Showing 101 - 120 results of 164 for search 'Halo 2', query time: 0.25s Refine Results
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    Z. Ivinskis: the first objective researcher of St. Casimir's life by Jonas Boruta

    Published 1997-12-01
    “…This in no way tarnished the halo of St. Casimir. On the contrary, the research of Z. …”
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    Effects of H^{−} low beam irradiation and high field pulsing tests in different metals by C. Serafim, S. Calatroni, F. Djurabekova, R. Peacock, V. Bjelland, A. T. Perez-Fontenla, W. Wuensch, A. Grudiev, S. Sgobba, A. Lombardi, E. Sargsyan

    Published 2025-01-01
    “…This paper focuses on the results with CuCr1Zr, CuBe2, SS316LN, and Ta, complementing and expanding previous work exploring Cu-OFE, Nb, and Ti6Al4V.…”
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    Space Weather Monitor at the L5 Point: A Case Study of a CME Observed with STEREO B by L. Rodriguez, C. Scolini, M. Mierla, A. N. Zhukov, M. J. West

    Published 2020-10-01
    “…We test the performance of L5 for space weather monitoring using STEREO B observations of an Earth‐directed coronal mass ejection (CME), seen as a partial halo by SOHO at L1. STEREO B (located close to L5) continuously tracked the CME. …”
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    Novel thiazolyl-pyrimidine derivatives as potential anticancer agents: Synthesis, biological evaluation, and molecular docking studies by Tariq Z. Abolibda, Abdel-Aziz A.A. El-Sayed, Basant Farag, Magdi E.A. Zaki, Abdulwahed Alrehaily, Hossein M. Elbadawy, Ahmad A. Al-Shahri, Saleh R. Alsenani, Sobhi M. Gomha

    Published 2025-01-01
    “…These were created by reacting 2-(1-(6-methyl-2-oxo-4-phenyl- 1,2,3,4-tetrahydropyrimidin-5-yl)ethylidene)hydrazine-1-carbothioamide with hydrazonoyl halides and α-halo compounds, with structures confirmed by spectroscopy. …”
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    Quasi-parallel Antisunward-propagating Whistler Waves Associated with the Electron Deficit in the Near-Sun Solar Wind: Particle-in-cell Simulation by Alfredo Micera, Daniel Verscharen, Jesse T. Coburn, Maria Elena Innocenti

    Published 2025-01-01
    “…In situ observations of the solar wind have shown that the electron velocity distribution function (VDF) consists of a quasi-Maxwellian core, comprising most of the electron population, and two sparser components: the halo, which are suprathermal and quasi-isotropic electrons, and an escaping beam population, the strahl. …”
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    BST1047+1156: A (Failing) Ultradiffuse Tidal Dwarf in the Leo I Group by J. Christopher Mihos, Patrick R. Durrell, Aaron E. Watkins, Stacy S. McGaugh, John Feldmeier

    Published 2024-01-01
    “…Finally, in the environment surrounding BST1047, our imaging also reveals the old, metal-poor ([ M/H ] = − 1.3 ± 0.2) stellar halo of M96 at a projected radius of 50 kpc.…”
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  13. 113

    Midkine: A Novel Biomarker to Predict Malignancy in Patients with Nodular Thyroid Disease by Fatih Kuzu, Dilek Arpaci, Mustafa Unal, Ayfer Altas, Gürkan Haytaoglu, Murat Can, Figen Barut, Furuzan Kokturk, Sevil Uygun Ilikhan, Taner Bayraktaroglu

    Published 2016-01-01
    “…Both SMK and NMK were found to be higher in hypoechoic nodules with an irregular border and without a halo (p<0.05). Serum MK levels were significantly higher in nodules with microcalcifications than nodules with macrocalcification or without calcification (p=0.001). …”
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    Stress-relieving plant growth-promoting bacterial co-inoculation enhances nodulation and nitrogen uptake in black gram under nitrogen-free saline conditions by Praveen Kumar Tiwari, Praveen Kumar Tiwari, Anchal Kumar Srivastava, Rachana Singh, Alok Kumar Srivastava

    Published 2025-01-01
    “…Non-halophytic plants are highly susceptible to salt stress, but numerous studies have shown that halo-tolerant microorganisms can alleviate this stress by producing phytohormones and enhancing nutrient availability. …”
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    Baryon Pasting the Uchuu Light-cone Simulation by Erwin T. Lau, Daisuke Nagai, Arya Farahi, Tomoaki Ishiyama, Hironao Miyatake, Ken Osato, Masato Shirasaki

    Published 2025-01-01
    “…These BP-Uchuu maps are constructed using more than 75 million dark matter halos with masses M _500 _c ≥ 10 ^13 M _⊙ within the redshift range 0 ≤ z ≤ 2. …”
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    Modeling the Saddle-like GeV–TeV Spectrum of HESS J1809–193: Gamma Rays Arising from Reverse-shocked Pulsar Wind Nebula? by Jiaxu Sun, Yang Chen, Yiwei Bao, Xiao Zhang, Xin Zhou

    Published 2025-01-01
    “…The gamma-ray emission from the escaped electrons can account for the TeV spectrum of component A of HESS J1809–193 or the TeV halo, while the electrons remaining after disruption can account for the GeV spectrum of J1810.3–1925e. …”
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