Injection Energy Research Articles

Clean three-level direct-phonon injection terahertz quantum cascade laser

For terahertz quantum cascade lasers employing the nonalignment injection scheme via direct-phonon resonance, this study presents the crucial effect of parasitic absorption in the narrow module architecture based on only two quantum wells. The optical gain can be restricted to small (or negative) values even at the low temperature. To address this issue, a suppression strategy by increasing the injection energy is used to isolate the relevant levels. The feasibility of this strategy is experimentally demonstrated by observing lasing at 194 K.

Predictive simulations for plasma scenarios in the SMART tokamak

The SMall Aspect Ratio Tokamak (SMART) is a new spherical machine that is currently being constructed at the University of Seville (Mancini et al., 2021; Agredano-Torres et al., 2021). The operation of SMART will cover three different phases reaching an inductive plasma current (IP) of more than 500 kA, a toroidal magnetic field (BT) of 1 T and a pulse length of 500 ms (Mancini et al., 2021; Agredano-Torres et al., 2021). The main goal of the SMART tokamak is to study high plasma confinement regimes in a broad triangularity range (-0.5≤δ≤0.5) (Doyle et al., 2021; Doyle et al., 2021). While in phase 1 the ohmic heating alone is expected to provide enough power to access the H-mode, in phase 2 and phase 3 the access to the H-mode will be ensured by applying Neutral Beam Injection (NBI) as external heating system. The NBI will consist of one injector at 25 keV and 1 MW of power. The overall design of the NBI, including injection geometry, energy and power have been optimized using the ASCOT5 code (Hirvijoki et al., 2021). The SMART scenarios have been developed with the help of the free boundary equilibrium solver code FIESTA (Cunningham, 2013) coupled to the linear time independent, rigid plasma model RZIP (Lazarus et al., 1990) to calculate the target equilibria for all the different operational phases. To assess the feasibility of those scenarios, predictive modelling needs to be included to evaluate properly the evolution of the temperatures, density profiles for both electrons and ions. To this extent, the 1.5D transport code ASTRA (Pereverzev and Yushmanov, 2002) has been used including models for the ohmic current, bootstrap current and current driven by NBI. This contribution discusses the electron and ion density and temperature profiles obtained for various scenarios for phase 1 and 2 and presents the design study of the NBI.

Pixelation of GaN based Micro-LED arrays by tailoring injection energy and dose of fluorine ion implantation

The pixelation of Micro-LED still faces intractable technological problems with the shrinkage of pixel by using conventional mesa etching processes, such as reduced luminous efficiency and tough metal interconnection. In this work, a novel pixelation strategy using fluorine (F) ion implantation with tailored injection energy and dose has been proposed and investigated through simulation and experiment. It is found that both the injection depth and spatial distribution range are determined by injection energy. The lateral spreading of the F ions could be effectively suppressed by decreasing injection energy and increasing dose while achieving equal electrical isolation. Furthermore, the uniformity of lateral spreading could be improved by introducing multi-energy injections. For verification and demonstration, Micro-LED arrays with fixed pitch and various pixel sizes were fabricated by F ion implantation, both photoluminescence and electroluminescence characteristics show that the pixel contrast and uniformity are well maintained even for the Micro-LED array with pixel size of 10 μm. For Micro-LED array with pitch and pixel sizes of 40 μm and 10 μm, the reverse leakage currents at a reverse bias voltage of −5 V is 1.45 × 10−7 A, which is lower than that formed by conventional bench top etching. The pixelation method by fluorine ion implantation with tailored injection energy and dose is expected to be able to pave the way toward high-performance Micro-LED and Nano-LED displays.

Transitions between surface force- and inertia-dominant contact dynamics regimes in high-speed scanning probe microscopy

