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Solving solar puzzle could help save Earth from planet-wide blackouts
space weather prediction convection sunspots
2021/8/5
Understanding the Sun's magnetic dynamo could help predict solar weather, such as potentially dangerous geothermal storms, solar flares and sunspots. Mathematicians have proposed a new model of the Su...
The Solar Wind: Our Current Understanding and How We Got Here
Solar wind coronal holes solar corona cyclotron resonance MHD waves
2010/9/16
In the original theory for the solar wind, the electron pressure gradient was the principal accelerating force. This was soon recognized to be insufficient to drive the high-speed streams. Subsequentl...
Solar eclipse seen over The University of Nottingham（图）
Solar eclipse The University of Nottingham
2009/7/27
Truly breathtaking — fabulous — spectacular. These were just some of the words used by students and members of staff who got an exclusive view of the longest solar eclipse of the century from an Engli...
The mass distribution of secondaries to solar-type stars
solar-type stars mass distribution
2009/6/16
The mass distribution of secondaries to solar-type stars。
Statistical properties of solar-type close binaries。
THE 50-DAY OSCILLATION IN THE EARTH`S ROTATION, ATMOSPHERIC ANGULAR MOMENTUM AND SOLAR ACTIVITY
50-DAY OSCILLATION THE EARTH`S ROTATION ATMOSPHERIC ANGULAR MOMENTUM
2009/4/8
THE 50-DAY OSCILLATION IN THE EARTH`S ROTATION, ATMOSPHERIC ANGULAR MOMENTUM AND SOLAR ACTIVITY。
ASTROMETRIC ASPECT OF 1980 INIDIAN TOTAL SOLAR ECLIPSE
TOTAL SOLAR ECLIPSE ASTROMETRIC ASPECT 1980 INIDIAN
2009/4/3
ASTROMETRIC ASPECT OF 1980 INIDIAN TOTAL SOLAR ECLIPSE。
Interplanetary Shock Parameters during Solar Activity Maximum (2000) and Minimum (1995-1996)
Interplanetary Shock Parameters Solar Activity Maximum
2003/3/31
Interplanetary shock parameters are analyzed for solar maximum (year 2000) and solar minimum (years 1995-1996) activity. Fast forward shocks are the most usual type of shock observed in the interplane...