標(biāo)題: Titlebook: Cosmic Rays, Supernovae and the Interstellar Medium; Maurice M. Shapiro,Rein Silberberg,John P. Wefel Book 1991 Springer Science+Business [打印本頁] 作者: invigorating 時(shí)間: 2025-3-21 17:35
書目名稱Cosmic Rays, Supernovae and the Interstellar Medium影響因子(影響力)
書目名稱Cosmic Rays, Supernovae and the Interstellar Medium影響因子(影響力)學(xué)科排名
書目名稱Cosmic Rays, Supernovae and the Interstellar Medium網(wǎng)絡(luò)公開度
書目名稱Cosmic Rays, Supernovae and the Interstellar Medium網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Cosmic Rays, Supernovae and the Interstellar Medium被引頻次
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書目名稱Cosmic Rays, Supernovae and the Interstellar Medium讀者反饋
書目名稱Cosmic Rays, Supernovae and the Interstellar Medium讀者反饋學(xué)科排名
作者: 紀(jì)念 時(shí)間: 2025-3-21 22:36 作者: 鬼魂 時(shí)間: 2025-3-22 01:24
Historiography of African Market Womencceleration and the conditions in the interstellar medium through which the particles travel. Recent (1988–90) measurements and interpretations have provided new information on cosmic ray composition and source abundances. These new results are described and compared to previous work.作者: Awning 時(shí)間: 2025-3-22 06:22 作者: Cabg318 時(shí)間: 2025-3-22 11:50
Defending Attacks Against Transhumanism, effects that apply to the identification of SNRs, and the uncertainties in the distances of most SNRs. Although it is clear that the distribution of high surfacebrightness remnants is concentrated in a nuclear disk, it is not possible to derive the distribution for SNRs within the solar circle in any detail.作者: Scleroderma 時(shí)間: 2025-3-22 14:42 作者: Scleroderma 時(shí)間: 2025-3-22 20:40
Researching the Rural: A , Loose in AfricaThe formation of molecular hydrogen in dense clouds is evaluated by means of a Monte Carlo simulation of the bombardment of cosmic protons and helium ions (E< 1 GeV) on interstellar dust grains of the Greenberg type. A comparison with results obtained for the Mathis model is given.作者: crutch 時(shí)間: 2025-3-23 01:10 作者: debase 時(shí)間: 2025-3-23 05:24 作者: Lyme-disease 時(shí)間: 2025-3-23 05:57 作者: Mitigate 時(shí)間: 2025-3-23 13:37
Shock Acceleration of Cosmic RaysThe basic concepts of diffusive shock acceleration are reviewed and the mechanism, applied to the shocks bounding Galactic supernova remnants, is considered as a possible source for the Galactic cosmic rays.作者: 土產(chǎn) 時(shí)間: 2025-3-23 15:38 作者: 巡回 時(shí)間: 2025-3-23 18:44 作者: 莎草 時(shí)間: 2025-3-23 23:01 作者: Preserve 時(shí)間: 2025-3-24 03:29 作者: 豎琴 時(shí)間: 2025-3-24 10:16 作者: infinite 時(shí)間: 2025-3-24 12:36 作者: 反叛者 時(shí)間: 2025-3-24 16:18
Humans, Transhumans and Humanoids,f the solar atmosphere. Since the condensation temperature for each of these elements is usually higher than 800K, the mechanism for the cosmic ray source matter to be formed seems to be causally connected to the condensation process of those elements in the circumstellar gases or in the matter ejec作者: rectum 時(shí)間: 2025-3-24 19:19 作者: 愛社交 時(shí)間: 2025-3-25 00:57 作者: Eeg332 時(shí)間: 2025-3-25 04:45 作者: 不怕任性 時(shí)間: 2025-3-25 07:50
Water Bears: The Biology of Tardigradeson the evolution of the expanding envelope. Relativistic bremsstrahlung is the dominant energy loss mechanism until the material through which the beam propagates becomes ionized. After an ionized channel is formed, plasma processes and inverse Compton losses become the dominant loss mechanisms. The作者: Eructation 時(shí)間: 2025-3-25 11:50 作者: escalate 時(shí)間: 2025-3-25 17:15 作者: CURT 時(shí)間: 2025-3-25 23:25 作者: DUST 時(shí)間: 2025-3-26 00:54 作者: 赤字 時(shí)間: 2025-3-26 06:20
he calculation of the energy production spectra of the γ-rays and neutrinos produced in the accretion processes onto collapsed objects. Because of the complexity of the problem we start in describing the physical processes in the case of spherical symmetric accretion..The results of these calculatio作者: 你不公正 時(shí)間: 2025-3-26 08:29 作者: muster 時(shí)間: 2025-3-26 13:00
The Composition of the Cosmic Rays: An Updatecceleration and the conditions in the interstellar medium through which the particles travel. Recent (1988–90) measurements and interpretations have provided new information on cosmic ray composition and source abundances. These new results are described and compared to previous work.作者: foliage 時(shí)間: 2025-3-26 19:20
Cosmic-Ray Age and the Interstellar Mediumhe galactic gas proves to be very essential for the interpretation of the data on the content of secondary stable and radioactive isotopes in the cosmic rays. Constraints on a galactic wind and on cosmic-ray distributed acceleration in the interstellar medium are discussed.作者: Euphonious 時(shí)間: 2025-3-27 00:42 作者: 反復(fù)無常 時(shí)間: 2025-3-27 04:44 作者: conjunctiva 時(shí)間: 2025-3-27 07:00 作者: vascular 時(shí)間: 2025-3-27 10:59 作者: 無表情 時(shí)間: 2025-3-27 16:25 作者: 拱墻 時(shí)間: 2025-3-27 20:30