In contact mode scanning probe microscopy (SPM), the microcantilever probe’s dynamics are governed by the (short-range) surface interaction forces, where the tip is “always-in-contact” with the sample. In intermittent contact modes such as “tapping” or bimodal SPM, on the other hand, these are governed by the frequency of the microcantilever’s own external excitation. However, when contact mode is employed with high scan speeds (for “video-rate” SPM), we see intermittent transitions—within a single oscillation cycle—between the “always-in-contact” regime and another which is dominated by the microcantilever’s inertia. We find—through experiments and physical modeling—that the fast in-plane motion of the sample relative to the probe results in a high surface excitation frequency v/λ (and its harmonics), which excite the microcantilever’s out-of-plane eigenmodes and cause it to “break free” of the surface and “overshoot” and “parachute.” The impacts of the tip that consequently occur upon the sample inject energy over a wide frequency band into the higher eigenmodes, especially when operating in a low dissipation ambient environment. The microcantilever, then, exhibits phenomena such as eigenmode switching, sidebands, and fractional and combination resonances; such behavior is not seen in, say, tapping mode SPM, since, there, energy is injected at an externally-determined temporal rate. This article investigates the transition from the dynamics of the microcantilever at low speeds to that exhibited at high speeds. The model for dynamic contact loss is validated against the experiments and can be used to propose mitigation of such dynamics in order to achieve high-resolution imaging.

Comment on "Nonideal Fields Solve the Injection Problem in Relativistic Reconnection".

Recently, Sironi (PRL, 128, 145102; S22) reported the correlation between particles accelerated into high energy and their crossings of regions with electric field larger than magnetic field (E>B regions) in kinetic simulations of relativistic magnetic reconnection. They claim that electric fields in E>B regions (for a vanishing guide field) dominate in accelerating particles to the injection energy. S22 presented test-particle simulations showing that if particle energies are reset to low energies in E>B regions, efficient injection is suppressed. This Comment re-examines these claims by analyzing a simulation resembling the reference case in S22. We show that during crossings E>B acceleration only contributes a small fraction to the injection energy as E>B regions only host particles for a short duration. The energization before any E>B crossings has a comparable contribution, indicating E>B regions are not unique in pre-accelerating particles. A new test-particle simulation shows that zero-outing electric fields in E>B regions does not strongly influence the injection. We suggest that the procedure used in S22 to exclude E>B acceleration partly removes acceleration outside E>B regions, leading to a false conclusion.

Particle Injection and Nonthermal Particle Acceleration in Relativistic Magnetic Reconnection* *Released January 10, 2023.

Magnetic reconnection in the relativistic regime has been proposed as an important process for the efficient production of nonthermal particles and high-energy emission. Using fully kinetic particle-in-cell simulations, we investigate how the guide-field strength and domain size affect the characteristic spectral features and acceleration processes. We study two stages of acceleration: energization up until the injection energy γ inj and further acceleration that generates a power-law spectrum. Stronger guide fields increase the power-law index and γ inj, which suppresses acceleration efficiency. These quantities seemingly converge with increasing domain size, suggesting that our findings can be extended to large-scale systems. We find that three distinct mechanisms contribute to acceleration during injection: particle streaming along the parallel electric field, Fermi reflection, and the pickup process. The Fermi and pickup processes, related to the electric field perpendicular to the magnetic field, govern the injection for weak guide fields and larger domains. Meanwhile, parallel electric fields are important for injection in the strong guide-field regime. In the post-injection stage, we find that perpendicular electric fields dominate particle acceleration in the weak guide-field regime, whereas parallel electric fields control acceleration for strong guide fields. These findings will help explain the nonthermal acceleration and emission in high-energy astrophysics, including black hole jets and pulsar wind nebulae.

Effects of rock ductility on the fracability of ductile reservoirs: An experimental evaluation

Deep hydrocarbon resources below 4000 m are an important replacement for shallow-depth resources; however, as depth increases, the difficulty and cost of development increase sharply. One of the possible reasons is that deep reservoir rocks exhibit strong ductility, which causes difficulties to stimulate a well-developed fracture network in rocks. To date, the mechanism by which rock ductility affects reservoir fracturing remains unclear, and there is a lack of quantitative evaluation models for reservoir fracability. To overcome the problems, in this study, artificial rock specimens with different ductility were fabricated using similar materials based on the geological data and petrophysical properties of the target deep reservoir; the specimens were classified using the proposed ductility index BIf. The hydrofracturing and CT scanning experiments of the artificial specimens with different BIf values under various horizontal stress differences Kh were conducted. The spatial fractal index Df was proposed to characterize the three-dimensional morphology and development of the fracturing network. The fracability evaluation function of ductile rock correlating the indices BIf and Kh was established. It was shown that ductile rocks tended to form non-planar hydraulic fractures with obvious tortuosity and the degree of fracture network development was lower than that of brittle rocks. The maximum breakdown pressure was approximately twice that of the brittle specimen, while the corresponding injection energy was approximately 5–10 times and the energy dissipation of fracture propagation was approximately 4–6 times those of the brittle rock. When Kh ≥ 0.3 the maximum horizontal principal stress played a major role in controlling the hydraulic fracture propagation in ductile rocks. If Kh < 0.3, the fracture propagation in rocks was mainly governed by material ductility rather than the maximum horizontal principal stress. This study provides a new way to explore and quantify the effect of rock ductility on the fracability of deep reservoirs.

