Results 221 to 230 of about 15,881 (262)

Analysis of lipid-assisted self-assembly of hydrophobic CuInS₂/ZnS quantum dots into water-stable nanoclusters that perform intra-cluster energy transfer.

Nanoscale
Whipp JT, Hancock AM, Aslam Z, Critchley K, Adams PG.   +4 more
europepmc   +1 more source

Self-powered mechanoluminescent elastomer for solar-blind ultraviolet emission. [PDF]

Light Sci Appl
Lv X, Duan T, Fang S, Wang Z, Chen D, Huang L, Liu H, Liu Z, Liu C, Wang XJ, Liang Y.   +10 more
europepmc   +1 more source

Bandgap-engineered Fe-doped LaCoO₃ perovskites for solar-driven photocatalytic degradation of crystal violet. [PDF]

BMC Chem
Kamal R, Pattanaik R, Pradhan D, Dash SK.   +3 more
europepmc   +1 more source

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Solar Particle Emission

Special Publications, 2013
A variety of flare-associated and recurrent solar particle events are analyzed using the technique of 'mapping' the fluxes back to the estimated high coronal longitude of the interplanetary field line passing through the spacecraft. Often it is possible to separate temporal from spatial effects as well as those of coronal and interplanetary propagation.
exaly   +2 more sources

Particle-in-cell simulation of plasma emission in solar radio bursts

Astronomy & Astrophysics, 2021
Aims. The present study aims to shed light on our understanding of the radiation processes of solar radio bursts associated with nonthermal electron propagation in the corona and interplanetary space. Methods. We performed 2.5-dimensional particle-in-cell (PIC) simulations to investigate the plasma emission excited by a relativistic electron beam using
T. M. Li, C. Li, P. F. Chen, W. J. Ding
openaire   +1 more source

Type II Radio Emission and Solar Energetic Particle Events

AIP Conference Proceedings, 2008
Type II radio bursts, solar energetic particle (SEP) events, and interplanetary (IP) shocks all have a common cause, viz., fast and wide (speed ⩾900 km/s and width ⩾60°)) coronal mass ejections (CMEs). Deviations from this general picture are observed as (i) lack of type II bursts during many fast and wide CMEs and IP shocks, (ii) slow CMEs associated ...
Nat Gopalswamy, Gang Li, Qiang Hu, Olga Verkhoglyadova, Gary P. Zank, R. P. Lin, J. Luhmann   +6 more
openaire   +1 more source

Energetic particle emission in two solar flares with open magnetic field

2022
<p>Energetic particle populations in the solar corona and in the heliosphere appear to have different characteristics even when produced in the same solar flare. It is not clear what causes this difference: properties of the acceleration region, the large-scale magnetic field configuration in the flare, or particle transport effects, such
Philippa Browning, Mykola Gordovskyy
openaire   +1 more source