Results 81 to 90 of about 314,174 (332)
Lithospheric and atmospheric interaction on the planet Venus [PDF]
Lithospheric and atmospheric interaction in the planet Venus are discussed. The following subject areas are covered: (1) manifestation of exogenic processes using photogeological data; (2) the chemical composition and a chemical model of the troposphere ...
Volkov, Vladislav P.
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ESC Heart Failure, EarlyView.The graphical abstract summarizes the key features of AFMR in terms of epidemiology, pathophysiology, diagnosis, medical therapy and rhythm control, surgical and transcatheter interventions, and future directions. Created in BioRender (https://BioRender.com/3zj03ko).
Matteo Pagnesi +14 more
wiley +1 more source
Peculiarities of the solar wind interaction with the upper atmospheres of Venus and Mars
Geofísica Internacional, 1980 Mediciones de plasma y de campos magnéticos en Venus y Marte así como observaciones de radio ocultamiento de satélites por sus atmósferas y ionosferas superiores revelan algunas diferencias y semejanzas en la configuración del flujo del viento solar ...
T. K. Breus
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Laboratory evaluation of microwave absorption properties under simulated conditions for planetary atmospheres [PDF]
The microwave absorbing properties of gaseous sulfuric acid (H2SO4) under Venus atmospheric conditions are investigated. The results are applied to measurements from Mariner 5, Mariner 10, and Pioneer/Venus Radio Occultation experiments, to determine ...
Steffes, P. G.
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Review of boundary model studies in the Venusian and Martian induced magnetosphere
地球与行星物理论评Although Venus and Mars do not have a global magnetic field but have atmospheres and ionospheres. During their coupling with the solar wind, the induced magnetospheres are created, as well as the boundaries of the bow shock and the magnetic pileup ...
Jiaqi Zhang +6 more
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On the sources of the night side ionosphere of Venus
Geofísica Internacional, 1978 Se presenta una descripción general de las características de la ionósfera nocturna en Venus y del medio magnético y plasmático en su estela. Se sugiere que el carácter variable de la ionósfera nocturna, es debido en parte, a condiciones de asimetría y ...
Héctor Pérez De Tejada
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Revealing the face of Venus: Magellan [PDF]
An overview of the Magellan spacecraft and mission is presented. Topics covered include: a description of the Magellan spacecraft; Venus geology; Venus gravity; synthetic aperture radar; and radar ...
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Epilepsia Open, EarlyView.Abstract Objective We investigated the theoretical optimal venous location for an endovascular seizure detection device using stereo‐EEG (SEEG) data. Methods Six venous sinus segments from consecutive SEEG patients: anterior, middle, and posterior sagittal sinus (SS‐A, SS‐M, SS‐P), straight sinus, and the ipsilateral/contralateral (relative to primary ...
Thanomporn Wittayacharoenpong +9 more
wiley +1 more source
Studies on the small-scale magnetic flux ropes at Venus and Mars
地球与行星物理论评Magnetic flux ropes (MFRs) with twisted magnetic field lines are common in the solar system, most of which can be caused by magnetic reconnection or velocity shear.
Lianghai Xie +4 more
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The solar parallax as derived from the American photographs of the transit of Venus, 1874, December 8-9 [PDF]
, 1881 David P. Todd
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