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Polar caps are theme parks. The carousel model of drifting subpulses.

Data: 
Monday, December 5, 2016 - 12:45

On December 7, at 11:15,  we invvite to seminar room (no. 34 in the A2 building).

"The Phenomenon of Drifting Subpulses in the Pulsar Population"

Data: 
Thursday, November 10, 2016 - 17:45

W środę, 16 listopada, o godz. 11:15 w sali 34 (bud. A-2, ul. Szafrana 2) seminarium wygłosi:


wygłosi dr. Rahul Basu (UZ)

Abstract/Streszczenie :

"Recent advances in the theory of pulsar magnetospheres"

Data: 
Friday, November 4, 2016 - 10:00

W środę, 9 listopada, o godz. 11:15 w sali 34 (bud. A-2, ul. Szafrana 2) seminarium wygłosi:

Andrey Timokhin
(NASA Goddard Space Flight Center)
 

Model edukacyjny łazika marsjańskiego

Data: 
Tuesday, May 17, 2016 - 09:30

18.05.2016 o godzinie 11:15 w sali 34 bud. A-2  dr Marek Sendyk wygłosi seminarium:
"Model edukacyjny łazika marsjańskiego".

Streszczenie:

Calibration of fundamental radiative flux scale with nearby eclipsing binaries.

Data: 
Sunday, May 8, 2016 - 20:30

Seminarium IA, środa 11 maja, godzina 11:15, sala 34 (A-2)

Prelegent: Dr Dariusz Graczyk (Universidad de Concepción, Chile)

Seminar:april 6-th, 11:15 am, room 34 (A-2). Speaker: Dr Rauhl Basu, Title: "Unravelling Off-pulse Emission in Pulsars".

Data: 
Tuesday, April 5, 2016 - 17:00

april 6th 2016, 11:15, room 34 w (A-2)

Speaker: Dr Rauhl Basu

Title: "Unravelling Off-pulse Emission in Pulsars".

Abstract:

How to calibrate the RINGO3 polarimeter as well as polarimetric statistical studies of DA and DC spectral types white dwarfs.

Data: 
Monday, February 15, 2016 - 08:30

IA seminar on Wednesday, February 17th at 11:15 a.m., building A-2, room number 34.

Speaker: Dr Agnieszka Słowikowska (IA, UZ)

The shape of a pulsar radio beam: fan beams, not the nested cones. Dr hab. Jarosław Dyks, CAMK PAN, Toruń

Data: 
Tuesday, November 10, 2015 - 08:30

Seminar, Tuesday, November 17th, 14:00, room 34 (A-2),

Abstract: The knowledge of radio emission geometry is crucial for establishing the orientation of their tilted magnetic field, and for interpreting their gamma-ray profiles. I will review the continually increasing evidence against the most popular (nested cone) radio beam geometry. ..........

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