ELFT HÍRADÓ

["Dr. FACSKO Gabor" <facsko.gabor AT wigner.hu>]

Elnézést, új linket küldök.


Gabor FACSKO is inviting you to a scheduled Zoom meeting.


Topic: David2
Time: Oct 20, 2022 10:30 Budapest

Join Zoom Meeting
https://wigner-hu.zoom.us/j/86356293501?pwd=MlFBbmYrRFBRbGVWT3NhVzViSlJkdz09

Meeting ID: 863 5629 3501
Passcode: 351820

2022. 10. 18. 0:57 keltezéssel, Dr. FACSKO Gabor írta:
> Kedves Kollégák, Kedves Listatagok! / Dear Colleagues,
>
> David SIBECK, a NASA Goddard Space Flight Center kutatója "Remotely 
> Sensing the Magnetosphere’s Boundaries" címmel előadást tart a Wigner 
> Fizikai Kutatóközpont 3-as épületének Tanácstermében 2022. október 20. 
> csütörtökön délelőtt 10 óra kezdettel. Az előadás kivonata alább látható
>
> Az előadás nyelve angol és online közvetíteni fogjuk. A belépési 
> kódokat alább közöljük. Külsős érdeklődők a beléptetéssel kapcsolatban 
> keressék meg FACSKÓ Gábort (facsko.gabor AT wigner.hu). Szívesen látunk 
> minden érdeklődőt
>
> ---
>
> On October 20, 2022, at 10:00 we will have a seminar of the Department 
> of Space Physics and Space Technology. David SIBECK, Chief Scientist, 
> Heliophysics Science Division and Mission Scientist will discuss 
> Remotely Sensing the Magnetosphere’s Boundaries. We are going to 
> broadcast the talk. See the Zoom link below.
>
> Outsiders contact Gabor FACSKO (facsko.gabor AT wigner.hu) related to 
> entry to the campus.
>
> Everyone is welcome to the seminar!
>
> Üdvözlettel / Best regards,
> FACSKÓ Gábor
>
> ---
>
> “Remotely Sensing the Magnetosphere’s Boundaries”
>
> Global magnetohydrodynamic models predict that plasma velocities vary 
> almost linearly from 0 km s^−1  at the nose of the stationary 
> magnetopause on the stagnation streamline to a limiting value of 0.25 
> /V/_SW  for high solar wind Alfvénic Mach numbers at the nose of the 
> bow shock, where /V/_SW  is the solar wind velocity. This paper 
> presents a proof-of-concept study showing how two-point measurements 
> of the plasma velocity in the subsolar magnetosheath can be used to 
> determine gradients in the plasma velocity and consequently the 
> steady-state or slowly moving locations of both the nose of the 
> magnetopause and the nose of the bow shock. The results may be of use 
> to those binning magnetosheath observations to develop empirical 
> models, those testing models for magnetopause erosion or deposition in 
> response to magnetic reconnection, and those determining the stand-off 
> distance of the bow shock as a function of solar wind conditions.
>
> ---
>
> Gabor FACSKO is inviting you to a scheduled Zoom meeting.
>
> Join Zoom Meeting
> https://us05web.zoom.us/j/87514620937?pwd=UTU1MWxoVlRGS3ZXQUUyMTRxRW9NZz09
>
> Meeting ID: 875 1462 0937
> Passcode: mTPt9y
>
> --
> Dr. Gabor FACSKO, PhD
> Wigner Research Centre for Physics
> Department of Space Physics and Technology
> H-1121 Budapest, Konkoly-Thege Miklos Road 29-33, Hungary

--
Dr. Gabor FACSKO, PhD
Wigner Research Centre for Physics
Department of Space Physics and Technology
H-1121 Budapest, Konkoly-Thege Miklos Road 29-33, Hungary