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History of Solar Activity Recorded in Polar Ice

History of Solar Activity Recorded in Polar Ice Free Conference is closed

Conference is closed

eawag16

Hosted by Markus Roth

Affiliation Thüringer Landessternwarte Tautenburg

Dübendorf

13.11.2016 - 14.11.2016

Organizing institutions

EAWAG, Dübendorf

Main category Natural Sciences (Astrophysics and Astrononmy)

Conference/Workshop objectives

This Thinkshop will deal with the question whether planets could have any effect on the magnetic activity of the Sun.

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Local organizing committee

Carlo Albert; Jürg Beer; Antonio Ferriz Mas

Scientific organizing committee (SOC)

Carlo Albert

Jürg Beer

Antonio Ferriz Mas

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Sessions

Main Session

Programme

Invited speakers

José Abreu

Jürg Beer

Svetlana Berdyugina

Francesco Berilli

Milan Palus

Markus Roth

Frank Stefani

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Important dates None.

Registration and payment information Registration is closed.

Conference venue Dübendorf

Hotel information

For those of you who need accommodation, we’ve reserved rooms in the Sonnental hotel.

Just mention Carlo Albert and Eawag at the reception.

Travel information

Local transport: The Forum Chriesbach is conveniently located along the Tram Line 12, which connects the airport with the Sonnental hotel (see attached map).

You will need a ticket for Zone 121, for the Tram line 12, and the city Zone 110, for the visit of the accelerator and the dinner.

Depending on when you arrive and leave, a 24h ticket for 3 zones (zone 110 counts double) might be worthwhile.

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Frank Stefani

Session: Main Session

903 views

Date of upload:

15.11.2016

Co-author:

Abstract:

Presentation at EAWAG

Frank Stefani

Session: Main Session

879 views

Date of upload:

15.11.2016

Co-author:

Abstract:

Presentation at EAWAG

Markus Roth

Session: Main Session

905 views

Date of upload:

15.11.2016

Co-author:

Abstract:

This is my talk given at the meeting in Dübendorf.

Carlo Albert

Session: Main Session

1000 views

Date of upload:

15.11.2016

Co-author:

Abstract:

Assuming a simple data-generating model of the type "pure harmonics plus noise" and applying Bayesian inference techniques has two advantages over Fourier analysis: (i) lines that are separated by less than the Fourier resolution might be detected and (ii) the uncertainties of the detected lines can be quantified. If the data stems from the solar activity, inferring the parameters of a stochastic dynamo model might be worthwhile.

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