標(biāo)題: Titlebook: Cosmic Gamma Rays, Neutrinos, and Related Astrophysics; Maurice M. Shapiro,John P. Wefel Book 1989 Kluwer Academic Publishers 1989 Superno [打印本頁(yè)] 作者: Fixate 時(shí)間: 2025-3-21 17:47
書(shū)目名稱(chēng)Cosmic Gamma Rays, Neutrinos, and Related Astrophysics影響因子(影響力)
書(shū)目名稱(chēng)Cosmic Gamma Rays, Neutrinos, and Related Astrophysics影響因子(影響力)學(xué)科排名
書(shū)目名稱(chēng)Cosmic Gamma Rays, Neutrinos, and Related Astrophysics網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱(chēng)Cosmic Gamma Rays, Neutrinos, and Related Astrophysics網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱(chēng)Cosmic Gamma Rays, Neutrinos, and Related Astrophysics被引頻次
書(shū)目名稱(chēng)Cosmic Gamma Rays, Neutrinos, and Related Astrophysics被引頻次學(xué)科排名
書(shū)目名稱(chēng)Cosmic Gamma Rays, Neutrinos, and Related Astrophysics年度引用
書(shū)目名稱(chēng)Cosmic Gamma Rays, Neutrinos, and Related Astrophysics年度引用學(xué)科排名
書(shū)目名稱(chēng)Cosmic Gamma Rays, Neutrinos, and Related Astrophysics讀者反饋
書(shū)目名稱(chēng)Cosmic Gamma Rays, Neutrinos, and Related Astrophysics讀者反饋學(xué)科排名
作者: Serenity 時(shí)間: 2025-3-21 20:56 作者: 拔出 時(shí)間: 2025-3-22 03:01
Conservation and Efficiency Issues,eriodicity of known binary systems. We describe the production of such γ-rays and the accompaning . production at binary sources, discuss the required proton luminosity and the modulation of the signals. We also outline the possible impacts of energetic proton, γ-ray and . beams on the stability and the dynamics of the source system.作者: GROWL 時(shí)間: 2025-3-22 06:14 作者: 贊美者 時(shí)間: 2025-3-22 11:53 作者: Immortal 時(shí)間: 2025-3-22 15:11 作者: Immortal 時(shí)間: 2025-3-22 18:42 作者: aspect 時(shí)間: 2025-3-22 23:17
Disinfection By-products in Recycled Waters,s discussed. Recent results from the CYGNUS experiment with regard to steady emission from sources such as Cygnus X-3 and Herculus X-l are compared with those from other experiments. Criteria for next generation of detectors are developed and discussed.作者: 使成整體 時(shí)間: 2025-3-23 03:35 作者: 乏味 時(shí)間: 2025-3-23 06:19
Production of Energetic Gamma-Rays and Neutrinos at Binary Systemseriodicity of known binary systems. We describe the production of such γ-rays and the accompaning . production at binary sources, discuss the required proton luminosity and the modulation of the signals. We also outline the possible impacts of energetic proton, γ-ray and . beams on the stability and the dynamics of the source system.作者: Paradox 時(shí)間: 2025-3-23 11:58 作者: Free-Radical 時(shí)間: 2025-3-23 17:52
Gamma-Ray Astronomy and the Holistic Galaxyistribution of galactic gas and cosmic rays. This picture is intrinsically tied to the overall processes of stellar birth and destruction on a galactic scale. Since it requires the balanced and coordinated use of multiwavelength studies to complete this scenario of the galaxy, it seems appropriate to refer to it as a holistic one.作者: 縱欲 時(shí)間: 2025-3-23 19:48 作者: forbid 時(shí)間: 2025-3-24 00:37 作者: LEVER 時(shí)間: 2025-3-24 03:08
Ultra High Energy Astronomys discussed. Recent results from the CYGNUS experiment with regard to steady emission from sources such as Cygnus X-3 and Herculus X-l are compared with those from other experiments. Criteria for next generation of detectors are developed and discussed.作者: 賞錢(qián) 時(shí)間: 2025-3-24 09:33
