Presentation is loading. Please wait.

Presentation is loading. Please wait.

Energy Conversion in the Auroral Magnetosphere O. Marghitu (1, 2), M. Hamrin (3), B.Klecker (1) M. André (4), S. Buchert (4), J. McFadden (5), H. Vaith.

Similar presentations


Presentation on theme: "Energy Conversion in the Auroral Magnetosphere O. Marghitu (1, 2), M. Hamrin (3), B.Klecker (1) M. André (4), S. Buchert (4), J. McFadden (5), H. Vaith."— Presentation transcript:

1 Energy Conversion in the Auroral Magnetosphere O. Marghitu (1, 2), M. Hamrin (3), B.Klecker (1) M. André (4), S. Buchert (4), J. McFadden (5), H. Vaith (1), (1) Max-Planck-Institut für extraterrestrische Physik, Garching, Germany (2) Institute for Space Sciences, Bucharest, Romania (3) Physics Department, Umeå University, Sweden (4) Swedish Institute of Space Physics, Uppsala, Sweden (5) Space Sciences Lab., University of California at Berkeley, USA DPG – AEF Spring Meeting, Berlin, March 4, 2005

2 Outline AMotivation BEvent on September 20, 2001: Conjunction geometry CEvent study: Data, EJ signature DSummary and prospects

3  There is a significant number of theoretical studies on the auroral generator region: Analytical => e.g. Rostoker and Boström, 1976 Semi-analytical => e.g. Lysak, 1985, Vogt et al., 1999 Numerical simulations => e.g. Birn et al, 1996, Birn and Hesse, 1996 A Motivation A  However, to our knowledge, the experimental investigations of the generator region are missing, as far as the evaluation of EJ is concerned: The one s/c missions before Cluster could not fully resolve J Both J and (mainly) E are close to the instrumental detection limit

4 The energy flux of a strong aurora, ~10 -2 W/m 2, maps to ~10 -5 W/m 2 in the tail (mapping factor ~1000). If the generator region extends 10 7 – 10 8 m along the magnetic field line, the power density is ~10 -13 – 10 -12 W/m 3. A Motivation A

5 B Conjunction Geometry B Cluster in the tail, at ~20R E ; FAST above the auroral oval, at ~0.5R E

6 B Conjunction Geometry B No ground optical data. No optical data from IMAGE or Polar.

7 C Event Study: Data C 16 mW/m 2 1 mW/m 2

8 C Event Study: EJ C EJ  5 10 -13 The signature EJ < 0 not seen in EFW, because it comes mainly form Cluster 1, where ASPOC is off.

9 D Summary and Prospects D  First experimental evidence for the crossing of an auroral generator region.  The signature in E J consistent with the order of magnitude estimate.  Extension of the time interval to 5h => includes two additional conjunctions with FAST  Potential for a statistical investigation of several events in September – October 2001.  Potential for application to other generator regions (LLBL,...)


Download ppt "Energy Conversion in the Auroral Magnetosphere O. Marghitu (1, 2), M. Hamrin (3), B.Klecker (1) M. André (4), S. Buchert (4), J. McFadden (5), H. Vaith."

Similar presentations


Ads by Google