標(biāo)題: Titlebook: Exploration of Halley’s Comet; Michael Grewing,Fran?oise Praderie,Rüdeger Reinhar Conference proceedings 1988 Springer-Verlag Berlin Heide [打印本頁(yè)] 作者: 猛烈抨擊 時(shí)間: 2025-3-21 17:42
書目名稱Exploration of Halley’s Comet影響因子(影響力)
書目名稱Exploration of Halley’s Comet影響因子(影響力)學(xué)科排名
書目名稱Exploration of Halley’s Comet網(wǎng)絡(luò)公開度
書目名稱Exploration of Halley’s Comet網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Exploration of Halley’s Comet被引頻次
書目名稱Exploration of Halley’s Comet被引頻次學(xué)科排名
書目名稱Exploration of Halley’s Comet年度引用
書目名稱Exploration of Halley’s Comet年度引用學(xué)科排名
書目名稱Exploration of Halley’s Comet讀者反饋
書目名稱Exploration of Halley’s Comet讀者反饋學(xué)科排名
作者: Injunction 時(shí)間: 2025-3-21 21:13
http://image.papertrans.cn/e/image/319390.jpg作者: 蟄伏 時(shí)間: 2025-3-22 02:07 作者: finale 時(shí)間: 2025-3-22 07:45 作者: ADAGE 時(shí)間: 2025-3-22 09:27
Giotto magnetic-field results on the boundaries of the pile-up region and the magnetic cavity the following results on the inner plasma boundaries in the magnetoplasma surrounding the comet:.The axis of symmetry had a transverse offset of about 80 000 km from the nucleus..The ionopause must be a tangential discontinuity thereby containing further evidence of the null magnitude of the cavity field.作者: erythema 時(shí)間: 2025-3-22 14:57 作者: erythema 時(shí)間: 2025-3-22 19:52 作者: 凹室 時(shí)間: 2025-3-23 01:07
Perspective: The Hereditary Longing,ased mainly on the magnetohydrodynamic description of the solar wind interaction with cometary plasma: the generation of strong magnetohydrodynamic turbulence by the loading of solar wind by cometary ions, the discovery of thin plasma structures in an inner coma that correlate with the bursts of pla作者: EXPEL 時(shí)間: 2025-3-23 03:48
,Anhang mit Bildtafeln zu den L?tversuchen,istance of ~8 million km upstream of the bow shock of comet P/Halley. The protons were observed to be elastically scattered out of their original cycloidal trajectories such that they were nonuniformly distributed over a spherical shell in velocity space. The shell radius (relative to its expected r作者: Graphite 時(shí)間: 2025-3-23 08:40
Eigenschaften und Aufbau von Hartmetallen,de observations of the proton and alpha particle distributions in the solar wind with 8 seconds time resolution. As the comet was approached, fluctuations were observed in all the primary bulk parameters, i.e. density, temperature and flow velocity, of both distributions at levels above the usual so作者: follicle 時(shí)間: 2025-3-23 12:53 作者: 腐爛 時(shí)間: 2025-3-23 17:22
General Thoughts on Capitalism,-Zinner and for comet Halley. Whereas previous reports have been concerned either with the magnetic field observations or with plasma observations, here we combine observations of the magnetic field with the solar wind proton and alpha particle distributions. This allows the three possible modes of 作者: reject 時(shí)間: 2025-3-23 21:11 作者: outset 時(shí)間: 2025-3-24 01:05 作者: 托運(yùn) 時(shí)間: 2025-3-24 04:06 作者: Frequency 時(shí)間: 2025-3-24 09:11 作者: tendinitis 時(shí)間: 2025-3-24 11:26 作者: 大喘氣 時(shí)間: 2025-3-24 15:44 作者: 值得 時(shí)間: 2025-3-24 22:10
Coda: Art in Conversation with Art, Halley on 1986, March 6 and 9. Electric fields are measured in the bandwidth 0–300 kHz with an antenna made of two spheres separated by a distance of 11 m. As the nucleus is approached, the average amplitude and bandwidth of the AC electric field increase dramatically; at frequencies above 1 kHz, t作者: 忙碌 時(shí)間: 2025-3-25 01:40
Integrated Systems of Mollusk Cultureexcept near the bow shock and that of alpha particle was almost constant (~ 7 cm.) in the cometosheath. Temperature of protons seems to decrease from bow shock to about 2 10. km, and increase thereafter slightly, but that of alpha particle seems to be almost constant. This decrease is likely caused 作者: interpose 時(shí)間: 2025-3-25 06:13
Harvesting Rainwater fromBuildingsclosest to Halley, ~28 10. km. No evidence is found for the presence of heavy ion cyclotron waves. However, from this search, two new wave modes are discovered in the solar wind: electromagnetic waves near the proton cyclotron frequency and drift mirror mode “waves”. Both modes have scales of 10–60 作者: PLUMP 時(shí)間: 2025-3-25 08:44 作者: 知識(shí) 時(shí)間: 2025-3-25 15:28 作者: PUT 時(shí)間: 2025-3-25 18:46
https://doi.org/10.1007/978-3-642-82971-0Libration; Perihel; Population; dynamics; environment; evolution; ionosphere; iron; observatory; solar; solar 作者: orient 時(shí)間: 2025-3-25 22:58
