標(biāo)題: Titlebook: Non-Solar X- and Gamma-Ray Astronomy; L. Gratton Book 1970 International Astronomical Union 1970 astronomy.instruments.neutron star.observ [打印本頁] 作者: 異國 時(shí)間: 2025-3-21 16:16
書目名稱Non-Solar X- and Gamma-Ray Astronomy影響因子(影響力)
書目名稱Non-Solar X- and Gamma-Ray Astronomy影響因子(影響力)學(xué)科排名
書目名稱Non-Solar X- and Gamma-Ray Astronomy網(wǎng)絡(luò)公開度
書目名稱Non-Solar X- and Gamma-Ray Astronomy網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Non-Solar X- and Gamma-Ray Astronomy被引頻次
書目名稱Non-Solar X- and Gamma-Ray Astronomy被引頻次學(xué)科排名
書目名稱Non-Solar X- and Gamma-Ray Astronomy年度引用
書目名稱Non-Solar X- and Gamma-Ray Astronomy年度引用學(xué)科排名
書目名稱Non-Solar X- and Gamma-Ray Astronomy讀者反饋
書目名稱Non-Solar X- and Gamma-Ray Astronomy讀者反饋學(xué)科排名
作者: 使激動(dòng) 時(shí)間: 2025-3-21 22:22
U. R. Rao,E. V. Chitnis,A. S. Prakasarao,U. B. Jayanthi作者: 悲痛 時(shí)間: 2025-3-22 02:38 作者: assent 時(shí)間: 2025-3-22 07:29
P. C. Agrawal,S. Biswas,G. S. Gokhale,V. S. Iyengar,P. K. Kunte,R. K. Manchanda,B. V. Sreekantan作者: groggy 時(shí)間: 2025-3-22 09:00
S. Hayakawa,T. Kato,F. Makino,H. Ogawa,Y. Tanaka,K. Yamashita,M. Matsuoka,S. Miyamoto,M. Oda,Y. Ogaw作者: Lumbar-Spine 時(shí)間: 2025-3-22 13:29
M. Matsuoka,S. Miyamoto,J. Nishimura,M. Oda,Y. Ogawara,M. Wada作者: collateral 時(shí)間: 2025-3-22 17:58 作者: REP 時(shí)間: 2025-3-22 21:22 作者: 熟練 時(shí)間: 2025-3-23 04:49
Sudden Changes in the Intensity of High Energy X-rays from Sco X-1, an angle of 32° with respect to the zenith. A pair of crossed flux gate magnetometers provided information every 8.2 sec on the azimuth of the telescope. The pulse heights from the X-ray detector were sorted into several channels extending from 10 to 120 keV. An Am. source came into the field of vi作者: FADE 時(shí)間: 2025-3-23 09:14
Intensities and Spectra of Several Galactic X-ray Sources,作者: 飛行員 時(shí)間: 2025-3-23 13:33
A Survey of Instruments and Experiments for X-ray Astronomy,arization of the X-ray sources, time variations are being studied and spectra are being measured to resolutions of the order of ~20%. The required instruments are being flown on sounding rockets, balloons and satellites. In addition, observation of the diffuse X-ray backgrounds requires even different instruments.作者: 煞費(fèi)苦心 時(shí)間: 2025-3-23 15:19 作者: 轉(zhuǎn)換 時(shí)間: 2025-3-23 18:53
,Energy Spectra of Several Discrete X-ray Sources in the 20–120 keV Range,68, and the balloon reached a ceiling of about 5.3 g cm. residual atmosphere and floated from 0230 to 0800 hrs. IST (Indian Standard Time). The second balloon was launched on December 22, 1968 and floated at about 7.5 g cm. of residual air from 1000 to 1130 hrs. IST.作者: 不真 時(shí)間: 2025-3-23 23:57 作者: Ondines-curse 時(shí)間: 2025-3-24 02:49 作者: MAOIS 時(shí)間: 2025-3-24 06:35
Interstellar Absorption of X-rays Emitted by Supernova Remnants,ay sources and the supernova remnants on the basis of there being a small a priori probability of having an accidental coincidence within 0.1 square degrees. Cas A is almost certainly the same source as Cas XR-1 which the NRL group saw in an earlier survey [1]. During the December flight the Crab nebula was also observed for a short time interval.作者: 吸引人的花招 時(shí)間: 2025-3-24 14:34
Introductory Remarks,r gas and the interstellar dust. For practical purposes, interstellar gas is completely transparent over galactic distances for all wavelengths from radio waves to the far ultraviolet. In this spectral region the visibility is partially impeded only by the unevenly distributed interstellar dust.作者: obscurity 時(shí)間: 2025-3-24 15:31
Upper-Air Fluorescence as a Tool in X-ray Astronomy and Searches for X-rays from NP 0532 and Other ith our respective installations. These are sited at Mount Hopkins (the SAO field station at 2300 m altitude near Amado, Arizona) and at Sparsholt Firs (approx. 300 m altitude, on the Berkshire Downs, near Harwell).作者: 無法解釋 時(shí)間: 2025-3-24 21:28 作者: defenses 時(shí)間: 2025-3-25 00:02 作者: 騎師 時(shí)間: 2025-3-25 04:54
