solar magnetic fieldsolar coronaRainbow topological modelsolar atmosphereprimary energy release/ A9660R Solar flares, bursts, and related phenomena A9660H Solar magnetic and electric fields A9660P Solar coronaA review of current questions related to the problem of large solar flares is given. The ...
[1] Vector magnetometer observations from the Challenging Minisatellite Payload (CHAMP) satellite are used to determine the solar quiet (Sq) current system during the recent solar minimum. Observations from 2006 to 2008 are combined, and after removal of a main field model and accounting for field...
First, the empirical Sq field model by Yamazaki et al. (2011) is analyzed to examine the impact of solar activity and seasonal variations. The results show that Jtotal changes by ±33% with the change of solar radiation activity in one solar cycle and by ±17% with the change of season...
Studies that considered this method of determining lycopene contents demonstrated that the use of the CIELAB model facilitates the calculations and provides high reliability, although the original color model of the sensors is the RGB model. A relevant finding is that the efficiency in the lycopene ...
Explore some of the primary challenges in high-voltage current sensing, with additional resources to aid and simplify your design process. Learn about higher system voltages, increased system protection, telemetry monitoring and reduced form factors. ...
5. For models of the crimping tool and removal wrench, use the recommended model or contact your dealer.6. Connect the PV string connector to the inverter connector, and then pull back the PV string connector along the axial direction to check whether the connectors are securely connected....
We propose an accurate analytical model for the source of hard X-ray emission from a flare in the form of a "thick target" with a reverse current to explain the results of present-day observations of solar flares onboard the GOES, Hinode, RHESSI, and TRACE satellites. The model, one-dim...
The nature of the solar wind-magnetosphere-ionosphere (SW-M-I) coupling has been a subject of intense study and scientific interest. We report results from a numerical simulation of the SW-M-I system which shed light on the physics and behavior of the controlling processes. The current-voltag...
We present a method to model the storm-time magnetospheric magnetic field using representations of the magnetic field arising from the various magnetospheric current systems. We incorporate the effects of magnetotail changes during substorms by introducing an additional localized thin current sheet into th...
The advanced skylight model requires reasonably modern hardware. If you are running e.g. Windows 10 on an Intel Pentium P6100 without dedicated graphics card, graphics mode of version 1.0 (Qt6-based 1.22.3) will only be Mesa, which means all graphics is computed on the main processor. Fur...