Sampling the volcanic plumes at Io: Impact speeds and shock conditions
Abstract The desire to sample material from the interior of Io, by flying through its volcanic plumes, requires consideration of the flyby speed and the types of sample collection techniques that can be utilized. Low speed collection (1–2.5 km s−1) would require an orbit around Io itself, which is unlikely due to the accumulated radiation dose that ...
M. J. Burchell +2 more
wiley +1 more source
Cassini-oval description of atomic binding: a new method to evaluate atomic hardness
This paper reports that the binding process of two heteronuclear atoms can be described by Cassini oval in dynamic form, every molecular state corresponds to one of these graphs. the approach is based on a constraint rule between hardness and deformation of atomic particles, then the critical phenomena of molecular deformation are discovered and the ...
openaire +1 more source
Cassini encounters with hot flow anomaly-like phenomena at Saturn's bow shock [PDF]
The first observations of the kronian equivalent of hot flow anomalies (HFAs) are presented. Using magnetic field and plasma data we discuss two events that were observed upstream of Saturn's bow shock during the first two orbits of the Cassini ...
Bertucci, Cesar +21 more
core +1 more source
Commented Bibliography on Models and Idealizations
This chapter provides a classified and commented bibliography of printedbooks on the philosophy of scientific modeling and related issues, such as representation,idealization, computer simulation, and others. It is intended as a guide forfurther readings
Cassini, Alejandro Pablo F. +1 more
core +1 more source
Geology of the Selk crater region on Titan from Cassini VIMS observations [PDF]
International audienceObservations of Titan obtained by the Cassini Visual and Infrared Mapping Spectrometer (VIMS) have revealed Selk crater, a geologically young, bright-rimmed, impact crater located similar to 800 km north-northwest of the Huygens ...
Brown, R.H. +19 more
core +1 more source
Jupiter Science Enabled by ESA's Jupiter Icy Moons Explorer. [PDF]
Fletcher LN +49 more
europepmc +1 more source
Preliminary interpretation of Titan plasma interaction as observed by the Cassini Plasma Spectrometer: Comparisons with Voyager 1 [PDF]
The Cassini Plasma Spectrometer (CAPS) instrument observed the plasma environment at Titan during the Cassini orbiter's TA encounter on October 26, 2004.
Crary, F +17 more
core
Parametrization of Curves in AutoCAD by the Example of Cassini''s Ovals
A new approach to the integrated study of descriptive geometry and computer graphics in a higher educational institution on the basis of in-depth study of some topics is proposed. The technique is demonstrated in a practical example devoted to the consideration of the possibility of quick creation and investigation of the properties of Cassini ovals on
Timofeeva T.V., Nesterenko M.A.
openaire +1 more source
Structure of Titan's mid-range magnetic tail: Cassini magnetometer observations during the T9 flyby [PDF]
We analyze the magnetic structure of Titan's mid-range magnetic tail (5-6 Titan radii downstream from the moon) during Cassini's T9 flyby. Cassini magnetometer (MAG) measurements reveal a well-defined, induced magnetic tail consisting of two lobes and a ...
Szego, K +7 more
core
An investigation into a semi-porous channel's forced convection of nano fluid in the presence of a magnetic field as a result of heat radiation. [PDF]
Jalili B +6 more
europepmc +1 more source