A Survey of Instruments and Experiments for X-ray Astronomy,many competing techniques have been devised for any given type of observation and that there has been a progression to increasingly sophisticated instruments. But most of this diversity is real and simply reflects the very broad range of observations that can be performed and the different kinds of 作者: 狂熱文化 時(shí)間: 2025-3-25 09:43 作者: muscle-fibers 時(shí)間: 2025-3-25 14:40
Upper-Air Fluorescence as a Tool in X-ray Astronomy and Searches for X-rays from NP 0532 and Other background of the upper-air fluorescence technique as a viable ground-based tool for studies of cosmic X-rays. After a discussion of the characteristics, merits and limitations of the technique, we describe some preliminary experiments which have been carried out, both separately and also jointly, w作者: 一回合 時(shí)間: 2025-3-25 16:40 作者: 注入 時(shí)間: 2025-3-25 22:55
Properties of Individual X-Ray Sources,te. These data have been obtained using actively collimated scintillation counters with apertures between 6 and 24o FWHM, areas between 10 and 50 cm. and which operate over the 10–300 keV range. The Crab Nebula has been observed on three occasions over a 22-month period between September 1965 and Ju作者: Laconic 時(shí)間: 2025-3-26 03:48 作者: 運(yùn)動(dòng)性 時(shí)間: 2025-3-26 07:25
X-ray Flux from Discrete Sources,, on November 3, 1968, and November 7, 1968, respectively, are presented. The results indicate the first evidence for the existence of low energy X-ray flux in the energy range 2–20 keV from Cen-X2 source since the reported extinction in May, 1967. The energy spectrum and the absolute flux of X-rays作者: 噴出 時(shí)間: 2025-3-26 08:54 作者: 鬧劇 時(shí)間: 2025-3-26 12:53
Sudden Changes in the Intensity of High Energy X-rays from Sco X-1,erval 29.9–52.3 keV on December 22, 1968 between 04 h 27 m and 05 h 53 m UT. The observation was made with an X-ray telescope flown in a balloon from Hyderabad, India. The balloon was launched at 0200 hr UT and reached the ceiling of 7.5 g/cm. of residual atmosphere at 0435 hr UT. The X-ray telescop作者: forbid 時(shí)間: 2025-3-26 19:49 作者: Obstacle 時(shí)間: 2025-3-26 22:32
The Flux of Hard Radiation from M87,f hard radiation from the general direction of Virgo; the experiment discussed here, conducted 16 months later, recorded approximately the same flux from a smaller region of sky that tends to isolate M87 as the most likely candidate for the source.作者: 受辱 時(shí)間: 2025-3-27 03:19
A Rocket Observation of Cosmic X-rays in the Energy Range between 0.15 and 20 keV,g rocket scanned a celestial region in which the galactic latitude .. changed from 30° to ?55° across the galactic plane in the Cygnus-Cassiopeia region. The spectrum of Cyg XR-2 thus obtained is represented by a thermal bremsstrahlung of temperature 3.4 keV modified by the interstellar absorption f作者: 偶像 時(shí)間: 2025-3-27 09:17 作者: 審問,審訊 時(shí)間: 2025-3-27 10:22 作者: jeopardize 時(shí)間: 2025-3-27 16:31
978-94-010-3313-8International Astronomical Union 1970作者: 過于平凡 時(shí)間: 2025-3-27 21:51
Non-Solar X- and Gamma-Ray Astronomy978-94-010-3311-4Series ISSN 1743-9213 Series E-ISSN 2352-2186 作者: 不斷的變動(dòng) 時(shí)間: 2025-3-28 00:00 作者: obscurity 時(shí)間: 2025-3-28 04:43
Techniques for Improving the Sensitivity of Proportional Counters Used in X-ray Astronomy,n the energy range from 1 to 50 keV, proportional counters have advantages over other types of detectors; they provide energy resolution and they can be made relatively easily with very large window areas.作者: craving 時(shí)間: 2025-3-28 10:08 作者: GENUS 時(shí)間: 2025-3-28 10:49 作者: GROWL 時(shí)間: 2025-3-28 16:32 作者: pancreas 時(shí)間: 2025-3-28 22:20
International Astronomical Union Symposiahttp://image.papertrans.cn/n/image/667027.jpg作者: Munificent 時(shí)間: 2025-3-28 23:36
https://doi.org/10.1007/978-94-010-3311-4astronomy; instruments; neutron star; observatory; solar wind作者: 立即 時(shí)間: 2025-3-29 06:21 作者: 討好女人 時(shí)間: 2025-3-29 08:40 作者: 不成比例 時(shí)間: 2025-3-29 13:17 作者: 書法 時(shí)間: 2025-3-29 18:54 作者: Aggressive 時(shí)間: 2025-3-29 23:22
