined.However.展开更多
基金Supported by National Natural Science Foundation of China(No.82000862,No.82201214)Shaanxi Key Research and Development Program(No.2021SF-156).
文摘AIM:To explore the clinical and pathological characteristics of thirteen patients with orbital liposarcoma.METHODS:The clinical history data of thirteen patients diagnosed as orbital liposarcoma at Beijing Tongren Hospital,from 2006 to 2021 were collected and analyzed.The data includes age,gender,affected orbital side,course of disease,status of disease(primary or recurrent),clinical manifestations,preoperative visual acuity,operative treatment,the relations between liposarcoma and surrounding tissue,longest diameter of liposarcoma,histological subtype,immunohistochemical indicators,follow-up treatment and prognosis.RESULTS:The initial symptoms are diverse.Proptosis is the most frequent chief complaint and the others included vision loss,epiphora,diplopia,and eyelid palpable mass.Results of imaging examination[computed tomography(CT)or magnetic resonance imaging(MRI)]showed orbital mass.In terms of treatment,10 patients received tumor resection,and the mean longest diameter of the tumor was 3.39±1.36 cm.The other 3 patients had optic nerve invaded,so they received orbital exenteration.Pathological examination results confirmed the diagnose of liposarcoma for 13 patients.Six patients displayed as myxoid type,and three patients in each type of dedifferentiated and welldifferentiated type.One patient was verified as pleomorphic,which was a rare type of liposarcoma.All of the patients showed Vimentin positive,and most showed CD34 and S-100 positive.Besides,four patients showed smooth muscle actin positive.All thirteen patients were alive.CONCLUSION:Orbital liposarcoma is a rare disease and it has no specific clinical manifestation.The diagnosis of liposarcoma should be considered when proptosis and orbital mass occurred in orbit.It is recommended to perform pathological examination to achieve early detection and early treatment.
文摘Recent measurements have shown that gravitational waves and thus the gravitational interaction propagate with the speed of light. The propagation delay of the gravitational interaction in orbiting systems couples the orbital and center of mass motions. This causes the orbits to spiral out and the center of mass to accelerate. It is one of a number of small effects modifying the Kepler orbits. The calculations show that the analytical describable expansion of the semimajor axis started at a time that is less than the age of the systems. This could be caused by a collision of a system component in the past. The effect of this propagation delay on the motion of the Earth Moon and the Brown Dwarf 569Bab binary star system is analyzed. These systems were chosen because a considerable amount of measured astronomical data is available. The calculated results are in excellent agreement with the measured data. In galaxies, too, the energy transfer from the orbit of the star cloud to the center of mass motion causes the galaxies to ac-celerate. If galaxies are considered to be molecules of the universe, then the acceleration of the galaxies will cause the molecular gas to heat and expand. Alternatively, the loss in orbital internal energy of the galaxies should be included in the mass and energy in the calculation of the expanding Universe.
基金Project supported by the National Natural Science Foundation of China (No. 11002076)the National Defence Preresearch Foundation of China (No. 51320010201)
文摘Spacecrafts with the pure gravity environment are of great significance in precision navigation, gravity field measurement for celestial bodies, and basic physics ex- periments. The radiometer effect is one of the important interfering factors on the proof mass in a purely gravitational orbit. For the gravity field measurement system based on the inner-formation flying, the relationship between the radiometer effect on the inner- satellite and the system parameters is studied by analytical and numerical methods. An approximate function of the radiometer effect suitable for the engineering computation and the correction factor are obtained. The analytic results show that the radiometer effect on the inner-satellite is proportional to the average pressure while inversely pro- portional to the average temperature in the outer-satellite cavity. The radiometer effect increases with the temperature difference in the cavity, and its minimum exists when the cavity radius increases. When the minimum of the radiometer effect arrives, the ratio of the cavity radius to the inner-satellite radius is 1.189 4. This constant is determined by the spherical cavity configuration and independent of the temperature and pressure distributions. When the ratio of the cavity radius to the inner-satellite radius is more than 10, it is believed that the cavity is large enough, the radiometer effect is approxi- mately proportional to the square of the inner-satellite radius, and the influence of the outer-satellite cavity radius on the radiometer effect can be ignored.
