Magnetic field determination of chromospheric spicules using the Weak Field Approximation

Precession frequency, also known as Larmor frequency, is closely related to the strength of the external magnetic field and can be obtained using the following equation

The axial magnetic effect describes the generation of an energy current parallel to an axial magnetic field B 5 (i.e., a magnetic field coupling with opposite signs to the left

scalar field, which is often called “ “ the the inflaton inflaton field.'' The stage field.'' The stage of inflation can be very short, but the universe within this tim of

As a result we present the temperature dependence of the electronic part of the heat capacity, the magnetic field dependence of the Sommerfeld coefficient, the temperature dependence

This behavior is attributed to the specific order parameter and magnetic field distributions, which favors the formation of superconducting vortices and order

Using a mean field approximation for the network activity we derive relationships between the parameters of the network that ensure that the overall level of activity of the

When we apply a magnetic field above the upper critical field, we do not find any signature for the magnetic impurities. This shows that there is no strong exchange cou- pling

The stellar evolution model of a red giant with 1.7 M  without planet engulfment and with a time-averaged rotation velocity during the main sequence equal to 100 km s −1 shows