scholarly journals Mexican Virtual Solar Observatory project

2006 ◽  
Vol 2 (14) ◽  
pp. 613-613
Author(s):  
Alfredo J. Santillán ◽  
Liliana Hernández ◽  
Guillermo Salas ◽  
Antonio Sánchez ◽  
Alejandro González ◽  
...  
Keyword(s):  
Numerical Simulations ◽  
Present State ◽  
Active Regions ◽  
Solar Observatory ◽  
Software Environment ◽  
The World ◽  
Solar Active Regions ◽  
Working Together ◽  
National Effort ◽  
Existing Data

The Virtual Solar Observatory (VSO) concept outlines a software environment for searching, obtaining and analyzing data from archives of solar data that are distributed at many different observatories around the world (Hill 2006, in this volume). The VSO, however, not only provides fast and reliable access to the existing data of Solar Active Regions, but also represents a powerful and unique tool to perform numerical simulations of the evolution and present state of solar phenomena. Two centers at UNAM, the Institute of Astronomy (IA) and the Supercomputer Center (DGSCA), along with the Sonora University, are working together to create the Mexican Virtual Solar Observatory (MVSO) that will be part of a wider national effort.

scholarly journals Validating Time‐Distance Far‐Side Imaging of Solar Active Regions through Numerical Simulations

2008 ◽  
Vol 689 (2) ◽  
pp. 1373-1378 ◽  
Author(s):  
Thomas Hartlep ◽  
Junwei Zhao ◽  
Nagi N. Mansour ◽  
Alexander G. Kosovichev
Keyword(s):  
Numerical Simulations ◽  
Active Regions ◽  
Solar Active Regions ◽  
Time Distance

Radio Measurements of Coronal Magnetic Fields

1994 ◽  
Vol 144 ◽  
pp. 21-28 ◽  
Author(s):  
G. B. Gelfreikh
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Solar Corona ◽  
Active Regions ◽  
High Sensitivity ◽  
Coronal Magnetic Field ◽  
Transverse Magnetic ◽  
Radio Sources ◽  
Radio Waves ◽  
Solar Active Regions

AbstractA review of methods of measuring magnetic fields in the solar corona using spectral-polarization observations at microwaves with high spatial resolution is presented. The methods are based on the theory of thermal bremsstrahlung, thermal cyclotron emission, propagation of radio waves in quasi-transverse magnetic field and Faraday rotation of the plane of polarization. The most explicit program of measurements of magnetic fields in the atmosphere of solar active regions has been carried out using radio observations performed on the large reflector radio telescope of the Russian Academy of Sciences — RATAN-600. This proved possible due to good wavelength coverage, multichannel spectrographs observations and high sensitivity to polarization of the instrument. Besides direct measurements of the strength of the magnetic fields in some cases the peculiar parameters of radio sources, such as very steep spectra and high brightness temperatures provide some information on a very complicated local structure of the coronal magnetic field. Of special interest are the results found from combined RATAN-600 and large antennas of aperture synthesis (VLA and WSRT), the latter giving more detailed information on twodimensional structure of radio sources. The bulk of the data obtained allows us to investigate themagnetospheresof the solar active regions as the space in the solar corona where the structures and physical processes are controlled both by the photospheric/underphotospheric currents and surrounding “quiet” corona.

On the nature of microwave pulsations from solar active regions

2003 ◽  
Vol 8 (5-6) ◽  
pp. 136-139
Author(s):  
G.B. Gelfreikh ◽  
◽  
Y.T. Tsap ◽  
Y.G. Kopylova ◽  
L.I. Tsvetkov ◽  
...  
Keyword(s):  
Active Regions ◽  
Solar Active Regions

A Study of the Evolution of Solar Active Regions for Improving Solar Flare Forecasts

1989 ◽  
Author(s):  
Patricia L. Bornmann ◽  
Darren Kalmbach ◽  
David Kulhanek ◽  
April Casale
Keyword(s):  
Solar Flare ◽  
Active Regions ◽  
Solar Active Regions

scholarly journals A New Transmission Route for the Propagation of the SARS-CoV-2 Coronavirus

Biology ◽  
2020 ◽  
Vol 10 (1) ◽  
pp. 10
Author(s):  
Antoine Danchin ◽  
Tuen Wai Ng ◽  
Gabriel Turinici
Keyword(s):  
Compartmental Model ◽  
Transmission Route ◽  
Future Trends ◽  
Prevention Measures ◽  
Public Records ◽  
Specific Strategy ◽  
Virus Tropism ◽  
The World ◽  
Novel Coronavirus ◽  
Existing Data

Background: Starting late 2019, a novel coronavirus spread from the capital of the Hubei province in China to the rest of the country, then to most of the world. To anticipate future trends in the development of the pandemic, we explore here, based on public records of infected persons, how variation in the virus tropism could end up in different patterns, warranting a specific strategy to handle the epidemic. Methods: We use a compartmental model to describe the evolution of an individual through several possible states: susceptible, infected, alternative infection, detected, and removed. We fit the parameters of the model to the existing data, taking into account significant quarantine changes where necessary. Results: The model indicates that Wuhan quarantine measures were effective, but that alternative virus forms and a second propagation route are compatible with available data. For the Hong Kong, Singapore, and Shenzhen regions, the secondary route does not seem to be active. Conclusions: Hypotheses of an alternative infection tropism (the gut tropism) and a secondary propagation route are discussed using a model fitted by the available data. Corresponding prevention measures that take into account both routes should be implemented to the benefit of epidemic control.

State variables for solar active regions

2003 ◽  
Vol 22 (1) ◽  
pp. 75-79
Author(s):  
S. Krasotkin ◽  
O. Chumak ◽  
E. Kononovich
Keyword(s):  
Active Regions ◽  
State Variables ◽  
Solar Active Regions
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