Energy, exergy, and economic (3E) analysis of air bubbles injection into plate heat exchangers

Energy, exergy, and economic (3E) analysis of air bubbles injection into plate heat exchangers

Host Material for Multi‐Color Display with High and Stable Electro‐Phosphorescent Efficiencies: Meta‐Linkage for Balanced Hole and Electron Injection

AbstractNovel host materials and their molecular design methods for phosphorescent materials are crucial for the application of phosphorescent organic light emitting diodes (PhOLEDs), which require balanced carrier injection and sufficient triplet energy levels (ET). Herein, two host materials, namely PPI22PPPBO and PPI33PPPBO, are designed by varying the linkage of benzoxazole (PBO) and phenanthroimidazole (PPI) groups with appropriate ET for green, yellow, and red phosphors. The meta‐link PPI33PPPBO is not only of smaller π‐conjugation, but also of more ordered face‐to‐face stacking for enhanced and more balanced carrier mobility. As a result, the green, yellow, and red PhOLEDs utilizing PPI33PPPBO as host materials show low turn‐on voltages of 2.8 V. The maximum external quantum efficiency (EQEmax) of the corresponding devices reaches 22.8%, 26.7%, and 17.6%, which is superior to that of the traditional host materials CBP and mCP, showing great application potential. More importantly, when the luminance is 1000 cd m−2, their EQE can still be as high as 21.9%, 25.5%, and 16.4%, corresponding to negligible efficiency roll‐offs of only 3.9%, 4.5%, and 6.8%. To the best of authors knowledge, it is the first time that PBO is applied to PhOLED host materials using a twisted connection method.

Visualization of fast ion phase-space flow in plasmas well-below, near and well-above Alfvén eigenmode stability threshold in tokamak

Transport of fast ions along certain local phase space paths, referred to as fast ion phase-space flow, has been systematically measured by an imaging neutral particle analyzer (INPA) in three plasma regimes, which are well-below, near, and well-above the Alfvén eigenmode stability threshold (Du et al 2021 Phys. Rev. Lett. 127 235002). (1) In plasmas well-below the Alfvén eignenmodes (AE) stability threshold, fast ions are well-confined on passing particle orbits without noticeable transport over the phase space. The observed INPA images agree well with the synthetic INPA images, using the fast ion distribution predicted by neoclassical theory. (2) In plasmas near the AE stability threshold, INPA images in the presence of AE activity moderately deviate from those without AE activity. The image difference can be well interpreted by AE-driven, phase-space fast ion flow. Paths of this flow over the velocity space (or streamlines) are reconstructed by the intersection lines of curved Eʹ and µ surfaces, referred to as Eʹ and µ line (where ; E, P ζ and µ are the energy, canonical toroidal momentum and magnetic moment of ions; ω and n are the angular frequency and toroidal mode number of AEs, respectively). Resonant fast ions move radially inward by gaining energy and move radially outward by losing energy and the trajectory well aligns with the Eʹ and µ lines that pass through the mode resonances near the injection energy of neutral beams. (3) In plasmas well-above the AE stability threshold, fast ion phase-space dynamics shows additional features. Fast ions are transported out of the birth positions so promptly along the streamlines that the slowing-down process from the injection energy is not observable, exhibiting strong critical gradient behavior at local phase space. As a result, the increase of electron temperature is very small, in spite of an increase of beam power by . It should be emphasized that the directions of phase-space transport, induced by AEs with different frequencies, structures and mode numbers, do not largely differ.

