Is this you? As a journalist, you can create a free Muck Rack account to customize your profile, list your contact preferences, and upload a portfolio of your best work.
Claim your profile
Articles by M Yu
Study of Resonance Production in the Multiparticle Exclusive $K^{-}p$ Channels at 32 GeV/c
Title Study of Resonance Production in the Multiparticle Exclusive $K^{-}p$ Channels at 32 GeV/c Author(s) Bogolyubsky, M Yu (Serpukhov, IHEP) ; Bryzgalov, V V (Serpukhov, IHEP) ; Kotova, A I (Serpukhov, IHEP) ; Kiseleva, S G (Serpukhov, IHEP) ; Levitsky, M S (Serpukhov, IHEP) ; Moiseev, A M (Serpukhov, IHEP) ; Patalakha, D I (Serpukhov, IHEP) ; Gensch, U (DESY, Zeuthen) ; Macnaughton, J (Vienna, OAW) Collaboration CERN-USSR Imprint 1983. - 8 p. In: Z. Phys.
Risk Factors associated with Hypertensive Disorders of Pregnancy within an Urban Indigenous Population in South Western Sydney
The prevalence of hypertensive disorders of pregnancy (HDP) in Australia's urban Indigenous women is unknown. To explore the risk factors associated with HDP for a cohort of urban Indigenous women in South-Western Sydney, Australia This study was conducted in partnership with the Tharawal Aboriginal Medical Service (TAMS). Women (18-45 years) were recruited at the clinic and community events. The quantitative questionnaire included obstetric history, personal and family history of hypertension.
Interaction of CME/ICME with HSS solar wind from coronal holes: case study
In this paper we look for traces of interaction of CME/ICME with high-speed stream (HSS) of solar wind from coronal hole (CH) for two serial Carrington rotations (CRs) during December 2011 - January 2012. We analyze two cases. (1) In CR 2118 instead of predicted arrival of HSS the signatures of ICME with modified back side and compressed slow stream were observed. (2) In CR 2119 the predicted HSS was observed in time, and after arrival of preceding ICME.
CERN Document Server
The paper presents the solutions for the two-beam reduction of the dense soliton gas equations (or Born-Infeld equation) obtained by analytical and numerical methods. The method proposed by the authors is used. This method allows to reduce the Cauchy problem for two hyperbolic quasilinear PDEs to the Cauchy problem for ODEs. In some respect, this method is analogous to the method of characteristics for two hyperbolic equations.
CERN Document Server
The inverse solution of the 1D Parker dynamo equations is considered. The method is based on minimization of the cost-function, which characterize deviation of the model solution properties from the desired ones. The output is the latitude distribution of the magnetic field generation sources: the $\alpha$- and $\omega$-effects. Minimization is made using the Monte-Carlo method.
Show More
loading
Actions
Is this you?
As a journalist, you can create a free Muck Rack account to customize your profile, list your contact preferences, and upload a portfolio of your best work.Get in touch with M
Contact M, search articles and posts on X, monitor coverage, and track replies from one place.
Learn more about Muck Rack