Results 61 to 70 of about 1,433,455 (143)

Electromagnetic monitoring in seismically active regions of Siberia

Геофизический журнал, 2012
Field data of the electromagnetic monitoring of controlled source have been obtained in two seismically active regions of Siberia. The article demonstrates an approach to the interpretation of regime observations data and it attempts to explain the ...
N. N. Nevedrova, M. I. Epov
doaj   +1 more source

Effects of a twisted magnetic rope at the stage of the appearance of a new active region in the photosphere

Solar-Terrestrial Physics
Using SDO/HMI data, we have studied the dynamics of small-scale magnetic field elements in the photosphere during the formation of small active region USAF/NOAA 12761.
Grigoryev Victor, Ermakova Lyudmila
doaj   +1 more source

Telemedicine Assessment for the Mental Health of Rural Residents Based on the Safety Degree of Housing in Seismically Active Regions. [PDF]

Front Public Health, 2021
Pan Y, Xie R, Yan Q, Zhou T.
europepmc   +1 more source

Light Bridges and Solar Active Region Evolution Processes

The Astrophysical Journal Supplement Series
The formation mechanism of light bridges (LBs) is strongly related to the dynamic evolution of solar active regions (ARs). To study the relationship between LB formation and AR evolution phases, we employ 109 LB samples from 69 ARs in 2014 using ...
Fuyu Li, Changhui Rao, Xinhua Zhao, Yang Guo, Xiaoying Gong, Yuhao Chen, Nanbin Xiang, Huaning Wang   +7 more
doaj   +1 more source

Center-to-limb variations of solar active regions

Astronomy & Astrophysics
Accurate modeling of stellar active regions (ARs) remains a major bottleneck for radial-velocity and transmission-spectroscopy studies aimed at finding Earth-like planets. While much effort has been devoted to AR modeling, their center-to-limb variations
Pietrow A. G. M., Sumra S., Petit dit de la Roche D. J. M., Lößnitz E. J., Denker C., Aßmus M.   +5 more
doaj   +1 more source

Complex Network View of the Sun’s Magnetic Patches. I. Identification

The Astrophysical Journal Supplement Series
Solar and stellar magnetic patches (i.e., magnetic fluxes that reach the surface from the interior) are believed to be the primary sources of a star’s atmospheric conditions. Here, we apply the complex network approach and investigate its efficacy in the
Zahra Tajik, Nastaran Farhang, Hossein Safari, Michael S. Wheatland   +3 more
doaj   +1 more source

STARRPeaker: uniform processing and accurate identification of STARR-seq active regions. [PDF]

Genome Biol, 2020
Lee D, Shi M, Moran J, Wall M, Zhang J, Liu J, Fitzgerald D, Kyono Y, Ma L, White KP, Gerstein M.   +10 more
europepmc   +1 more source

Epstein-Barr Virus Episome Physically Interacts with Active Regions of the Host Genome in Lymphoblastoid Cells. [PDF]

J Virol, 2020
Wang L, Laing J, Yan B, Zhou H, Ke L, Wang C, Narita Y, Zhang Z, Olson MR, Afzali B, Zhao B, Kazemian M.   +11 more
europepmc   +1 more source

ATM-Dependent Recruitment of BRD7 is required for Transcriptional Repression and DNA Repair at DNA Breaks Flanking Transcriptional Active Regions. [PDF]

Adv Sci (Weinh), 2020
Hu K, Li Y, Wu W, Xie L, Yan H, Cai Y, Chen D, Jiang Q, Lin L, Chen Z, Liao JY, Zhang Y, Koeffler HP, Yin D, Song E.   +14 more
europepmc   +1 more source

First Insights into the Applicability and Importance of Different 3D Magnetic Field Extrapolation Approaches for Studying the Preeruptive Conditions of Solar Active Regions

The Astrophysical Journal
The three-dimensional (3D) coronal magnetic field has not yet been directly observed. However, for a better understanding and prediction of magnetically driven solar eruptions, 3D models of solar active regions are required.
Marianna B. Korsós, Robert Jarolim, Robertus Erdélyi, Astrid M. Veronig, Huw Morgan, Francesca Zuccarello   +5 more
doaj   +1 more source