https://doi.org/10.1007/978-3-7091-8127-0The Giotto RPA-COPERNIC plasma experiment identified several regions in which the solar wind interaction with the cometary plasma displayed characteristic features:.The detailed plasma features associated with these regions are successively described.作者: conduct 時(shí)間: 2025-3-26 01:37 作者: 憤憤不平 時(shí)間: 2025-3-26 08:21
General features of comet P/Halley: solar wind interaction from plasma measurementsThe Giotto RPA-COPERNIC plasma experiment identified several regions in which the solar wind interaction with the cometary plasma displayed characteristic features:.The detailed plasma features associated with these regions are successively described.作者: 種族被根除 時(shí)間: 2025-3-26 10:33 作者: 模范 時(shí)間: 2025-3-26 16:01 作者: 口訣 時(shí)間: 2025-3-26 17:49
https://doi.org/10.1007/978-3-642-51505-7ley (Olson, 1979), a great deal of new information has come to light. We present a synopsis of the textual, visual, and astronomical evidence to support the theory that when Giotto painted his comet in the Scrovegni Chapel he was reflecting his viewing of Comet Halley in 1301.作者: 調(diào)味品 時(shí)間: 2025-3-27 00:44 作者: EWER 時(shí)間: 2025-3-27 04:44 作者: Locale 時(shí)間: 2025-3-27 07:58
https://doi.org/10.1007/978-3-030-56429-2 those sampled by Vega and Sakigake, it is important to compare observations from the three missions that carried dedicated wave instruments. Here we summarize ICE plasma wave measurements associated with both comet encounters and relate the very high sensitivity ICE observations to corresponding measurements from the other Halley spacecraft.作者: 爭(zhēng)吵 時(shí)間: 2025-3-27 11:58 作者: Melanocytes 時(shí)間: 2025-3-27 15:28
Waves in the magnetic field and solar wind flow outside the bow shock at comet P/Halleypropagation for these waves to be separated. The magnetic component is predominantly transverse to the magnetic field and linearly polarised. The flow vector also has a substantial amount of power parallel to the magnetic field. A examination of the pressure variations shows that slow magnetosonic waves are more common than the fast mode.作者: Accede 時(shí)間: 2025-3-27 21:48
Plasma flow in the cometosheath of P/Halley during the encounter of Suiseiby the cooling effect accompanying with the charge exchange process as well as with the mass addition of cold pickup ions. On the contrary, the observed temperature of alpha particles stayed almost constant throughout the cometosheath. This is because that there is no effective cooling process for alpha particles within the cometosheath.作者: 鬼魂 時(shí)間: 2025-3-28 00:45 作者: 縱欲 時(shí)間: 2025-3-28 02:57
Harvesting Rainwater fromBuildingsar wind streams, presumably associated with stream-stream interactions. VLF electrostatic emissions are found to occur in field minima or at gradients of the drift mirror structures. Possible generation mechanisms of drift mirror mode waves, cyclotron waves and electrostatic waves are discussed.作者: CHANT 時(shí)間: 2025-3-28 10:07 作者: 發(fā)生 時(shí)間: 2025-3-28 13:51
munity with a wealth of exciting new discoveries, the most remarkable of which was undoubtedly the first image of a cometary nucleus. Halley‘s Comet is the brightest periodic comet, and the most famous of the 750 known comets. With its 76-year period, its recent appearance was truly a "once-in-a-lif作者: 裝飾 時(shí)間: 2025-3-28 15:21
,Anhang mit Bildtafeln zu den L?tversuchen,oidal trajectories such that they were nonuniformly distributed over a spherical shell in velocity space. The shell radius (relative to its expected radius) and thickness increased as the bow shock was approached. Down-stream of the shock, the cometary protons could not be distinguished from the heated solar wind protons.作者: NUL 時(shí)間: 2025-3-28 19:08
,Schutz gegen Unf?lle beim Spanablauf,e environment of the comet directly taking the opportunity of the re-revisiting of the first class comet, Halley. Plasma and neutral hydrogen environments were selected for scientific exploration. This article gives the overview of recent scientific results of our missions作者: 抵押貸款 時(shí)間: 2025-3-29 02:06 作者: fatty-acids 時(shí)間: 2025-3-29 04:31 作者: 冷峻 時(shí)間: 2025-3-29 07:56
Perspective: The Hereditary Longing,mation of these structures and boundaries. The paper reviews the observations of these phenomena from spacecraft and the kinetic theories of cometary plasma that were developed recently and that are able to provide a natural explanation of observed puzzling phenomena.作者: orthopedist 時(shí)間: 2025-3-29 14:21