Constraints on the Production Mechanism of TeV γ-Rays in X-Ray Binaries of the absorption regions, the accretion disk corona, causes very strong attenuation of TeV γ-rays produced near to its centre, and suggests that a more likely method for their creation would be the dumping of a proton beam into some outlying matter, such as the rim of the accretion disk.作者: 能夠支付 時(shí)間: 2025-3-24 12:23
https://doi.org/10.1007/978-94-009-0921-2Supernova; active galactic nuclei; astronomy; astrophysics; black hole; cosmic ray; galaxies; gamma-ray bur作者: Muffle 時(shí)間: 2025-3-24 16:46 作者: 下垂 時(shí)間: 2025-3-24 20:51 作者: 服從 時(shí)間: 2025-3-25 02:41
Conservation and Efficiency Issues,eriodicity of known binary systems. We describe the production of such γ-rays and the accompaning . production at binary sources, discuss the required proton luminosity and the modulation of the signals. We also outline the possible impacts of energetic proton, γ-ray and . beams on the stability and作者: 附錄 時(shí)間: 2025-3-25 06:00 作者: Ondines-curse 時(shí)間: 2025-3-25 10:38 作者: 自愛(ài) 時(shí)間: 2025-3-25 13:13 作者: 縮短 時(shí)間: 2025-3-25 17:49
Conservation and Efficiency Issues, observations were important, pride of place must be given to the detection of neutrinos from the SN (the SN being denoted SN 1987A; its location was the Large Magellanic Cloud)..The neutrino detection was important from a number of standpoints, not least for the confirmation given to the general co作者: Cpr951 時(shí)間: 2025-3-25 20:23 作者: Mercurial 時(shí)間: 2025-3-26 03:04
Conservation and Efficiency Issues,ons involving the three flavour neutrinos is considered without simplifying assumptions. The T-violating asymmetry in three-neutrino oscillations in matter with constant density is discussed and it is shown that this asymmetry can be much larger than the corresponding asymmetry in vacuum oscillation作者: EVICT 時(shí)間: 2025-3-26 06:23 作者: 中世紀(jì) 時(shí)間: 2025-3-26 11:50 作者: 專(zhuān)心 時(shí)間: 2025-3-26 16:29
Student Elicitation for Estimation, pointing accuracy of better than 1.5° to look at point sources. From April 1986-87 muon detectors of total area 200 m. have also been in operation. We present upper limits on the flux of gamma rays from CYGNUS-X3 and demonstrate the usefulness of our muon detectors in improving the signal to noise 作者: 魯莽 時(shí)間: 2025-3-26 18:18
Petter Gottschalk,Lars Gunnesdal of the absorption regions, the accretion disk corona, causes very strong attenuation of TeV γ-rays produced near to its centre, and suggests that a more likely method for their creation would be the dumping of a proton beam into some outlying matter, such as the rim of the accretion disk.作者: reserve 時(shí)間: 2025-3-26 23:24
Conservation and Efficiency Issues,Gamma-ray Astronomy investigates the electromagnetic radiation coming from Outer Space in the energy range above~100 KeV, bordering and mixing on the low energy side with the upper end of X-Ray Astronomy; no limit is indicated on the high energy side if not that imposed by the vanishing intensity of the incoming flux (Fig.1).作者: 確保 時(shí)間: 2025-3-27 03:29
Toshihiro Fujito,Kei Kimura,Yuki MizunoIt is shown that experimentally measured ratio of atmospheric electron-neutrino flux to that of muon-neutrinos and expected theoretical ratio do not contradict each other if muon polarization is taken into account in calculations.作者: Receive 時(shí)間: 2025-3-27 07:33
Conservation and Efficiency Issues,We discuss the question whether a laboratory placed on the Moon has some advantages for astrophysical neutrino studies compared to such a laboratory on the Earth.作者: Gingivitis 時(shí)間: 2025-3-27 09:56
