標(biāo)題: Titlebook: Mars’ Magnetism and Its Interaction with the Solar Wind; Daniel Winterhalter,Mario Acu?a,Alexander Zakharov Book 2004 Springer Science+Bus [打印本頁] 作者: 不同 時間: 2025-3-21 18:56
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作者: 簡潔 時間: 2025-3-21 20:34
Daniel Winterhalter,Mario Acu?a,Alexander ZakharovA primary reference for the researcher studying solar wind/planet interactions.Includes supplementary material: 作者: 拉開這車床 時間: 2025-3-22 01:27
Space Sciences Series of ISSIhttp://image.papertrans.cn/m/image/624866.jpg作者: 靈敏 時間: 2025-3-22 05:46
978-90-481-6582-7Springer Science+Business Media Dordrecht 2004作者: Detain 時間: 2025-3-22 09:02
Mars’ Magnetism and Its Interaction with the Solar Wind978-0-306-48604-3Series ISSN 1385-7525 作者: Gorilla 時間: 2025-3-22 14:38
The Plasma Environment of Marsservations. However, measurements by the Phobos-2 and Mars Global Surveyor (MGS) spacecraft, with different instrument complements and orbital parameters, led to a significant improvement of our knowledge about the regions and boundaries surrounding Mars.作者: anticipate 時間: 2025-3-22 17:55
1385-7525 an internal magnetic field is of fundamental importance to the understanding of Mars‘ formation and thermal evolution, and of the evolution of Mars‘ atmosphere, surprisingly few of the many spacecraft sent to Mars were equipped with instrumentation for such investigations. Of the 9 or so orbiters th作者: 打折 時間: 2025-3-22 23:34 作者: dandruff 時間: 2025-3-23 04:51
Mars Crustal Magnetism an inner core is likely. Thermal evolution models cannot yet distinguish between these two possibilities. The magnetic record contains a wealth of information on the thermal evolution of Mars and the Mars dynamo, but we have just begun to decipher its message.作者: gnarled 時間: 2025-3-23 09:15
Unusually Distant Bow Shock Encounters at Mars: Analysis of March 24, 1989 Eventystem of discontinuities observed in the solar wind between 18:42 and 19:36 UT was the consequence of unusually distant planetary bow shock excursions. The cause was unusually small ρV. and .. values in the solar wind flow.作者: Exploit 時間: 2025-3-23 13:15
M. I. Verigin,J. Slavin,A. Szabo,G. A. Kotova,A. P. Remizov,H. Rosenbauer,S. Livi,K. Szeg?,M. Tátral作者: ARBOR 時間: 2025-3-23 16:16
Bow Shock and Upstream Phenomena at Marsmagnetic field data (Acu?a ., 1998). As detailed by a series of review papers in this monograph, the Mars Global Surveyor (MGS) mission has now shown that the Mars environment is very complex with strong, highly structured crustal magnetic remnants in the southern hemisphere, while the northern hemi作者: 小教堂 時間: 2025-3-23 19:50 作者: meditation 時間: 2025-3-23 23:02 作者: absorbed 時間: 2025-3-24 04:46
Magnetic Flux Ropes in the Martian Atmosphere: Global Characteristicsentation is more horizontal near the terminator for altitudes greater than 200 km. We have identified fewer flux ropes for SZA between 40 to 60 deg and for SZA lower than 20 deg, like in the case of Venus (Elphic and Russell, 1983b). Statistically, Mars’ ionosphere with SZA range between 40. to 60. 作者: hangdog 時間: 2025-3-24 10:09
Mars Express and MARSISwhich have been predicted in the dayside/terminator ionosphere. Measurements on the nightside can be used to search for proposed fine structures (‘holes’) in the electron density. Hydrodynamic waves are predicted to be excited by the solar wind/ionosphere interaction and their influence on the elect作者: Arrhythmia 時間: 2025-3-24 13:37
1385-7525 he solar wind comes, for the first time, into sharp focus. This work, detailing the integration and new interpretation of the MGS and Phobos results, is a primary reference for the researcher studying solar wind/planet interactions. .978-90-481-6582-7978-0-306-48604-3Series ISSN 1385-7525 作者: Gourmet 時間: 2025-3-24 18:03
Mars’ Magnetism and Its Interaction with the Solar Wind作者: Gourmet 時間: 2025-3-24 19:09
