Results 91 to 100 of about 322,202 (327)

Occultation of a compact radio source by Venus [PDF]

open access: yes, 1992
An occultation of the compact radio source P 0507+17 by Venus on 19 Jul. 1988, was observed in Tidbinbilla, Australia at a frequency of 2.3 GHz. The purpose of this observation was to measure the position of Venus in the radio reference frame.
Linfield, R.
core   +1 more source

Identification of Surface, Interface, and Bulk States on the Pristine and Passivated InP (001) and (111) Surfaces Using Surface Photovoltage Spectroscopy

open access: yesphysica status solidi (RRL) – Rapid Research Letters, EarlyView.
This study investigates surface, interface, and bulk states of pristine and passivated InP crystals, which show distinct characteristics due to their different growth orientations and reconstructions. The study also examines how radiative and nonradiative processes related to surface reconstruction influence luminescence and absorption phenomena, that ...
Deepesh Nimje   +7 more
wiley   +1 more source

Mantle avalanches in a Venus-like stagnant lid planet

open access: yesEarth and Planetary Physics
Stagnant lid planets are characterized by a globe-encircling, conducting lid that is thick and strong, which leads to reduced global surface heat flows. Consequently, the mantles of such planets can have warmer interiors than Earth, and interestingly, a ...
Madeleine C. Kerr, Dave R. Stegman
doaj   +1 more source

Peculiarities of the solar wind interaction with the upper atmospheres of Venus and Mars

open access: yesGeofísica 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
doaj   +1 more source

Comments on the tectonism of Venus [PDF]

open access: yes
Preliminary tectonic mapping of Venus from Venera 15/16 images shows unquestionable evidence of at least limited horizontal tectonism. The majority of tectonic features on Venus have no relation to topography.
Kozak, R. C., Schaber, G. G.
core   +1 more source

Progress of MXenes‐based responsive materials for soft sensors and actuators

open access: yesResponsive Materials, EarlyView.
MXene, a promising 2D material, excels at mimicking human sensing and feedback system, making it ideal for intelligent robots. This review first covers its structure, properties, and synthesis. It then summarizes recent MXene‐based sensors and actuator.
Peidi Zhou   +10 more
wiley   +1 more source

On the sources of the night side ionosphere of Venus

open access: yesGeofísica 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
doaj   +1 more source

Methane measurement by the Pioneer Venus large probe neutral mass spectrometer [PDF]

open access: yes
The Pioneer Venus Large Probe Mass Spectrometer detected a large quantity of methane as it descended below 20 km in the atmosphere of Venus. Terrestrial methane and Xe-136, both originating in the same container and flowing through the same plumbing ...
Donahue, T. M., Hodges, R. R., Jr.
core   +1 more source

Building Connections to Teach the Nature of Science: An Experienced Science Teacher's Formative Assessment Practices in a High School Classroom

open access: yesJournal of Research in Science Teaching, EarlyView.
ABSTRACT While understanding the nature of science (NOS) is recognized as a key component of science education because of its potential benefits in nurturing scientific literacy, there is currently limited knowledge on how NOS learning can be supported by teachers' ongoing, in‐the‐moment assessment in the classroom.
Wonyong Park   +2 more
wiley   +1 more source

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