Junhee Cho,Sewon Park,Martin ZieglerA short historical outline of VHE and UHE gamma-ray astronomy is given, including personal reminiscences of the author. Special attention is paid to the development of experimental techniques and methods of analysis. The main results obtained in the field to date are critically reviewed.作者: 季雨 時(shí)間: 2025-3-27 14:49
Ligy Philip,C. Ramprasad,D. KrithikaWe compare the observations of Cygnus X-3 performed in 1986 by different arrays in the 100 TeV energy range. Three experiments (Baksan, Plateau Rosà, Grex in Leeds) show similar excesses at 2 ÷ 3σ. A search for pulsar periodicity in the Baksan Hercules X-l data is presented ; no positive evidence is found.作者: 中國(guó)紀(jì)念碑 時(shí)間: 2025-3-27 20:04 作者: DAMP 時(shí)間: 2025-3-27 22:42
Other Macroeconomic Estimations,The Crab pulsar (PSR0531+21) has been observed with the Whipple Observatory 10 m Reflector in imaging mode for ~102h. A suggestion of a broad light curve has been found, but with a low statistical significance. An upper limit (95% confidence level) for the pulsed flux (energy > 0.7TeV) is 4.5x10. photons-cm.-s..作者: Hormones 時(shí)間: 2025-3-28 06:10 作者: 健壯 時(shí)間: 2025-3-28 06:30
A Comment on ,,/,, Ratio in Atmospheric Neutrino FluxesIt is shown that experimentally measured ratio of atmospheric electron-neutrino flux to that of muon-neutrinos and expected theoretical ratio do not contradict each other if muon polarization is taken into account in calculations.作者: Diluge 時(shí)間: 2025-3-28 10:43
Fluxes of Muons and Neutrinos Generated by Primary Radiation on the MoonWe discuss the question whether a laboratory placed on the Moon has some advantages for astrophysical neutrino studies compared to such a laboratory on the Earth.作者: hysterectomy 時(shí)間: 2025-3-28 15:39
VHE and UHE Gamma Ray Astronomy: History and ProblemsA short historical outline of VHE and UHE gamma-ray astronomy is given, including personal reminiscences of the author. Special attention is paid to the development of experimental techniques and methods of analysis. The main results obtained in the field to date are critically reviewed.作者: 語(yǔ)源學(xué) 時(shí)間: 2025-3-28 21:53 作者: 復(fù)習(xí) 時(shí)間: 2025-3-29 02:43
Observation of TeV Gamma-rays from the Crab NebulaThe Whipple Observatory 10 m Reflector operating as a 37-pixel camera has been used to observe the Crab Nebula in TeV gamma rays. Using gamma-ray image selection a detection is reported at the 9.0 sigma level; this corresponds to a flux of 1.8 x 10. photons-cm.-s. above 0.7 TeV.作者: Thrombolysis 時(shí)間: 2025-3-29 06:09 作者: acrimony 時(shí)間: 2025-3-29 10:44
Nato Science Series C:http://image.papertrans.cn/c/image/238878.jpg作者: 慷慨不好 時(shí)間: 2025-3-29 12:13
Cosmic Gamma Rays, Neutrinos, and Related Astrophysics作者: 勛章 時(shí)間: 2025-3-29 19:34
Ultra High Energy Radiation from Hercules X-l; New Physics Above 100 TEV ?7±0.0003sec with a statistical significance of ~ 2 ×10.. The showers were found to have a muon content similar to that for hadronic showers and the energy of their progenitors were greater than 400 TeV. The characteristic muon poor feature of similar gamma ray initiated showers was not observed for the signal.作者: 不容置疑 時(shí)間: 2025-3-29 22:14
UHE Gamma Ray Observations with the KGF Air Shower Arraye present upper limits on the flux of gamma rays from CYGNUS-X3 and demonstrate the usefulness of our muon detectors in improving the signal to noise ratio for gamma ray showers, if conventional interaction models are valid.作者: –DOX 時(shí)間: 2025-3-30 03:34
