268 research outputs found
Gastrodia elata powder capsule enhances anti-epileptic effect of carbamazepine by decreasing P-gp expression
Purpose: To investigate the influence of Gastrodia elata powder capsule (GC) or gastrodin (GTD) on the anti-epileptic effect of carbamazepine (CBZ) on penicillin (PG)-induced epilepsy in rats.
Methods: A total 116 rats were used in this study. Rats in the control group (n = 8) were injected with normal saline (NS) in place PG. Epilepsy was induced in the remaining 108 rats on the first day via PG injection. The rats were then divided randomly into six groups (18 rats per group): PG group, CBZ group, CBZ + GC group, CBZ + GTD group, GC group, and GTD group, which were given (p.o.) NS, CBZ (100 mg/kg), CBZ (100 mg/kg.) + GC (350 mg/kg), CBZ (100 mg/kg) + GTD (100 mg/kg), GC (350 mg/kg), and GTD (100 mg/kg), respectively, once a day for 15 days. The behavioral characteristics of the rats were observed and used to assess the anti-epileptic effect of the test drugs. Real-time quantitative reverse transcription-PCR and Western blot assays were employed for the determination of the effect of CBZ, GC and GTD on the expression levels of P-gp.
Results: CBZ significantly reduced the symptoms of epilepsy, while GC and GTD enhanced the antiepileptic effect of CBZ, and reversed the CBZ-induced increases in the protein expressions of mrd1a and P-gp (p < 0.05).
Conclusion: GC reverses CBZ drug resistance, probably through downregulation of P-gp expression. This finding indicates that GC is a potential anti-epilepsy drug, but it merits further studies
3D Seismic Sedimentology of Nearshore Subaqueous Fans – A Case Study from Dongying Depression, Eastern China
The Extending of Observing Altitudes of Plasma and Ion Lines During Ionospheric Heating
Source at https://doi.org/10.1002/2017JA024809. The ultrahigh-frequency observation during an ionospheric heating experiment on 11 March 2014 at the European Incoherent Scatter Scientific Association Tromsø site illustrated a remarkable extension of observing altitudes of the enhanced plasma line and the ion line, implying that the enhanced ion acoustic wave and Langmuir wave should satisfy the Bragg condition within the extending altitude range. An analysis shows that the dependence of the wave number of the traveling ion acoustic wave on the profiles of enhanced electron temperature and ion mass, as are expected from the dispersion relation of the ion acoustic wave, leads to the extension of observing altitudes of the enhanced ion line. In addition, the altitude extension of the enhanced plasma line is dependent mainly on the profile of the electron density, although it is not independent of the profile of the electron temperature. Considering a small gradient profile of electron density, however, the enhanced electron temperature, as well as the thermal conduction along the magnetic field, may lead to the altitude extension of the enhanced plasma line
Simultaneous detection of flare-associated kink oscillations and extreme-ultraviolet waves
Kink oscillations, which are frequently observed in coronal loops and
prominences, are often accompanied by extreme-ultraviolet (EUV) waves. However,
much more needs to be explored regarding the causal relationships between kink
oscillations and EUV waves. In this article, we report the simultaneous
detection of kink oscillations and EUV waves that are both associated with an
X2.1 flare on 2023 March 03 (SOL2023-03-03T17:39). The kink oscillations, which
are almost perpendicular to the axes of loop-like structures, are observed in
three coronal loops and one prominence. One short loop shows in-phase
oscillation within the same period of 5.2 minutes at three positions. This
oscillation could be triggered by the pushing of an expanding loop and
interpreted as the standing kink wave. Time lags are found between the kink
oscillations of the short loop and two long loops, suggesting that the kink
wave travels in different loops. The kink oscillations of one long loop and the
prominence are possibly driven by the disturbance of the CME, and that of
another long loop might be attributed to the interaction of the EUV wave. The
onset time of the kink oscillation of the short loop is nearly same as the
beginning of an EUV wave. This fact demonstrates that they are almost
simultaneous. The EUV wave is most likely excited by the expanding loop
structure and shows two components. The leading component is a fast coronal
wave, and the trailing one could be due to the stretching magnetic field lines.Comment: accepted for publication in the Science China Technological Science
Observational signatures of electron-driven chromospheric evaporation in a white-light flare
We investigate observational signatures of explosive chromospheric
evaporation during a white-light flare (WLF) that occurred on 2022 August 27.
