Results 191 to 200 of about 2,436,355 (386)
Solar Wind Protons in the Diamagnetic Cavity at Comet 67P/Churyumov-Gerasimenko. [PDF]
Goetz C+7 more
europepmc +1 more source
Implications of Observations of the Solar Wind and Corona for Solar Wind Models [PDF]
J. F. McKenzie, W. I. Axford
openaire +3 more sources
HKUST‐1/TiO2 composite materials show a very high photocatalytic hydrogen evolution rate which increases as a function of the irradiation time until reaching a plateau and even surpasses the performance of the 1%Pt/TiO2 material after three photocatalytic cycles.
Alisha Khan+9 more
wiley +1 more source
Revisiting the Solar Wind Deceleration Upstream of the Martian Bow Shock Based on MAVEN Observations
The solar wind deceleration upstream of the Martian bow shock is examined using particle and magnetic field measurements obtained by the Mars Atmosphere and Volatile EvolutioN (MAVEN).
Yuqi Liu+8 more
doaj +1 more source
11- and 22-year variations of the cosmic ray density and of the solar wind speed [PDF]
Cosmic ray density variations for 17-21 solar activity cycles and the solar wind speed for 20-21 events are investigated. The 22-year solar wind speed recurrence was found in even and odd cycles. The 22-year variations of cosmic ray density were found to
Chirkov, N. P.
core +1 more source
Ozone‐based gas‐phase metal‐assisted chemical etching enables unprecedented room‐temperature fabrication of high‐quality silicon nanowires. The superior oxidation potential of O3 drives rapid vertical etching (1 µm min−1) while maintaining exceptional structural integrity. The pristine nanowire surfaces enable high‐performance core‐shell photodetectors
Hyein Cho+11 more
wiley +1 more source
Interchange reconnection as the source of the fast solar wind within coronal holes. [PDF]
Bale SD+16 more
europepmc +1 more source
The Effect of a Solar Wind Blast Wave on the Chromosphere.
Donat G. Wentzel, Alan B. Solinger
openalex +2 more sources
Triple Passivation Treatment (TPT) strategy enables 1.75 eV wide‐bandgap perovskite solar cells (WB‐PSCs) with suppressed halide phase segregation and n‐to‐p type surface transition. The photoluminescence quantum yield increases from 0.5 to 2.1%, indicating reduced non‐radiative losses.
Siming Huang+12 more
wiley +1 more source
Magnetosheath Jet Formation Influenced by Parameters in Solar Wind Structures. [PDF]
Koller F+5 more
europepmc +1 more source