Experimental optimization of compact double-cell stimulated Brillouin scattering pulse compressor

To optimize the output of SBS sub-nanosecond pulse compression, two kinds of compact double-cell structures are carried out and compared experimentally. The beam parameters of the compact double-cell structure are calculated theoretically, which provides the selection guidance of structural parameters such as lens focal length and SBS cell size. The dependence of lens parameters and medium parameters on SBS output parameters are experimentally studied. Results show that SBS pulse compression enters the saturation region at a low injection energy with a long focal length lens or a large gain coefficient medium. For compact double-cell setup with one lens, it is easy to obtain narrow pulses for the medium FC40 with a short phonon lifetime. While in setup with two lenses, it is easy to obtain SBS output with a high energy efficiency and narrow pulse width for HT110 medium with a large gain coefficient. The pulse width compression ratio is up to 16 times after optimization. These experimental results can provide references for the experimental design of SBS pulse compression.

An APEX Study of Molecular Outflows in FUor-type Stars

The FU Orionis–type objects (FUors) are low-mass pre-main-sequence objects that go through a short-lived phase (∼100 yr) of increased mass accretion rate (from 10−8 to 10−4 M ⊙ yr−1). These eruptive young stars are in the early stages of stellar evolution and thus still deeply embedded in a massive envelope that feeds material to the circumstellar disk that is then accreted onto the star. Some FUors drive molecular outflows, i.e., low-velocity wide-angle magnetohydrodynamical winds, that inject energy and momentum back to the surrounding envelopes and help clear the material surrounding the young star. Here we present a 12CO (3–2), 13CO (3–2), and 12CO (4–3) survey of 20 FUor-type eruptive young stars observed with APEX. We use our 13CO (3–2) observations to measure the masses of the envelopes surrounding each FUor and find an agreement with the FUor evolutionary trend found from the 10 μm silicate feature. We find outflows in 11 FUors, calculate their masses and other kinematic properties, and compare these with those of outflows found around quiescent young stellar objects gathered from the literature. This comparison indicates that outflows in FUors are more massive than outflows in quiescent sources, and that FUor outflows have a higher-ratio outflow mass with respect to the envelope than the quiescent sample, indicating that the eruptive young stars have lower star-forming efficiencies. Finally, we find that the outflow forces in FUors are similar to those of quiescent young stellar objects, indicating that their accretion histories are similar or that the FUor outflows have lower velocities.

DFT Studies on a Metal Oxide@Graphene-Decorated D-π1-π2-A Novel Multi-Junction Light-Harvesting System for Efficient Dye-Sensitized Solar Cell Applications.

Graphene nanocomposites have emerged as potential photoanode materials for increased performance of the dye-sensitized solar cells (DSSCs) via charge transfer. Various metal-oxide-decorated graphene nanocomposites have widespread applications in energy devices, such as solar cells, fuel cells, batteries, sensors, electrocatalysis, and photocatalysis. However, the possible role of these composites in DSSC applications has largely remained unexplored. Herein, we studied a Sb2O3-decorated graphene-D-π1-π2-A sensitized TiO2 nanocomposite (dye-(TiO2)9/Sb2O3@GO) as a model multi-junction light-harvesting system and examined the impact of various π-bridges on the optical and photovoltaic properties of the push-pull dye system employed in this light-harvesting system. We have shown that by changing the spacer unit, the light sensitivity of nanocomposites can be varied from visible to near-infrared wavelengths. Furthermore, with the integration of metal-oxide-decorated graphene nanocomposites on D-π1-π2-A systems and D-π-A systems, composite photoelectrodes displayed better optical and photovoltaic characteristics with an enhanced absorption spectrum in the wavelength range of 800-1000 nm. The performance of the D-π1-π2-A system has been evaluated in terms of various photovoltaic parameters such as the highest occupied molecular orbital-lowest unoccupied molecular orbital energy gaps, excited-state oxidation potential (E dye *), free energy of electron injection (G inject), total reorganization energy (λtotal), and open-circuit voltage (V oc). This work throws light on the current trends and the future opportunities in graphene-metal oxide nanocomposite-based DSSCs for better harvesting of the solar spectrum and better performance of solar devices.

Generative machine learning-based multi-objective process parameter optimization towards energy and quality of injection molding.