Using the moment analysis, bisector techniques, and the Gaussian fitting
method, red-shifted velocities of less than 20 km/s are detected in
low-temperature spectral lines of Ha, C I and Si IV at the conjugated flare
kernels, which could be regarded as downflows caused by chromospheric
condensation. Blue-shifted velocities of about 30-40 km/s are found in the
high-temperature line of Fe XXI, which can be interpreted as upflows driven by
chromospheric evaporation. A nonthermal hard X-ray (HXR) source is co-spatial
with one of the flare kernels, and the Doppler velocities are temporally
correlated with the HXR fluxes. The nonthermal energy flux is estimated to be
at least (1.3+-0.2)*10^10 erg/s/cm^2. The radiation enhancement at Fe I 6569.2
A and 6173 A suggests that the flare is a WLF. Moreover, the while-light
emission at Fe I 6569.2 A is temporally and spatially correlated with the blue
shift of Fe XXI line, suggesting that both the white-light enhancement and the
chromospheric evaporation are triggered and driven by nonthermal electrons. All
our observations support the scenario of an electron-driven explosive
chromospheric evaporation in the WLF.Comment: The manuscript was accepted for publication in ApJ, and it was a part
of the ApJ Focus Issue "Early results from the Chinese Ha Solar Explorer
(CHASE)
Effects of epigallocatechin-3-gallate on bovine oocytes matured
Objective Epigallocatechin-3-gallate (EGCG) is a major ingredient of catechin polyphenols and is considered one of the most promising bioactive compounds in green tea because of its strong antioxidant properties. However, the protective role of EGCG in bovine oocyte in vitro maturation (IVM) has not been investigated. Therefore, we aimed to study the effects of EGCG on IVM of bovine oocytes. Methods Bovine oocytes were treated with different concentrations of EGCG (0, 25, 50, 100, and 200 μM), and the nuclear and cytoplasmic maturation, cumulus cell expansion, intracellular reactive oxygen species (ROS) levels, total antioxidant capacity, the early apoptosis and the developmental competence of in vitro fertilized embryos were measured. The mRNA abundances of antioxidant genes (nuclear factor erythriod-2 related factor 2 [NRF2], superoxide dismutase 1 [SOD1], catalase [CAT], and glutathione peroxidase 4 [GPX4]) in matured bovine oocytes were also quantified. Results Nuclear maturation which is characterized by first polar body extrusion, and cytoplasmic maturation characterized by peripheral and cortical distribution of cortical granules and homogeneous mitochondrial distribution were significantly improved in the 50 μM EGCG-treated group compared with the control group. Adding 50 μM EGCG to the maturation medium significantly increased the cumulus cell expansion index and upregulated the mRNA levels of cumulus cell expansion-related genes (hyaluronan synthase 2, tumor necrosis factor alpha induced protein 6, pentraxin 3, and prostaglandin 2). Both the intracellular ROS level and the early apoptotic rate of matured oocytes were significantly decreased in the 50 μM EGCG group, and the total antioxidant ability was markedly enhanced. Additionally, both the cleavage and blastocyst rates were significantly higher in the 50 μM EGCG-treated oocytes after in vitro fertilization than in the control oocytes. The mRNA abundance of NRF2, SOD1, CAT, and GPX4 were significantly increased in the 50 μM EGCG-treated oocytes. Conclusion In conclusion, 50 μM EGCG can improve the bovine oocyte maturation, and the protective role of EGCG may be correlated with its antioxidative property
Role of Leptin in Mood Disorder and Neurodegenerative Disease
The critical regulatory role of leptin in the neuroendocrine system has been widely reported. Significantly, leptin can improve learning and memory, affect hippocampal synaptic plasticity, exert neuroprotective efficacy and reduce the risk of several neuropsychiatric diseases. In terms of depression, leptin could modulate the levels of neurotransmitters, neurotrophic factors and reverse the dysfunction in the hypothalamic-pituitary-adrenal axis (HPA). At the same time, leptin affects neurological diseases during the regulation of metabolic homeostasis. With regards to neurodegenerative diseases, leptin can affect them via neuroprotection, mainly including Alzheimer’s disease and Parkinson’s disease. This review will summarize the mechanisms of leptin signaling within the neuroendocrine system with respect to these diseases and discuss the therapeutic potential of leptin
Global energetics of solar powerful events on 6 September 2017
Solar flares and coronal mass ejections (CMEs) are thought to be the most
powerful events on the Sun. They can release energy as high as 10^32 erg in
tens of minutes,and could produce solar energetic particles (SEPs) in the
interplanetary space. We explore global energy budgets of solar major eruptions
on 6 September 2017, including the energy partition of a powerful solar flare,
the energy budget of the accompanied CME and SEPs. In the wavelength range
shortward of 222 nm, a major contribution of the flare radiated energy is in
the soft X-ray (SXR) 0.1-7 nm domain. The flare energy radiated at wavelengths
of Ly-alpha and middle ultraviolet is larger than that radiated in the extreme
ultraviolet wavelength, but it is much less than that radiated in the SXR
waveband. The total flare radiated energy could be comparable to the thermal
and nonthermal energies. The energies carried by the major flare and its
accompanied CME are roughly equal, and they are both powered by the magnetic
free energy in the AR NOAA 12673. Moreover, the CME is efficient in
accelerating SEPs, and that the prompt component (whether it comes from the
solar flare or the CME) contributes only a negligible fraction.Comment: accepted for publication in Research in Astronomy and Astrophysic
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