Julie Rodgerseader. It is not normal to see such controversial concepts as "Renaissance," "Renaissance Thought," "Spanish Renaissance," or even "Spanish Thought" freely linked together in the crowded intimacy of one single printed line. The author of these essays is painfully aware of the com- plexity of the gro作者: heterogeneous 時(shí)間: 2025-3-30 01:12
Potential Exposure to Arsenic and Other Elements from Rice in Bangladesh: Health Risk Index,Chandpur) of Bangladesh. Rice samples were collected from 99 households and analyzed for this purpose. The mean concentrations of As, Cd, Co, Cr, Cu, Mn, Ni, Pb, and Zn in rice?were 187 μg/kg, 40 μg/kg, 16 μg/kg, 819 μg/kg, 1.8 mg/kg, 7.3 mg/kg, 549 μg/kg, 61 μg/kg, and 8.9 mg/kg, respectively. Food作者: degradation 時(shí)間: 2025-3-30 05:11
Generation and Analysis of Residential Microgrid Databasey Management Systems (EMS). To investigate such issues, a Microgrid Platform (MGP) has been developed in the National Engineers School of Tunis (ENIT). As all residential microgrids, MGP provides a large amount of data from various types of equipment and devices. Each of these data has its format an作者: Proponent 時(shí)間: 2025-3-30 08:24
,Reale Treibhausgasemissionen und Gesamtkosten je Antriebstechnologie und Energietr?ger für repr?sent of Ownership (TCO) Methodik für repr?sentative Fahrzeuge dargelegt. Anhand dessen wird ersichtlich, welche THG-Emissionen (LCA) und Kosten für PKW mit verschiedenen Antriebstechnologien in Kombination mit bestimmten Energietr?gern hervorgehen. Soweit Technologien einschlie?lich der verwendeten Ene作者: 評論性 時(shí)間: 2025-3-30 16:03 作者: hermitage 時(shí)間: 2025-3-30 17:07 作者: A精確的 時(shí)間: 2025-3-31 00:11 作者: Mirage 時(shí)間: 2025-3-31 02:50
On the Statistics-Changing Phase Transition in Gauge Theories It is invariant under a topologically trivial transformation (the one which can be continuously deformed into the identity transformation) but adds a constant under a topologically nontrivial transformation, proportional to the winding number of that transformation.作者: Lipoprotein 時(shí)間: 2025-3-31 06:36
Risikomanagement für volatile Rohstoffm?rkte den meisten Unternehmen ein langfristig, strategisch ausgerichtetes Risikomanagement, das nicht nur situative Einzelma?nahmen, sondern auch ein bewusst aufgestelltes System m?glicher Ma?nahmen zur Risikobew?ltigung umfasst und seine organisatorische Verankerung im Funktionsbereich Beschaffung findet.作者: spondylosis 時(shí)間: 2025-3-31 11:19
Tianyu Fu,Fengming Li,Yukun Zheng,Rui Songl verwendet — spricht schon für ihre eigene Durchg?ngigkeit. Doch spielt sie quantitativ keine Rolle, und . Ergebnisse, nach denen sich bei Kaninchen, die mit ?l übergossen worden waren, die s?mtlichen Organe als mit dem Fett angefüllt erwiesen, sind unglaubwürdig.作者: PHIL 時(shí)間: 2025-3-31 15:26 作者: heartburn 時(shí)間: 2025-3-31 18:13
Methods of Measuring Lipid Peroxidation in Biological Systems: An Overviewtforward to perform, others tedious; some are more sensitive than others, some more prone to interference; some measure end-products, some measure unstable intermediates, and some measure specific identified compounds whilst others measure poorly characterised entities.作者: HARP 時(shí)間: 2025-4-1 00:26
Yukari Shirota,Tosiyasu L. Kuniif liver lesions is expected to increase considerably over the years to come, and therefore detailed knowledge about the specifics of target volume delineation and organ at risk sparing is required for high-quality radiotherapy.作者: BULLY 時(shí)間: 2025-4-1 03:24
978-3-030-06527-0Springer International Publishing AG, part of Springer Nature 2019作者: Hyperlipidemia 時(shí)間: 2025-4-1 08:38 作者: barium-study 時(shí)間: 2025-4-1 13:10
ler Verknüpfungen zwischen Unternehmen - eine Ebene, die ebenfalls zu gestalten ist. .Der Autor vertritt die Meinung, dass das Controlling die Rationalit?t des Supply Chain Management subsidi?r sichern muss - eine ebenso neue wie zukunftstr?chtige Auffassung. .978-3-8244-9074-5978-3-663-10716-3Series ISSN 0175-8802 Series E-ISSN 2945-8129
