Synonyme wurden verwendet für:
Solar wind
•
wind
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keywords:(Solar wind)
RIMS analysis of Ca and Cr in Genesis solar wind collectors
Effects of satellite dimensions in the solar pressure formulation for formation flying
The occurrence of operational anomalies in spacecraft and their relationship to space weather
Characteristics of the radiation field in low earth orbit and in deep space
Multifractal analysis of high resolution solar wind proton density measurements
Generalized Bohm sheath criterion in dusty plasma of space environment
The relative biological effectiveness of proton and ion beams
Physical and biomedical countermeasures for space radiation risk
Sharp boundaries of solar wind plasma structures and their relationship to solar wind turbulence
Optimum area of solar array for stratospheric solar-powered airship
Electric sail displaced orbit control with solar wind uncertainties
Effect of uncertainties in solar synoptic magnetic flux maps in modeling of solar wind
Sunspot activity and cosmic ray modulation at 1a.u. for 1900–2013
Tribocharging and electrical grounding of a drill in shadowed regions of the Moon
A wavelet based approach to Solar–Terrestrial Coupling
Predicted dependence of the cross polar cap potential saturation on the type of solar wind stream
Optimal stereoscopic angle for reconstructing solar wind inhomogeneous structures
Effect of current sheets on the power spectrum of the solar wind magnetic field using a cell model
Fast Analysis of Multi-Asteroid Exploration Mission Using Multiple Electric Sails
Fast measurements of parameters of the Solar Wind using the BMSW instrument
Fast measurements of parameters of the Solar Wind using the BMSW instrument
CME–flare association during the 23rd solar cycle
Correlation level between solar wind and magnetosheath plasma and magnetic field parameters
Thermospheric winds over Abuja during solar minimum period
Solar cycle variations of magnetopause locations
Changes in sea-level pressure over South Korea associated with high-speed solar wind events
Relation between Dst* and interplanetary parameters during single-step geomagnetic storms