Conservation and Efficiency Issues,, Pérez-Fournon et al. 1988) leads a) to a prediction of high energy neutrino-emission in addition to photon emission, to physical arguments about b) shock structure and sharpness of cutoff and c) the radial dependence of the cutoff frequency in the M87 jet, and d) to a possible explanation of X-ray emission as secondary synchrotron radiation.作者: 撫慰 時(shí)間: 2025-3-30 07:32
Conservation and Efficiency Issues,hus provide an important new diagnostic of black holes not obtainable with x-ray observations. This has important implications for both the theory and strategies of future high energy observation of black holes.作者: 柔聲地說(shuō) 時(shí)間: 2025-3-30 11:05 作者: 恃強(qiáng)凌弱 時(shí)間: 2025-3-30 14:46 作者: 短程旅游 時(shí)間: 2025-3-30 18:23
Conservation and Efficiency Issues,ino signal was smaller than that for which some of the ‘neutrino detectors’ were designed. Consequently, problems have arisen and they will be described. Despite the problems it is concluded that neutrinos were detected with just about the characteristics predicted by contemporary theories.作者: 引導(dǎo) 時(shí)間: 2025-3-31 00:06 作者: Heart-Rate 時(shí)間: 2025-3-31 03:46
Water Scarcity and Ways to Reduce the Impact7±0.0003sec with a statistical significance of ~ 2 ×10.. The showers were found to have a muon content similar to that for hadronic showers and the energy of their progenitors were greater than 400 TeV. The characteristic muon poor feature of similar gamma ray initiated showers was not observed for the signal.作者: Phenothiazines 時(shí)間: 2025-3-31 06:44 作者: 侵略者 時(shí)間: 2025-3-31 11:59
Photon and Neutrino-Emission from Shockwaves in Active Galactic Nucleier to explain the observed ubiquitous sharp cutoff in the nonthermal synchrotron emission observed in hot spots, jets and compact cores. Application of the theory, developed in a series of papers (Webb et al. 1984, Pérez-Fournon 1985, Biermann and Strittmatter 1987, Klemens 1987a,b, Fritz 1987, 1988作者: scotoma 時(shí)間: 2025-3-31 14:02
Production of Energetic Gamma-Rays and Neutrinos at Binary Systemseriodicity of known binary systems. We describe the production of such γ-rays and the accompaning . production at binary sources, discuss the required proton luminosity and the modulation of the signals. We also outline the possible impacts of energetic proton, γ-ray and . beams on the stability and作者: 螢火蟲(chóng) 時(shí)間: 2025-3-31 19:09
Cosmic Gamma-Rays and Cosmic-Ray Neutrinos from Galactic and Solar Dark Matter Annihilation heavy neutral fermions (sometimes called WIMPS for Weakly Interacting Massive Particles), assuming that such particles make up the dark matter in the galactic halo. For neutrinos, both galactic and solar production spectra are given.作者: 數(shù)量 時(shí)間: 2025-4-1 00:17 作者: BUCK 時(shí)間: 2025-4-1 02:00 作者: ABYSS 時(shí)間: 2025-4-1 07:38
The Neutrino Signal from SN 1987A observations were important, pride of place must be given to the detection of neutrinos from the SN (the SN being denoted SN 1987A; its location was the Large Magellanic Cloud)..The neutrino detection was important from a number of standpoints, not least for the confirmation given to the general co作者: Choreography 時(shí)間: 2025-4-1 12:04
On the Spectrum of Neutrinos from SN 1987Ainos is assumed to be twice that of the .. neutrinos. Then the . oscillations on the way from LMC can provide a suitably mixed neutrino spectrum even for an extremely small oscillation parameter, Δm. > 10. eV..