The high energy intensity and rigorous quality demand of injection molding have received significant interest under the background of the soaring production of global plastic industry. As multiple parts can be produced in a multi-cavity mold during one operation cycle, the weight differences of these parts have been demonstrated to reflect their quality performance. In this regard, this study incorporated this fact and developed a generative machine learning-based multi-objective optimization model. Such model can predict the qualification of parts produced under different processing variables and further optimize processing variables of injection molding for minimal energy consumption and weight difference amongst parts in one cycle. Statistical assessment via F1-score and R2 was performed to evaluate the performance of the algorithm. In addition, to validate the effectiveness of our model, we conducted physical experiments to measure the energy profile and weight difference under varying parameter settings. Permutation-based mean square error reduction was adopted to specify the importance of parameters affecting energy consumption and quality of injection molded parts. Optimization results indicated that the processing parameters optimization could reduce ~ 8% energy consumption and ~ 2% weight difference compared with the average operation practices. Maximum speed and first-stage speed were identified as the dominating factors affecting quality performance and energy consumption, respectively. This study could contribute to the quality assurance of injection molded parts and facilitate energy efficient and sustainable plastic manufacturing.

Oxygenated carbon functionalized TiO2 aerogel surface: Facile synthesis, surface, structural and photovoltaic investigations

The present study reports the synthesis of in-situ surface functionalized TiO2 aerogel through microwave-assisted sol-gel method. Glucose was used as a carbon source, and different amounts of oxygenated carbon were inserted on the surface of TiO2 aerogel. The presence of oxygenated carbon on the surface of TiO2 is confirmed by Raman analysis. The microstructural analysis of the materials was performed by Field Emission Scanning Electron Microscope (FESEM) and transmission Electron Microscope (TEM). After doping with COx, the retained porous surfaces were achieved. X-ray Photoelectron Spectroscopy (XPS) indicates an increase in the amount of carbon and oxygen compared to the titanium and oxygen ratio of TiO2. The increase in the peak area of O1s spectra indicates the insertion of different forms of oxygenated carbon. The C1s spectra confirm that various forms of oxygenated carbon, such as –COH, –COOH, CO–C and OC=O, are on the surface of TiO2 aerogel. Due to surface-adsorbed COx, the TACOx samples had extended absorption band edges and reduced band gaps in optical studies. As a result of that, the energy for the electron injection (0.52 eV) was significantly reduced in the TACOx-20% sample. In addition, the BET surface area analysis reveals a high surface area of 144 m2/g for the TACOx-20% sample. Dye adsorption studies also reveal the high dye loading of 0.65 μmol/mg found in the TACOx-20% sample due to more surface hydroxyl groups on the surfaces. The porous network structure, altered optical properties, and the insertion of hydrophilic groups on the surface of COx-doped titania aerogel are beneficial for adsorbing more dye molecules, which are crucial for improving the photovoltaic efficiency of the materials.

Radiation effects of hydrogen beam injection into a boron-11 tokamak plasma

Injection of a hydrogen neutral beam (H) is studied into the boron-11 (11B) fusion tokamak plasma. The conclusions show that the most desirable injection energy of the hydrogen beam, , into pure 11B target plasma is 5 MeV for performing the H11B reaction with the maximum fusion energy multiplication factor (). This factor for decreases with the increase in and increases with the electron temperature. A change in the thermal ion mixture had only a small effect on . decreases when the effect of radiation losses is considered through bremsstrahlung and synchrotron powers . The difference between the curves of and the fusion power is minimized in the ion temperature range 300–400 keV. A higher ion-to-electron temperature ratio is required to obtain higher . increases with an increase in plasma beta. Increasing the ratio of the fusion power to each radiation power can enhance the value.

Design and optimization of an adjustable RF positive hydrogen ion source

An adjustable radio frequency (RF) positive hydrogen ion source is designed in Huazhong University of Science and Technology (HUST) to provide ion beam with adaptive beam current and beam energy for neutral beam injection (NBI) related material research. The ion source aims to produce 10–20 keV positive hydrogen ion beam with total current of 50–125 mA. This paper investigates the design of the RF ion source including RF driver via inductively discharge mechanism and the extractor which is designed and optimized, including ion beam optics simulation, thermal analysis and power supply analysis. The vacuum analysis of the source is carried out as well.

