With the rapid development of cold atom physics and quantum optics,Quantum Precision M easurement(QPM)is becoming a more and more active research field.An extreme high measurement precision and sensitivity could be
The equation of magnetostatic equilibrium of a plasma in a uniform gravity field is applied widely in solar physics. Many phenomena in the solar atmosphere such as sunspots, quiescent prominences and various other hro...The equation of magnetostatic equilibrium of a plasma in a uniform gravity field is applied widely in solar physics. Many phenomena in the solar atmosphere such as sunspots, quiescent prominences and various other hromospheric, and coronal structures can last several hours to several days. Hence, they can be studied approximately by using a model of magnetostatic equilibrium of which the equation展开更多
The equation of magnetostatic equilibrium of plasma is widely applied in solar physics, with which many phenomena in the solar physics (for example, the sunspots, the quiescent prominences) can be treated approximatel...The equation of magnetostatic equilibrium of plasma is widely applied in solar physics, with which many phenomena in the solar physics (for example, the sunspots, the quiescent prominences) can be treated approximately. Low has discussed the magnetostatic equilibrium of a two-dimensional plasma with non-identical temperature in a uniform gravity field, and studied the structure of the quiescent展开更多
文摘With the rapid development of cold atom physics and quantum optics,Quantum Precision M easurement(QPM)is becoming a more and more active research field.An extreme high measurement precision and sensitivity could be
文摘The equation of magnetostatic equilibrium of a plasma in a uniform gravity field is applied widely in solar physics. Many phenomena in the solar atmosphere such as sunspots, quiescent prominences and various other hromospheric, and coronal structures can last several hours to several days. Hence, they can be studied approximately by using a model of magnetostatic equilibrium of which the equation
文摘The equation of magnetostatic equilibrium of plasma is widely applied in solar physics, with which many phenomena in the solar physics (for example, the sunspots, the quiescent prominences) can be treated approximately. Low has discussed the magnetostatic equilibrium of a two-dimensional plasma with non-identical temperature in a uniform gravity field, and studied the structure of the quiescent