Book 2004teraction between Mars and the solar wind comes, for the first time, into sharp focus. This work, detailing the integration and new interpretation of the MGS and Phobos results, is a primary reference for the researcher studying solar wind/planet interactions. .作者: 初學(xué)者 時間: 2025-3-25 00:08 作者: 性行為放縱者 時間: 2025-3-25 06:29
A. F. Nagy,D. Winterhalter,K. Sauer,T. E. Cravens,S. Brecht,C. Mazelle,D. Crider,E. Kallio,A. Zakhartiellen Differentialgleichungen. In den beiden letzten Kapiteln werden einige der grundlegenden Begriffe der Finanzmathematik eingeführt? und es wird gezeigt, wie man Methoden der stochastischen Differentialgleichungen erfolgreich einsetzen kann, um Optionen korrekt zu bewerten (Black-Scholes-Formel)..?.?.?.?.978-3-658-00987-8978-3-658-00988-5作者: 煩擾 時間: 2025-3-25 07:35
C. Mazelle,D. Winterhalter,K. Sauer,J. G. Trotignon,M. H. Acu?a,K. Baumg?rtel,C. Bertucci,D. A. Brairechenden Gütekriterien (Reliabilit?t und Validit?t) hier ausführlich und mit zahlreichen Beispielen behandelt. Daneben wird auch – deutlich kürzer – die zweite Form der Datenerhebung, die Beobachtung, vorgestellt und durch Beispiele illustriert. Hier sei ausdrücklich darauf hingewiesen, dass die Da作者: 商店街 時間: 2025-3-25 13:32 作者: 相信 時間: 2025-3-25 19:11 作者: 思想流動 時間: 2025-3-25 22:24 作者: Tractable 時間: 2025-3-26 02:21 作者: 為敵 時間: 2025-3-26 07:05 作者: 寬容 時間: 2025-3-26 08:56
a disability is a handicap depends on a number of factors such as the type of job a person has, the services which exist to help, the attitudes of society and the personality of the person with the disability. Ann Shearer illustrates this point by arguing that not being able to run for a bus would 作者: CRATE 時間: 2025-3-26 13:02 作者: jocular 時間: 2025-3-26 17:14 作者: conception 時間: 2025-3-26 21:14 作者: Figate 時間: 2025-3-27 04:29 作者: 歹徒 時間: 2025-3-27 08:41 作者: 用手捏 時間: 2025-3-27 09:59 作者: Projection 時間: 2025-3-27 16:17
D. Vignes,M. H. Acu?a,J. E. P. Connerney,D. H. Crider,H. Rème,C. Mazelle-house themes, and Herbert’s seeming homeliness. The simplicity is, of course, deceptive. In fourteen lines, Herbert traces a soul’s journey from ignorance to knowledge, from sin to ‘redemption’, from death to life. The theme is a quest, and the treatment of time is highly sophisticated. The ‘I’ of 作者: Organization 時間: 2025-3-27 19:02 作者: 胰島素 時間: 2025-3-28 01:37
oint in their lives and most people are ‘a(chǎn)ble’ in some situations and not in others. The line from ‘normality’ to ‘a(chǎn)bnormality’ is a continuum with no sharp cut-off point. Labelling some people as ‘the disabled’ is part of the problem of disability. Whilst it is impossible to reach any clear and una作者: Ceramic 時間: 2025-3-28 03:49 作者: 易達(dá)到 時間: 2025-3-28 07:47
The Plasma Environment of Marsdepending upon whether this obstacle has a large-scale planetary magnetic field and/or a well-developed atmosphere/ionosphere. For a number of years significant uncertainties have existed concerning the nature of the solar wind interaction at Mars, because of the lack of relevant plasma and field ob作者: Rinne-Test 時間: 2025-3-28 12:34 作者: SPALL 時間: 2025-3-28 15:48 作者: palliative-care 時間: 2025-3-28 21:59
Mars Global Surveyor Observations of Solar Wind Magnetic Field Draping Around Marsents at a large range of altitudes, local times, and solar zenith angles as the spacecraft orbit evolved. We choose orbits with very clean signatures of draping to establish the nominal morphology of the magnetic field lines at local times of near-subsolar and near-terminator. Next, using a compilat作者: foppish 時間: 2025-3-29 02:45 作者: Platelet 時間: 2025-3-29 06:36
Unusually Distant Bow Shock Encounters at Mars: Analysis of March 24, 1989 Eventanetary obstacle and bow shock models relevant for the period of Phobos 2 observations and for low Mach numbers, respectively. It is proven that the system of discontinuities observed in the solar wind between 18:42 and 19:36 UT was the consequence of unusually distant planetary bow shock excursions