Disc-halo gas outflows driven by stellar clusters as seen in multiwavelength tracers

ABSTRACT We consider the dynamics of and emission from growing superbubbles in a stratified interstellar gaseous disc driven by energy release from supernovae explosions in stellar clusters with masses Mcl = 105 − 1.6 × 106 M⊙. Supernovae are spread randomly within a sphere of rc = 60 pc, and inject energy episodically with a specific rate $1/130~\mathrm{M}_\odot ^{-1}$ proportional to the star formation rate (SFR) in the cluster. Models are run for several values of SFR in the range 0.01 to 0.1 M⊙ yr−1, with the corresponding average surface energy input rate ∼0.04–0.4 erg cm−2 s−1. We find that the discrete energy injection by isolated SNe are more efficient in blowing superbubbles: Asymptotically they reach heights of up to 3 to 16 kpc for Mcl = 105 − 1.6 × 105 M⊙, correspondingly, and stay filled with a hot and dilute plasma for at least 30 Myr. During this time, they emit X-ray, Hα and dust infrared emission. X-ray luminosities LX∝SFR3/5 that we derive here are consistent with observations in star-forming galaxies. Even though dust particles of small sizes a ≤ 0.03 μm are sputtered in the interior of bubbles, larger grains still contribute considerably ensuring the bubble luminosity $L_{\rm IR}/{\rm SFR}\sim 5\times 10^7 \, \mathrm{L}_\odot \, \mathrm{M}_\odot ^{-1} ~{\rm yr}$. It is shown that the origin of the North Polar Spur in the Milky Way can be connected with activity of a cluster with the stellar mass of ∼105 M⊙ and the SFR ∼ 0.1 M⊙ yr−1 some 25–30 Myr ago. Extended luminous haloes observed in edge-on galaxies (NGC 891 as an example) can be maintained by disc spread stellar clusters of smaller masses M* ≲ 105 M⊙.

A quantum chemical study: thoughtful exploration for optimal donors in Y-type dual donor-based dye sensitizers.

This research explores the influence of different dual donors on the effectiveness of dye sensitizers. We selected 35 diverse donors to construct Y-type dual donor-based dyes, connecting them with thiophene as the π-spacer and cyanoacrylic acid as the acceptor. Density functional theory calculations indicate that these dual donor-based dyes exhibit superior optoelectronic properties compared to their single donor counterparts. Notably, significant variations in charge distribution among the different dual donors affect their donor capabilities. Our calculations specifically highlight the enhanced thermodynamic parameters, including light harvesting efficiency (LHE), the free energy of dye injection (ΔGinject), and regeneration (ΔGreg), for donor moieties containing nitrogen atoms, such as NS-3 (N,N-dimethylaniline), NS-5 (diphenylamine), NS-6 (triphenylamine), and NS-8 (4-methoxy-N-(4-methoxyphenyl)-N-phenylaniline). These results suggest that nitrogen-containing donor moieties act as promising candidates for donors for efficient dye sensitizers. However, further experimental validation in the near future will be necessary to confirm our findings.

Improvement of fundamental frequency performance of SGII-UP laser facility

The SGII-UP laser facility is one of the most important high power laser systems in China, and it is also one of a few inertial confinement fusion laser devices that operate all year round in the world. In order to further improve its output capacity to meet higher physical requirements, measures such as increasing the number of neodymium glasses, adopting new N41 neodymium glasses, and improving the energy configuration of xenon lamps are taken to improve the gain capacity of the main amplifier. Calculation of the new main amplifier construction model predicts that the small gain coefficient will reach 4.9%. And further modulation of the laser device shows that when the output of 10 kJ fundamental frequency energy is needed, the injection energy decreases from 5 J to 1.26 J, which supports a higher output energy and a stronger basic frequency output capability. Furthermore, it is analyzed that under different laser pulse injection conditions of 1, 5, 10 ns, the &lt;i&gt;B&lt;/i&gt; integral is obviously reduced, which means that the near-filed quality of the beams is better. According a small-size modulation suppression is induced by nonlinear phase shift, and high-fluence laser is expected to pass before and after the improvement, which is a key prerequisite for a higher output energy. Based on these analyses, fundamental frequency output energy values with different pulse injections are calculated and an improvement from 8 kJ to 12.5 kJ output is expected under 10 ns square pulse condition. Tests show that the small signal gain coefficient of the device increases from 4.15% cm to 4.94% cm, which is consistent with simulation results, and the average gain multiple of a single beam increases from 9000 to 118000, which is an order of magnitude higher. The output verifies the fundamental frequency output capacity exceeding 12.5 kJ under 10 ns square pulse as well as a small-size modulation suppression around 0.16 mm&lt;sup&gt;–1&lt;/sup&gt; as a result of joint action of non-linear phase shift and spatial filtering. After the significant improvement, the SGII-UP laser facility will strongly support more ambitious physical experiment targets.