https://doi.org/10.1007/978-3-642-93385-1 km. There is evidence for a further excursion back into the cometary ion foot after the initial shock crossing. The cometary ion density is inferred from the solar wind speed changes and is compared with measurements.作者: allude 時(shí)間: 2025-3-29 16:28
Einleitung und Geschichte der Hartstoffe,oard Vega-1 and as expected from quasilinear theory. The entrance into the cometary bow shock is furthermore characterized by an order of magnitude increase of the fluctuation level, both on the in- and outbound pass of Giotto.作者: 動(dòng)脈 時(shí)間: 2025-3-29 23:20
Samson Mil’shtein,Dhawal Asthanaely, and with an IMF sector boundary observed by Vega-1 on March 7.9 UT. Additional work is needed to determine the possible role of solarwind plasma effects in producing the DE. Relationships between other occurrences of plasma-tail activity and Halley Armada spacecraft measurements remain to be explored.作者: 主動(dòng) 時(shí)間: 2025-3-30 00:35
Encounters with comets: discoveries and puzzles in cometary plasma physicsmation of these structures and boundaries. The paper reviews the observations of these phenomena from spacecraft and the kinetic theories of cometary plasma that were developed recently and that are able to provide a natural explanation of observed puzzling phenomena.作者: 人造 時(shí)間: 2025-3-30 05:14
Solar wind flow through the comet P/Halley bow shock km. There is evidence for a further excursion back into the cometary ion foot after the initial shock crossing. The cometary ion density is inferred from the solar wind speed changes and is compared with measurements.作者: OMIT 時(shí)間: 2025-3-30 08:48 作者: 弄臟 時(shí)間: 2025-3-30 15:14 作者: muscle-fibers 時(shí)間: 2025-3-30 20:17
The pick-up of cometary protons by the solar windoidal trajectories such that they were nonuniformly distributed over a spherical shell in velocity space. The shell radius (relative to its expected radius) and thickness increased as the bow shock was approached. Down-stream of the shock, the cometary protons could not be distinguished from the heated solar wind protons.作者: Peak-Bone-Mass 時(shí)間: 2025-3-30 20:49 作者: 洞穴 時(shí)間: 2025-3-31 01:04 作者: 主動(dòng) 時(shí)間: 2025-3-31 05:25
Fine structure of the magnetic field in comet P/Halley’s comaed at distances of 50 ÷ 70 10. km. Most likely these events are due to spatial plasma irregularities inside the coma region and not to temporal field variations. The observed effects may be caused by cometary plasma rays.作者: 舞蹈編排 時(shí)間: 2025-3-31 11:27
New information on comet P/Halley as depicted by Giotto di Bondone and other Western artistsal evidence of comet P/Halley at several passages through that of 1301 and compare it with descriptions and modern images. Since it was first recognized that Giotto di Bondone painted a comet in place of the Star of Bethlehem and suggested that this was a portrait of the 1301 apparition of comet Hal作者: 懶惰人民 時(shí)間: 2025-3-31 15:42
Encounters with comets: discoveries and puzzles in cometary plasma physicsased mainly on the magnetohydrodynamic description of the solar wind interaction with cometary plasma: the generation of strong magnetohydrodynamic turbulence by the loading of solar wind by cometary ions, the discovery of thin plasma structures in an inner coma that correlate with the bursts of pla作者: CANE 時(shí)間: 2025-3-31 20:23
The pick-up of cometary protons by the solar windistance of ~8 million km upstream of the bow shock of comet P/Halley. The protons were observed to be elastically scattered out of their original cycloidal trajectories such that they were nonuniformly distributed over a spherical shell in velocity space. The shell radius (relative to its expected r作者: CROAK 時(shí)間: 2025-4-1 01:31 作者: Lumbar-Stenosis 時(shí)間: 2025-4-1 05:05
The Sakigake/Suisei encounter with comet P/Halley P/Halley at minimum distances of 7 million and 150 thousand kilometers respectively. The scientific objectives of these spacecraft were to explore the environment of the comet directly taking the opportunity of the re-revisiting of the first class comet, Halley. Plasma and neutral hydrogen environm作者: Carcinogenesis 時(shí)間: 2025-4-1 08:09
Waves in the magnetic field and solar wind flow outside the bow shock at comet P/Halley-Zinner and for comet Halley. Whereas previous reports have been concerned either with the magnetic field observations or with plasma observations, here we combine observations of the magnetic field with the solar wind proton and alpha particle distributions. This allows the three possible modes of
