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Chinese solar telescope reveals acceleration of magnetic reconnection


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IMAGE: Two groups of fibrils, marked L2 and L4, converge and reconnect with each other. Two sets of newly formed fibrils, marked L1 and L3, then appear and retract from the.
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Credit: LI Leping
Magnetic reconnection refers to the reconfiguration of magnetic field geometry. It plays an elemental role in the rapid release of magnetic energy and its conversion to other forms of energy in magnetized plasma systems throughout the universe.
Researchers led by Dr. LI Leping from the National Astronomical Observatories of the Chinese Academy of Sciences (NAOC) analyzed the evolution of magnetic reconnection and its nearby filament. The result suggested that reconnection is significantly accelerated by the propagating disturbance caused by the adjacent filament eruption. ....

Hardi Peter , Max Planck Institute For Solar System Research , Atmospheric Imaging Assembly , National Astronomical Observatories , Chinese Academy , Astrophysical Journal , New Vacuum Solar Telescope , Fuxian Solar Observatory , Yunnan Astronomical Observatories , Magnetic Imager , Solar Dynamic Observatory , Max Planck Institute , Solar System Research , Space Planetary Science , ஹார்டி பீட்டர் , வளிமண்டலம் இமேஜிங் சட்டசபை , தேசிய வானியல் அவதானிப்புகள் , சீன கலைக்கழகம் , வானியற்பியல் இதழ் , புதியது வெற்றிடம் சூரிய தொலைநோக்கி , யுன்னன் வானியல் அவதானிப்புகள் , காந்த இமேஜர் , சூரிய மாறும் கண்காணிப்பு , சூரிய அமைப்பு ஆராய்ச்சி , இடம் கிரகங்கள் அறிவியல் ,

Messier 106 in Canes Venatici - Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets, Telescopes


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Messier 106 is a spiral galaxy lying 22 million light-years from Earth in the constellation Canes Venatici. It is a Seyfert galaxy with an active nucleus emitting radio waves and X-rays due to presence of a supermassive black hole actively consuming matter within its core. Violent churning of spiral arms, dust clouds, and sprays of ionized hydrogen can be seen revolving around the nucleus. The the irregular galaxy to its lower left is UGC7356 which lies at a similar distance and the edge on spiral galaxy to its lower right is NGC 4248 which lies 24 million light-years away. Other faint, distant galaxies can be seen scattered around the image. ....

United States , Celestron Compustar , Pommier Observatory , Amateur Astronomy , Amature Astronomy , Astronomy Magazine , Astronomy Mag , Astronomy Charts , Big Bang , Black Hole , Cosmic Microwave Background , Cosmic Ray , Dark Adaption , Dark Adaptation , Dark Sky , Deep Sky , Drift Method , Earth Like , Finder Scope , Field Of View , F Ratio , Gamma Ray , Go To , Interactive Star Chart , Kuiper Belt , Kuyper Belt ,

vdB 80 - Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets, Telescopes


Luminance – 12x600s – 120 minutes – binned 1x1
RGB – 6x300s – 30 minutes each – binned 2x2
210 minutes total exposure – 3 hours 30 minutes
Imaged on March 3rd, 2021 at the Danville Conservation Area (New Florence, Missouri) with a SBIG ST-8300M on an Astro-Tech AT90EDT at f/6.7 603mm.
LRGB - https://www.flickr.com/photos/dcrowson/51010577911/sizes/l/
Comments ....

United States , Danville Conservation Area , New Florence , Amateur Astronomy , Amature Astronomy , Astronomy Magazine , Astronomy Mag , Astronomy Charts , Big Bang , Black Hole , Cosmic Microwave Background , Cosmic Ray , Dark Adaption , Dark Adaptation , Dark Sky , Deep Sky , Drift Method , Earth Like , Finder Scope , Field Of View , F Ratio , Gamma Ray , Go To , Interactive Star Chart , Kuiper Belt , Kuyper Belt ,