Zobrazeno 1 - 10
of 4 333
pro vyhledávání: '"INTERPLANETARY SCINTILLATION"'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Waszewski, A., Morgan, J. S., Chhetri, R., Ekers, R., Cheung, M. C. M., Bhat, N. D. R, Johnston-Hollitt, M.
We have conducted a blind search in 49 consecutive days of interplanetary scintillation observations made by the Murchison Widefield Array from mid-2019, with overlapping daily observations approximately East and South-East of the Sun at an elongatio
Externí odkaz:
http://arxiv.org/abs/2309.10349
Autor:
Tokumaru, Munetoshi1 (AUTHOR) tokumaru@isee.nagoya-u.ac.jp, Nagai, Miho1 (AUTHOR), Fujiki, Ken'ichi1 (AUTHOR), Iwai, Kazumasa1 (AUTHOR)
Publikováno v:
Solar Physics. Nov2023, Vol. 298 Issue 11, p1-21. 21p.
Autor:
Tiburzi, C., Jackson, B. V., Cota, L., Shaifullah, G. M., Fallows, R. A., Tokumaru, M., Zucca, P.
Publikováno v:
AdSpR (2022)
Solar-wind 3-D reconstruction tomography based on interplanetary scintillation (IPS) studies provides fundamental information for space-weather forecasting models, and gives the possibility to determine heliospheric column densities. Here we compare
Externí odkaz:
http://arxiv.org/abs/2306.07451
The effect of interplanetary plasma on pulsed pulsar radiation passing through is considered. The pulses of two rotating radio transients (J0609+16, J1132+25) and a pulsar (B0320+39) detected on the Large Phased Array (Pushchino observatory) were ana
Externí odkaz:
http://arxiv.org/abs/2305.07422
We have shown previously that the Murchison Widefield Array (MWA), can detect hundreds of Interplanetary Scintillation (IPS) sources simultaneously across a field of view $\sim30^\circ$ in extent. To test if we can use this capability to track helios
Externí odkaz:
http://arxiv.org/abs/2303.09134
Observations of interplanetary scintillation (IPS - the scintillation of compact radio sources due to density variations in the solar wind) enable the velocity of the solar wind to be determined, and its bulk density to be estimated, throughout the i
Externí odkaz:
http://arxiv.org/abs/2210.02135
Autor:
Iwai, Kazumasa, Fallows, Richard A., Bisi, Mario M., Shiota, Daikou, Jackson, Bernard V., Tokumaru, Munetoshi, Fujiki, Ken'ichi
Interplanetary scintillation (IPS) is a useful tool for detecting coronal mass ejections (CMEs) throughout interplanetary space. Global magnetohydrodynamic (MHD) simulations of the heliosphere, which are usually used to predict the arrival and geo-ef
Externí odkaz:
http://arxiv.org/abs/2209.12486
Autor:
Chhetri, Rajan, Morgan, John, Moss, Vanessa, Ekers, Ron, Scott, Danica, Bannister, Keith, Day, Cherie K., Deller, Adam T., Shannon, Ryan M.
We report on a measurement of interplanetary scintillation (IPS) using the Australian Square Kilometre Array Pathfinder (ASKAP) radio telescope. Although this proof-of-concept observation utilised just 3 seconds of data on a single source, this is no
Externí odkaz:
http://arxiv.org/abs/2208.04981
Understanding the mechanism(s) of the solar wind acceleration is important in astrophysics and geophysics. A promising model of the solar wind acceleration is known as the wave/turbulence-driven (WTD) model, in which Alfv\'en waves feed energy to the
Externí odkaz:
http://arxiv.org/abs/2202.10768