Zobrazeno 1 - 10
of 1 329
pro vyhledávání: '"Sanjiv, K"'
Autor:
Anan, Tetsu, Casini, Roberto, Uitenbroek, Han, Schad, Thomas A., Socas-Navarro, Hector, Ichimoto, Kiyoshi, Jaeggli, Sarah A., Tiwari, Sanjiv K., Reep, Jeffrey W., Katsukawa, Yukio, Asai, Ayumi, Qiu, Jiong, Reardon, Kevin P., Tritschler, Alexandra, Wöger, Friedrich, Rimmele, Thomas R.
The efficient release of magnetic energy in astrophysical plasmas, such as during solar flares, can in principle be achieved through magnetic diffusion, at a rate determined by the associated electric field. However, attempts at measuring electric fi
Externí odkaz:
http://arxiv.org/abs/2410.09221
We report seven examples of a long-ignored type of confined solar flare eruption that does not fit the standard model for confined flare eruptions. Because they are confined eruptions, do not fit the standard model, and unexpectedly erupt in ostensib
Externí odkaz:
http://arxiv.org/abs/2408.09021
Publikováno v:
Cell Communication and Signaling, Vol 22, Iss 1, Pp 1-22 (2024)
Abstract Acquired drug resistance is a major challenge in the management of cancer, which underscores the need for discovery and development of novel therapeutic strategies. We report here the mechanism of the anti-cancer activity of a small coordina
Externí odkaz:
https://doaj.org/article/4134644b5c45448bb91c2e3bab582881
Autor:
Tetsu Anan, Roberto Casini, Han Uitenbroek, Thomas A. Schad, Hector Socas-Navarro, Kiyoshi Ichimoto, Sarah A. Jaeggli, Sanjiv K. Tiwari, Jeffrey W. Reep, Yukio Katsukawa, Ayumi Asai, Jiong Qiu, Kevin P. Reardon, Alexandra Tritschler, Friedrich Wöger, Thomas R. Rimmele
Publikováno v:
Nature Communications, Vol 15, Iss 1, Pp 1-9 (2024)
Abstract The efficient release of magnetic energy in astrophysical plasmas, such as during solar flares, can in principle be achieved through magnetic diffusion, at a rate determined by the associated electric field. However, attempts at measuring el
Externí odkaz:
https://doaj.org/article/1c1ccbb820d44227aa9c3624f67db35a
We propose that coronal heating in EUV coronal plumes is weaker, not stronger, than in adjacent non-plume coronal magnetic funnels. This expectation stems from (i) the observation that an EUV plume is born as the magnetic flux at the foot of the plum
Externí odkaz:
http://arxiv.org/abs/2303.00097
Autor:
Sterling, Alphonse C., Moore, Ronald L., Panesar, Navdeep K., Samanta, Tanmoy, Tiwari, Sanjiv K., Savage, Sabrina L.
Solar coronal jets are frequently occurring collimated ejections of solar plasma, originating from magnetically mixed polarity locations on the Sun of size scale comparable to that of a supergranule. Many, if not most, coronal jets are produced by er
Externí odkaz:
http://arxiv.org/abs/2302.13179