基金Supported by National Natural Science Foundation of China(No.81300805)。
文摘AIM:To characterize spectral-domain optical coherence tomography(SD-OCT)features of chorioretinal folds in orbital mass imaged using enhanced depth imaging(EDI).METHODS:Prospective observational case-control study was conducted in 20 eyes of 20 patients,the uninvolved eye served as a control.All the patients underwent clinical fundus photography,computed tomography,EDI SDOCT imaging before and after surgery.Two patients with cavernous hemangiomas underwent intratumoral injection of bleomycin A5;the remaining patients underwent tumor excision.Patients were followed 1 to 14mo following surgery(average follow up,5.8mo).RESULTS:Visual acuity prior to surgery ranged from 20/20 to 20/200.Following surgery,5 patients’visual acuity remained unchanged while the remaining 15 patients had a mean letter improvement of 10(range 4 to 26 letters).Photoreceptor inner/outer segment defects were found in 10 of 15 patients prior to surgery.Following surgical excision,photoreceptor inner/outer segment defects fully resolved in 8 of these 10 patients.CONCLUSION:Persistence of photoreceptor inner/outer segment defects caused by compression of the globe by an orbital mass can be associated with reduced visual prognosis.Our findings suggest that photoreceptor inner/outer segment defects on EDI SD-OCT could be an indicator for immediate surgical excision of an orbital mass causing choroidal compression.
文摘目的建立基于Turboflow在线净化结合超高效液相色谱-静电场轨道阱高分辨质谱法(ultra performance liquid chromatography-electrostatic field orbital high resolution mass spectrometry,UPLC-Q Exactive MS)测定水产品中4种地西泮及代谢物和6种丁香酚类化合物的方法。方法采用Turboflow在线净化,Accucore^(TM) aQ C_(18)柱(100 mm×2.1 mm,2.6μm)分离,以水-乙腈为流动相梯度洗脱,全扫描+自动触发二级质谱的正离子扫描监测模式,外标法定量。结果地西泮及代谢物和丁香酚类化合物在1.0~100.0μg/L范围内线性良好,化合物的相关系数(r^(2))均大于0.995;在水产品中的定量限分别为0.5μg/kg、2.0μg/kg;加标回收率为75.3%~110.0%,相对标准偏差小于10%。结论该方法操作简便、灵敏度高、检出限低,适用于水产品中地西泮及丁香酚类化合物的测定。通过调查发现,运输环节中水产品中检出地西泮和丁香酚类化合物,亟需对水产品中镇静剂或麻醉剂残留情况开展风险监测,加强监管以保障水产品质量安全。
基金supported by the National Basic Research Program of China(973 Program),(Grant 2012CB720000)China Postdoctoral Science Foundation(Grant 2014M560076)Support from Shanghai Satellite Engineering Research Institute(Grant 13dz2260100)is also acknowledged
文摘The aim of this paper is to understand the common characteristics of the generalized flyby trajectory around natural elongated bodies. Such flyby trajectories provide a short-term mechanism to clear away vicinal objects or temporally capture ejecta into circling orbits. The gravitational potential of elongated bodies is described by a unified approximate model, i.e., the rotating mass dipole which is two point masses connected with a constant massless rod The energy power is used to illustrate the flyby effect in terms of the instantaneous orbital energy. The essential of the single flyby trajectory is studied analytically, and the relationship between the flyby trajectory and its Jacobi integral is also illustrated. Sample trajectories are given to show the variational trend of the energy increment with respect to differen orbital periapsides. The distribution of natural ejecting orbits is presented by varying the parameters of the approximate model.
文摘Stars in the Pulkovo Observatory program are observed with a 65-cm refractor during many years to study their positions and movements. We present examples of two visual binary stars, for which orbits and masses of components were determined, and two astrometric stars, for which masses of their unseen companions were estimated. The first two stars are ADS 14636 (61 Cygni) and ADS 7251, and the others are Gliese 623 and ADS 8035 (Alpha UMa). Direct astrometric methods are used for estimation of mass-ratio and masses.
基金financially supported by the National Natural Science Foundation of China(Grant No.41730317)Special Basic Program of Ministry of Science and Technology of China(Grant No.2015FY310100)+1 种基金Bureau of Geological Survey of China and National Committee ofStratigraphy of China(Grant No.DD20160120-04)UNESCO-IUGS IGCP project 632.
文摘1 Introduction The end-Triassic mass extinction event is one of the five global mass extinctions,and destroyed both the marine and terrestrial biological worlds.Though years the marine endTriassic mass extinction(ETE)event has been widely studied and discussed,and the standard marine Triassic/Jurassic boundary(TJB)(base-Jurassic)has also been determined.However.