Humans, Transhumans and Humanoids,on is discussed which may achieve higher maximum energy and maintain for a short period of time high cosmic ray luminosities. Accelerated cosmic rays will interact on the material of the supernova shell and give rise to high energy neutrino and γ-ray signals.作者: indignant 時(shí)間: 2025-3-28 02:01
https://doi.org/10.1007/978-3-319-95702-9. Emission from the southern extension of the remnant generally has a steeper radio spectrum than the north, with α up to ≈ 0.55. These results are discussed in relation to available theories for the radio emission from supernova remnants, and to the radio structure of the remnant.作者: 領(lǐng)帶 時(shí)間: 2025-3-28 05:27
Ralph O. Schill,Steffen Hengherr-3, Her X-1, Vela X-1 and Cen X-3 and of the radio pulsar sources PSR 0531 +21 and PSR 0833-45, the Crab and the Vela pulsars, are described in more detail. Possible VHE and UHE gamma ray source catalogs are examined. The current state and future requirements of VHE and UHE gamma ray astronomy are briefly discussed.作者: 道學(xué)氣 時(shí)間: 2025-3-28 08:13 作者: Peristalsis 時(shí)間: 2025-3-28 13:11 作者: GUILT 時(shí)間: 2025-3-28 17:40
The Production of Antiprotons in the Interstellar Gas by Propagating Cosmic Raysdromegnetic waves. It could be shown that the calculated . ratio is enhanced in the diffusive reacceleration model compared to that derived from the Leaky Box Model, but it remains difficult to bring it into agreement with the data.作者: 發(fā)出眩目光芒 時(shí)間: 2025-3-28 19:49 作者: Indelible 時(shí)間: 2025-3-29 01:44 作者: saphenous-vein 時(shí)間: 2025-3-29 03:52 作者: 消耗 時(shí)間: 2025-3-29 09:36 作者: 饒舌的人 時(shí)間: 2025-3-29 13:39
Acceleration of Cosmic Rays At Young Supernova Remnantson is discussed which may achieve higher maximum energy and maintain for a short period of time high cosmic ray luminosities. Accelerated cosmic rays will interact on the material of the supernova shell and give rise to high energy neutrino and γ-ray signals.作者: 凝視 時(shí)間: 2025-3-29 18:41 作者: 商品 時(shí)間: 2025-3-29 20:01 作者: 黃瓜 時(shí)間: 2025-3-30 01:13 作者: 嚴(yán)峻考驗(yàn) 時(shí)間: 2025-3-30 07:50
Historiography of African Market Womenly the isotopic ones; lifetime of the GCR; acceleration of the particles and their injection into the ISM. Finally the significance of cosmic neutrinos, cosmic gamma rays, and antiprotons is briefly treated.作者: Constrain 時(shí)間: 2025-3-30 09:25 作者: Stable-Angina 時(shí)間: 2025-3-30 16:05
ns will be used to evaluate the upper limit to the number of the black holes in the Galaxy and to fit the γ-ray COS B experimental data of the quasar 3C 273 and to predict the neutrino fluxes from the directions of 3C 273 and the Galactic Center.作者: 雕鏤 時(shí)間: 2025-3-30 17:58 作者: 支柱 時(shí)間: 2025-3-30 21:23
A Brief Introduction to the Cosmic Radiationhing the earth and the “primordial” or source composition; the energy spectra and their modulation in the heliosphere; the effects of magnetic fields, notably on the directional distribution; the propagation of the GCR in the interstellar medium (ISM), and what is inferred about abundances, especial作者: 斑駁 時(shí)間: 2025-3-31 04:41
The Composition of the Cosmic Rays: An Updatecceleration and the conditions in the interstellar medium through which the particles travel. Recent (1988–90) measurements and interpretations have provided new information on cosmic ray composition and source abundances. These new results are described and compared to previous work.作者: FLAX 時(shí)間: 2025-3-31 06:57 作者: 口訣法 時(shí)間: 2025-3-31 10:25
Source Composition, Sites of Origin and Acceleration of Cosmic Raysulations make corrections for the nuclear spallation reactions suffered by the cosmic-ray nuclei in the interstellar gas and clouds. To learn about the sites of origin, the source composition is compared with the general Galactic abundance of elements and isotopes, which is based on spectroscopic st作者: 挑剔為人 時(shí)間: 2025-3-31 17:05
Cosmic-Ray Age and the Interstellar Mediumhe galactic gas proves to be very essential for the interpretation of the data on the content of secondary stable and radioactive isotopes in the cosmic rays. Constraints on a galactic wind and on cosmic-ray distributed acceleration in the interstellar medium are discussed.作者: lactic 時(shí)間: 2025-3-31 20:57
The Production of Antiprotons in the Interstellar Gas by Propagating Cosmic Raysof cosmic ray origin and propagation. We have present a detailed discussion of the equilibrium antiprotonproton ratio predictions calculated in the Standard Leaky Box Model and in the diffusive reacceleration model, where cosmic ray particles are reaccelerated due to gyroresonant interaction with hy
