Space Group Department of Physics Umeå University

8
Space Group Department of Physics Umeå University Staff: Kjell Rönnmark, prof. Patrik Norqvist, lektor Maria Hamrin, lektor Annie Reiniusson, doktorand Jörgen Vedin, doktorand Niklas Melander, exjobbare

description

Space Group Department of Physics Umeå University. Staff: Kjell Rönnmark, prof. Patrik Norqvist, lektor Maria Hamrin, lektor Annie Reiniusson, doktorand Jörgen Vedin, doktorand Niklas Melander, exjobbare. Current research topics. - PowerPoint PPT Presentation

Transcript of Space Group Department of Physics Umeå University

Page 1: Space Group Department of Physics Umeå University

Space Group

Department of PhysicsUmeå UniversityStaff:

Kjell Rönnmark, prof.Patrik Norqvist, lektorMaria Hamrin, lektor

Annie Reiniusson, doktorandJörgen Vedin, doktorand

Niklas Melander, exjobbare

Page 2: Space Group Department of Physics Umeå University

Current research topics

Tracking down the (auroral) generator and load regions Maria Hamrin, Octav Marghitu (MPI-Garching & Bucharest), …

Method development, GALS Maria Hamrin, Kjell Rönnmark, Jörgen Vedin.

Numerical simulations of auroral flux tubesJörgen Vedin, Kjell Rönnmark.

Small scale density gradients, FrejaAnnie Reiniusson, Gabriella Stenberg, Patrik Norqvist, Kjell Rönnmark, …

Small scale density gradients, Cluster Patrik Norqvist, Gabriella Stenberg, …

Bonus project 1: Cluster passage of reconnection separatricesMaria Hamrin, Gabriella Stenberg, …

Bonus project 2: Calibration of IMA, Mars ExpressNiklas Melander, Maria Hamrin, Patrik Norqvist, Rickard Lundin, …

Hamrin, Uppsala, May 2006

Page 3: Space Group Department of Physics Umeå University

Generator and load regions in the plasma sheet (Cluster+FAST)

Earlier study on auroral generator (Cluster + FAST).

Now: Cluster plasma sheet crossings, fall 2001.

E·J signatures → concentrated loads and generators found (CLR, CGR).

CLR more common. Often close to the neutral sheet.

CGR often in PSBL.

Good agreement with simulations (Birn & Hesse 2005).

Many future prospects…

Page 4: Space Group Department of Physics Umeå University

GALS: Gradient Analysis by Least Squares

Method for reconstructing the (B-) field and its gradients at an arbitrary point in space-time by using multi-spacecraft observations.

Current density from Ampere’s law.

Not very sensitive to the s/c configuration.

Comparable or better than the Curlometer.

Hamrin, Uppsala, May 2006

L=100kmW=20km

Page 5: Space Group Department of Physics Umeå University

Reasonable measures of quality.

Hamrin, Uppsala, May 2006

Page 6: Space Group Department of Physics Umeå University

Numerical simulations of auroral flux tubes

Numerical model: auroral current circuit.

Electrons both modeled as fluid and individual particles (→temperature).

Driving mechanism: applied generator in the equatorial magnetotail → Alfvén waves propagating towards the ionosphere.

Electrons are strongly heated (parallel and perpendicularly) in the acceleration region.

The model explains how field-aligned potential drops of several kV are supported by gradients in the electron temperature (pressure).

Hamrin, Uppsala, May 2006

Page 7: Space Group Department of Physics Umeå University

Small scale density gradients, Freja + Cluster

Previous studies: increased E in lower hybrid cavities.

Now: increased E and B is found on irregular small scale density gradients.

More electrostatic waves (E/B bigger) on sharp gradients.

Dens

Grad Dens

ΣSE

SE

SB

ΣSB

Cluster data confirms this.

Page 8: Space Group Department of Physics Umeå University

Bonus projects

Bonus project 1:Cluster passage of the separatrices of a distant reconnection site.

Bonus project 2: Calibration of IMA, Mars Express..

Hamrin, Uppsala, May 2006